PHYSICO-CHEMICAL METHODS BY DR. J. TRAUBE, PRIVATDOCENT IN THE TECHNICAL HICTT SCHOOL OF BERLIN AUTHORIZED TRANSLATION s BY WILLETT L. HARDIN, Ph.D., HARRISON SENIOR FELLOW IN CHEMISTRY, UNIVERSITY OF PENNSYLVANIA ICUtb ffilustrations PHILADELPHIA P. BLAKISTON’S SON & CO. 1012 WALNUT STREET 1898 Copyright, 1898, by P. Blakiston’s Son & Co. Press of Wm. F. Fell & Co., 1220-24 Sansom St., PHILADELPHIA. PREFACE. In the preface to the German edition the author calls attention to the ever-widening application of physico-chemical methods in the various branches of chemistry. He says the vapor density, melting point, boiling point, and specific gravity are no longer the only constants the determination of which is necessary in organic chemistry. The electric conductivity, specific refraction, thermal constants, depression of the freezing point and vapor pressure, etc., are of fundamental importance in determining the constitution and molecular weight of substances, as well as in determining their identity and degree of purity. The theoretical significance of physico-chemical constants, and the fact that their application has been extended to almost every branch of chemistry, renders it desirable, if not necessary, for all students of the science to become more or less familiar with the methods of measurement. In this book the author has systematized the more important physico-chemical methods. The very complete descriptions of apparatus and the minute details in the methods of operation, as well as the large number of references given throughout the book, seem to warrant its translation. In the preparation of the English edition no additions have been made to the text. The few references which have been added are inclosed in brackets. The Translator. CONTENTS. I. THE CHEMICAL BALANCE, 9 11. DENSITY (Specific Gravity), 13 1. Density of Solids, 14 (a) The Pyknoraeter, 14 (£) The Crystal-float Method, 17 2. Density of Liquids 19 [a] The Pyknometer, 19 The Mohr-Westphal Balance, 24 (r) The Araometer, 27 (1d) Determination of the Specific Gravity at Elevated Tempera- tures as well as the Molecular Volume of Liquids at Their Boiling Points, 28 (if) Contraction and Dilation, 31 3. Density of Gases (Vapor Density), 32 (rt) Method of Dumas, 32 (ib) Method of Gay-Lussac-A. W. Hofmann, 34 (<;■) Method of V. Meyer (Air Displacement), 38 [d) Method of Lunge and Neuberg, 41 111. CAPILLARITY, 45 1. The Rise in a Capillary Tube (The Capillarimeter), ... 45 2. The Drop-method (The Stalagmometer), 49 IV. THE CONSTANT OF VISCOSITY, 53 1. Method of Poiseuille-Ostwald, 53 V. SOLUBILITY, 56 VI. THE ELECTRIC CONDUCTIVITY OF LIQUIDS, 58 1. Method of F. Kohlrausch, 58 2. Calibration of a Wire (Method of Strouhal and Barus), . 73 v VI CONTENTS. VII. EXPANSION OF LIQUIDS, 75 1. Determination of the Coefficients of Cubical Expan- sion of Glass and Liquids, 76 VIII. MELTING POINT AND SOLIDIFYING POINT, 79 IX. DEPRESSION OF THE FREEZING POINTS OF SOLU- TIONS, 81 1. Method of Beckmann, 81 2. Method of Raoult, 86 X. BOILING POINT AND VAPOR PRESSURE, 90 1. Ordinary Method for Determining the Boiling Point, 91 2. Determination of the Boiling Points of Liquids in Small Quantities, 93 (a) Method of Siwoloboff, 93 3. Determination of the Boiling Point at Different Pressures, 95 (/>) Method of Jones-Schleiermacher, 93 XI. ELEVATION OF THE BOILING POINTS OF SOLUTIONS, 97 1. Method I of Beckmann, 97 2. Method II of Beckmann, 103 XII. SPECIFIC PI EAT, 109 1. The Method of Mixtures, no (a) Specific Heat of Solids, ill (1b) Specific Heat of Liquids (Methods of Kopp, Schiff, and Andrews), 117 2. The Ice-calorimeter (Method of Bunsen), 121 XIII. HEAT OF FUSION, 126 XIV. HEAT OF VAPORIZATION 129 Method of R. Schiff, 129 XV. THERMOCHEMICAL CONSTANTS, 132 1. Heat of Neutralization, 133 2. Heat of Solution,. 137 3. Heat of Dilution, 139 4. Heat of Hydration, . . 140 5. Heat of Combustion, 141 The Calorimetric Bomb (Method of Berthelot), 141 CONTENTS. XVI. MEASUREMENT OF CRYSTALS, 153 1. The Reflection Goniometer of Wollaston, .... 153 2. The Microscope with Polarizing Attachments, . . 160 («) Measurement of Plane Angles, 163 (.b) Testing for Double Refraction and Determination of the Directions of Vibration in Crystals, 164 (c) Investigations in Convergent Light, 165 XVII. INDEX OF REFRACTION, 168 x. The Refractometer of Abbe, 168 2. The Refractometer of Pulfrich, 172 XVIII. SPECTRUM ANALYSIS, 182 1. The Direct-vision Spectroscope, 182 2. The Spectroscope of Bunsen, 183 3. The Universal Spectroscope of KRtiss, . 189 4. The Universal Spectroscope as Spectrophotometer (Method of Vierordt), 193 XIX. ROTATION OF THE PLANE OF POLARIZATION, ... 201 1. The Polariscope of Mitscherltch, 207 2. The Polaristrobometer of Wild, 209 3. The Half-shadow Apparatus of Laurent, 211 4. The Half-shadow Apparatus of Lippich, 2x4 XX. GENERAL CONTRIVANCES FOR MEASUREMENTS, . 215 1. The Vernier (Circular Vernier), 215 2. The Cathetometer, 216 3. The Thermometer, 218 XXI. TABLES, 226 4. The Barometer, 224 ERRATA, Page 21, line 9, read 76 for 69. “ 28, “ 2, “ are for is. “ 49, “ 20, “ (p. 45) for (p. 39). “ 57, “ 39, omit comma after reaction. “ 153, “ 27, read (p. 215) for (p. 218). “ 160, “ 16, and foot-note, read (p. 201) for (p. 203). “ 174, “ 24, read 205 for 207. “ 178, “ 18, 226 for 229; line 19, read 232 for 235 “ 194, lines IX and 35, read 233 for 229. I. THE CHEMICAL BALANCE. General Rules for Weighing.—The balance is placed so that it is protected from the direct rays of the sun and other sources of heat which would produce an inequality of temperature in the different parts. The balance is brought into a horizontal position by means of foot-screws on the bottom of the case. The horizontality is indi- cated by a spirit-level or a plumb-line. It must also be free from the influence of vibrations. The interior of the balance case is always kept dry by means of calcium chloride, etc. With constant load a good balance should always take the same position when allowed to come to rest. The extent of the swing for any load should diminish slowly. After the arrestment of the balance the pointer should remain at the middle division of the scale; in raising the arrestment the two supports of the beam should be removed at the same instant. In regard to the equality in the length of the two arms, see page 11. The weights should be placed on the balance only after the arrest- ment of the beam, and should in no case be touched with the fin- gers. Rapid swinging of the beam will cause error in the weighing. For accurate weighing, the balance case should be kept closed. Adjustment of the Balance.—The sensibility and hence the vibration period of the balance are regulated by means of a gravity-bob situated near the middle of the pointer. The adjust- ment is so made that the vibration period for a short-armed balance is from six to ten seconds, and from ten to fifteen seconds for a long- armed balance. The adjustment of the balance so that the pointer will swing equal distances on both sides of the middle division of the scale is made by means of movable weights attached to the ends of the THE CHEMICAL BALANCE. beam or, when these fail, the unsymmetrical weight at the middle of the beam is given such a position that the inequality in the weights of the two arms is counterbalanced. Determination of the Resting Point. Method of Weighing.—lt is not necessary nor desirable in weighing, that the weights be adjusted so that the pointer will swing equal dis- tances on both sides of the middle division of the scale; e.g., if 10 is the middle division, the resting point may be 9 or 9.5. The resting point is calculated from several turning points of the pointer. The arithmetic mean of the turning points is taken for each side, and the mean of these two is taken as the resting point. The first and last observation used in the calculation must be made on the same side; therefore, an uneven number of swings are observed. The observation of 3 -f- 2 or 4 -)- 3 turning points is sufficient for accurate weighing; the resting point in this case is determined to the second decimal place. It frequently happens that the position of the resting point changes, especially after the weighing of heavy loads. Suppose the resting point to be 9.53 on the scale, then in the process of weighing it is unnecessary to adjust the weights so that the second resting point will be exactly at the same position. Assuming, when the weighing is made to one centigram, the weight = 10.28 gm., let the rider be placed at 5 mg., and suppose the resting point then to be 9.20. Let the rider be next placed at 6 mg., and suppose the resting point to be 10.16. Then 1 mg. corresponds to 0.96 scale divisions, and hence 10.285 gm- are too light by an amount which corresponds to 9.53 9.20 = 0.33 scale divisions, i.e., |-;|-| = 0.34 mg. The true weight therefore is equal to 10.28534 g. It is even unnecessary to make this double adjustment of the rider. Apart from the determination of the resting point, a single observation near the correct weight will suffice when the operator has once constructed a sensibility table. By the sensibility of a balance is meant the deviation in scale divisions produced by an increase of 1 mg. in the load. The amount of deviation is always more or less dependent on the load. For different loads the balance is adjusted with equal weights in each pan. A small excess of a mg. is then placed in the one pan. THE CHEMICAL BALANCE. The resting point is thereby removed n scale divisions, and the sensibility for the given load is —. When this value has been de- a termined for loads of 5:5 or 10 : 10 gm, and a curve constructed with the loads as abscissas and the corresponding sensibilities as ordinates, the operator can, with the help of this curve, easily make the necessary correction for any weighing which is approximately correct. Relative and Absolute Weighing.—The chemical balance is generally employed to determine relative and not absolute weights. This being the case, a slight inequality in the lengths of the arms can be neglected if the weights are always placed upon the same pan. On the other hand, if the absolute weight is to be determined, it is desirable to know the ratio of the lengths of the two arms. This is found by the method of double weighings. If p represents the weight of the load q placed upon the left pan of the balance, and px the weight of the same load placed upon the right pan, then the ratio of the lengths I and r of the left and right arms is found from the simple equation of the lever: ql=p r and pxl= qr; _A__ The weight of a load obtained by placing the weights on the right pan of the balance must be multiplied by the above ratio in order to obtain the absolute weight. The absolute weight can also be determined from a double r weighing without a knowledge of the ratio —. From the equations q I—pr and pxl=q r, we have q= Vp p1; or, simplified =\ (p p\ )*,—i. e., the true weight of the load qis the arithmetic mean of the weighings on the right and left pans of the balance. The tare method is also applicable. The load qis brought into equilibrium with a second set of weights, or another load, and then instead of q is placed enough weights to bring the balance again into equilibrium. * Kohlrausch, Prakt, Phys. VII, 35, 1892. THE CHEMICAL BALANCE. Reduction of Weighings to a Vacuum Standard.—When brass weights (density = 8.4) are used, this reduction is made ac- cording to the formula,— P=p + 0.0012 * J; * where P represents the weight of the substance in vacuo, p is the apparent weight obtained by weighing in air, and d is the density of the weighed substance. The error introduced by neglecting this reduction to a vacuum standard is greater, the greater the difference between the specific gravity of the weighed substance and that of the weights. Even for relative weighings in chemical analysis, where it is unnecessary to determine the absolute weight, this reduction is too often neglected. Calibration of a Set of Weights and Preparation of a Correction Table.—Let the larger weights of the set be desig- nated as 50', 20', 10', 10", s', 2', T, 1", T", and let the arms of the balance be of unequal length. In this case, by the method of double weighings of the weights against each other, suppose we have,— Left. Right. sc/ correspond to 20/ -)- 10/ . . . a mg. 20/ -j- xo/ -(- 10// I) mg. correspond to sc/. Then according to page 11 : In the same manner we obtain sc/ = 20/ ic/ + 10" -f . . . \{a4* b) mg. 20' ic/ 4- 10" 4- \ (c -f d); lo" = io/ -j- \ {e 4-/), etc., etc. Representing the corrections \(a 4- \(T ( /), . . . by a, /9, y, . . . we have the following relations: sc/ = 20' -) io7 -f- io// 4- ... a 20/ - io/ -t- 10// 4- . ./3 10" io/ -j- ... y 5' 4- 2/ 4- i/ 4- i" 4- x"' iq/ in which a, ft, y, and 8 can be positive or negative. * Kohlrausch, Prakt. Phys. VII, 36, 1892, and Landolt-Bornstein, p. 4, 1883, Tables. DENSITY. Comparing all the weights against the xo' gm. weight, we have,— sq/5q/ =5 X IQ/ +a+P+ 2 7 + J 20/ =2 X 10/ +P + 7 io// =i X xc/ -f 7 ic/ ' = i X io/ 5' +2; +i' + i// + i/7/ =i X >o' 4- (! ■S = 50/ -)- 20/ + XC/ -)- XO'' -|- 5/ +27 -f- I/ + -)- I/// =IO X XC/ + (« + 2/3 + 47 + 2 (5)- If the correction table is to be drawn up with reference to the standard gram, one of the weights must be compared with a standard weight. For most work in chemistry (analysis, specific gravity determinations, etc.) this is not necessary. In such cases the corrections for the single weights are assumed to be so small that the sum Sof the larger weights is correct; then 5= 10 X io'-|- (a -(- 2 /? -f 4 y -j- 2 d) 100 gm. Let (o. —[— 2ft —4 y-: 2 4 then io/ =io g. a 10" =. xo “ + y 5/ + 2' -f- i/ -)- IO “ a -f 6 20/ =2O “ 2(T4-/? -f y sq/5q/ =s° “ 5 +a+/? + 2 7 + In a similar manner the five weights s', 2', I', 1", and 1"' are compared with each other, and likewise the smaller weights. For the latter, however, a single weighing is sufficient, even though the balance-arms are of unequal length. If the balance-arms are equal, a single weighing is sufficient for any of the weights. 11. DENSITY (Specific Gravity). General.—The density of a body is the mass of unit volume. For solid and liquid bodies the mass of 1 c.c. of water at 40 is con- sidered the unit of mass. The density, then, of a body may be defined as the ratio of its mass to the mass of an equal volume ot water at 40. DENSITY OF SOLIDS. The specific gravity of a body is the weight of unit volume. As the ratio of the weights of bodies in a vacuum is the same as the ratio of their masses, the numerical value of the density and specific gravity is the same. The densities of gases are usually spoken of as vapor densities. The vapor density of a gas is the ratio of the mass of unit volume of the gas to the mass of unit volume of a standard gas at the same temperature and pressure. Dry air is usually taken as the standard gas. By specific volume is meant the reciprocal of the specific gravity,—the volume of unit mass. The atomic and molecular volumes are the volumes which the weights corresponding to the atomic and molecular weights occupy. Let p represent a given weight of substance in grams, v the volume in cubic centimeters, d and s the density and specific gravity,
1891. 28
DENSITY OF LIQUIDS.
(ff) Determination of the Specific Gravity at Higher Tem-
peratures AS WELL AS THE MOLECULAR VOLUME OF
Liquids at Their Boiling Points.
METHOD OF RAMSAY-LOTHAR MEYER.*
Principle and Calculation.—The specific gravity and molec-
ular volume of a liquid at the boiling point is determined by this
method, in which a pyknometer (Fig. 10) is filled with the liquid
and heated to the boiling point in the vapor of the
same liquid in a boiling-vessel.
As the volume of the pyknometer changes with the
temperature, the coefficient of the cubical expansion
of glass must be known. If the pyknometer is made
of Jena standard glass (No. 14), then, according to
Weidmann,f 3/? 0.0000237. The value of 3/9 can
be determined in the manner described on page 75.
The pyknometer is next weighed filled with air and
Fig. 10.
then with distilled water at two temperatures, t and
tv rather far apart, about the temperature of the room
and the boiling point of water; then from page 14 we have :
-vt and vtx —l-
where v, p, and .y represent the volume, weight, and specific
gravity of water at the temperatures given ;
therefore ;
pt 1 _pt
Pt\ Pt 1 r) Sti
For the specific gravity of water at different temperatures see
Landolt-Bornstein’s Tables, pp. 34-36, 1883.
If 3 /? is known, the volume for any given boiling point $ be-
tween t and tx is :
v$ vt -f 3 p (1? —t) + 3 p (1? t),
* Neubeck, Zeitschr. physik. Chem. I, p, 651, 1887, and Feitler, ibid. 4,
p. 66, 1889.
jWeidmann, Inaug. Dissert., Jena, 1886. MOLECULAR VOLUME OF LIQUIDS.
29
pt is the weight and st the specific gravity of the water in the
pyknometer at t°. By making a larger number of determinations
the corresponding volumes for temperatures between t and tx can
be calculated according to the above formula.
If ft- represents the boiling point of the substance to be investi-
gated, then the specific gravity at that temperature is s$ = £fL
where p& is the weight of the liquid at the boiling point [(pyk. -j-
Hq.) —(pyk. + air)], and is the volume of pyknometer at
the temperature ft. Then the molecular volume vm = --, where m
represents the molecular weight of the substance. The reduction
of the weighings to a vacuum standard can here be omitted. For
molecular weights see table at end of this volume.
Apparatus and Method of Operation.—The pyknometer
(Fig. 10) of about 2.5 c.c. capacity consists of thin glass (Jena
standard glass, No. 14).
The wider, closed cylindrical part is united with a somewhat
longer, rather narrow capillary tube with a turned-up point.
The filling of this pyknometer with a liquid can be accomplished
with the help of the apparatus shown in figure 11.
A wide tube closed with a rubber stopper is connected through
a side tube with an exhaust pump and the outer air by means of
two stop-cocks. The air, before entering from the outside, must
pass through a calcium chloride tube.
The bottom of the tube is filled with the liquid, into which the
pyknometer is sunk by means of a wire which passes air-tight
through the rubber stopper. The pyknometer is lowered into the
vessel until the point of the capillary tube is immersed in the
liquid. By repeated opening and closing of the pump and letting
in air, it is an easy matter to fill the pyknometer with liquid, with
the exception of a small air-bubble which, upon subsequent heat-
ing, disappears. Simultaneous heating of the liquid and apparatus
hastens the filling.
The subsequent emptying of the pyknometer is accomplished in
the same apparatus. The pyknometer is hung with the point up-
ward, and the two stop-cocks alternately opened and closed. It
is then dried by means of alcohol and anhydrous ether. DENSITY OF LIQUIDS.
The almost filled vessel is hung in the boiling-flask* represented
in figure 12, by means of a nickel wire y which passes air-tight
through the cork k.
The rather wide boiling-flask, in which the liquid in the
pyknometer is allowed to boil, is connected with a reflux con-
denser, which in turn can be connected with a Stadel-Hahn
or some other form of pressure regulator. With this arrangement
the liquid can be made to boil under in-
creased or diminished pressure. The
method permits then of a determination
of the specific gravity and molecular
volume at different pressures and tem-
peratures. By means of the regulators
mentioned, the pressure can be measured
accurately to within about 2 mm.
Fig. 11.
Fig. 12.
The thermometer a fastened in the cork must be tested and ad
justed as described under Section xx.
For liquids which cause bumping, it is advantageous to have a
capillary tube /? passing through the stopper to the bottom of the
flask, through which a current of air or carbon dioxide is passed.
* Of course, the filling and emptying of the pyknometer can also be accomplished
in this flask ; however, it is less convenient. CONTRACTION AND DILATION.
31
The pyknometer filled completely, with the exception of a small
air-bubble, is hung in the flask so that the point of the capillary
tube remains in the vapor. The desired pressure is then obtained
and the liquid in the boiling-flask brought to boiling. The liquid
in the pyknometer expands and drops out of the capillary tube,
taking with it the last trace of air, until it has assumed the constant
temperature equal to that of the boiling point of the liquid.
The boiling is then stopped. The liquid in the pyknometer
cools and draws back through the capillary tube, with the excep-
tion of a small drop which hangs on the end of the tube; the
vessel is then dried and weighed.
If the substance becomes stiff on cooling, the pyknometer may
break. This danger can be avoided by repeatedly melting the
outer layer, thereby distributing the mass uniformly, or by weighing
before the complete stiffening of the substance. Substances for in-
vestigation, see Neubeck, Zeitschr. physik. Chem. 1, p. 651, 18187.
A second method which is to be recommended for determining
molecular volumes is that of R. Schiff (see p. 76).
Literature on Molecular Volumes.—Ostwald, Allgemeine Chemie, 2. Aufl.,
Bd. I, pp. 357 and 838; R. Schiff, Lieb. Ann. 220, pp. 71 and 278, also Ber. d. d.
chem. Ges. 14, p. 2761, 1881; Ramsay, Jour. Chem. Soc. 35, p. 463, 1879;
Thorpe, ibid. 37, pp. 141 and 327, 1880; Lessen and his students, Lieb. Ann.
214, p. 81 ; 221, p. 61 ; 224, p. 56; 225, p 109; Gartenmeister, Inaug. Dissert.,
Konigsberg, 1885, and Lieb. Ann. 233, p. 249; Stadel, Ber. d. d. chem. Ges.
15, p. 2559, 1882; Elsasser, Lieb. Ann. 218, p. 302, 1883; Vollmar, Ber. d. d.
chem. Ges. 15, p. 2560,1882 ; Horstmann, ibid, ig, p. 1579, 1886, and 20, p. 766,
1887 ; Bartoli, Ann. chim. phys. (6), ser. VII, p. 394,1886 ; Kopp, Memoires sur les
vol. mol. des liquides (Winter, Heidelberg, 1886), and Lieb. Ann., 250, p. 1,
1889; Neubeck, Zeitschr. physik. Chem. 3, p. 649, 1889; Feitler, ibid. 4, p. 66,
1889; Lessen, 243, p. 64, and 254, p. 42, 1889; Gro.vhans, Kosmos, 1891, Ref.
Zeitschr. physik. Chem. 8, p. 431, 1891.
[See also the recent investigations of J. Traube, Zeit. f. anorg. Chem. 3,
p. 11, 1893, and 8, p. 12, 1895; Ber. d. d. chem. Ges. 28, p. 2924, 1895;
28, p. 3296, 1896; 30, p. 273; and 33, p. 130, 1898; Wied. Ann. 61, pp. 380
and 395, 1897.—Tr.]
() Contraction and Dilation.
By the contraction or dilation, produced in the mixing of liquids
or the solutions of solids in liquids, is meant the change of volume
per unit volume of the original substances. 32
DENSITY OF GASES.
If, for example, two liquids of volumes vx and v 2 are mixed and
the volume of the mixture is v 3, then the volume change per unit
volume is:
_ v\ + v-i ya
+
A contraction has taken place when c is positive, and a dilation
when cis negative. From page 14 we have v% —, where p3 and s%
h
represent the weight and specific gravity of the mixture. p3 is equal
topx p2, the weights of the original liquids, and these in turn
are equal to vx sx -j- z>2 V We have then the equation :
c _ K + V,) S3 {vx Jt +vt S2) _
K + w2j J«
For the determination of contraction or dilation according to this
equation, it is only necessary to note the volumes vx and v 2 of the
original liquids, and to determine, by known methods, their specific
gravities sx and 2, as well as the specific gravity ss of the mixture.
For solutions of solids the same formula holds good. On con-
traction of solutions, see Ostwald, Allgem. Chem., 2. Aufl.,Bd. i,
p. 782 et seq., 1891.
3. THE DENSITY OF GASES (Vapor Density).
(.a) Method of Dumas.
Principle.—The weight of a given volume of a gas is determined,
and then, according to the known laws of Boyle and Gay-Lussac,
the vapor density is calculated, i. e., the weight of unit volume of
the gas compared with dry atmospheric air at the same temperature
and pressure.
Apparatus and Method of Operation.—A thin-walled glass
balloon of about xoo to 300 c.c. capacity, with a side tube (Fig.
13) is, after drying, drawn out at a into a smaller tube of about
1 mm. in diameter. Let the weight of the dry balloon be repre-
sented by p. While gently warming the balloon several grams of
the liquid to be investigated are allowed to enter. The balloon is
placed in a water-, oil- or paraffin-bath up to the narrowed part a. METHOD OF DUMAS.
33
The temperature of the bath is regulated so as to be at least io°
above the boiling point of the liquid at the end of the experiment.
When the liquid in the balloon has been completely changed to
vapor, there being enough of the substance present to expel all the
air, the balloon is melted off at a by means of a blow-pipe flame,
after which the barometric pressure b and the temperature t of the
water-bath are observed. After cooling, the balloon, together with
the melted-off glass tube, is weighed. Let this weight be repre-
sented by ps; let the barometric pressure and the temperature at the
time of weighing be bx and tx. To test for the presence of air in
the balloon, the point is then broken off under recently boiled water
which is free from air. The balloon is filled completely with water
only in cases where the previous removal of air had been complete.
If the filling with water is complete, the balloon together with
the water and the melted-off glass tube is placed upon a balance
and weighed to within one centi-
gram. Let the weight be pw and
the temperature of the water again
be tx.
the empty balloon can be taken
Calculation.—The weight of
equal to p, since the quantity of
Kig. 13.
air displaced by the thin-walled balloon is nearly the same as that
present in the balloon at the time of weighing.
pw—p can be taken as the weight of the water at t°, since the
weight of the air displaced by the balloon in comparison with the
weight of the water can be neglected. If Qis the specific gravity
of water at /x°,* then the volume of the balloon is :
_ pw —P
1 Q '
The volume vt at the temperature of the water-bath may be calcu-
lated from vtx by the formula vt =tx -)- 3/? (t— tx), where 3/5 is
the coefficient of cubical expansion of glass, and can be taken as
o, 000025.
The weight g of the vapor contained in the balloon is found from
* Landolt-Bsrnstein’s Tables, pp. 33 and 34, 1883. 34
DENSITY OF GASES
the expression g = ps—/ +/, where /is the weight of the air
displaced by the balloon.
At the ordinary pressure temperature tx we have :
I K 0-001293
76 (1 + a/)
where vtx is the volume of the balloon at t°, 0.001293 is the weight
of 1 c.c. of air at o° and 76 cm. pressure, and a the coefficient
of expansion of gases = 0.00366.
The vapor density d is then given by the formula
d = K. 76 (1 +« 0
Wt £ 0.001293
and the molecular weight m is equal to 28.9 d.
It frequently happens in the vaporization of the substance that
the air is not completely removed from the balloon, as can easily
be seen from the subsequent filling of the vessel with water. If
the error introduced in this manner is to be neglected, fill the
balloon completely and calculate according to the above for-
mula. Otherwise the balloon is sunk into the water after break-
ing off the point, until the inner and outer surfaces of the water
stand at the same level. The balloon with this quantity of water
is weighed and the weight represented by pwl; it is then filled com-
pletely with water and again weighed; this weight =pw. The
calculation of the exact vapor density, taking into account all
sources of error, follows from the equation :
{ps /) —y + pml pa
d= ——
b I 4- 0.00367/.
jt 11+313 {‘-'M -{p-
)! represents the density of the air at the temperature and pres-
sure by. *
(£) Method of Gay-Lussac-A. W. Hofmann.
Principle.—A quantity of substance weighed off in a small
glass vessel is introduced into a barometer tube, the lower end of
* Kohlrausch, Prakt. Phys. vn, 55 ; ibid. Table, p. 406, 1892. METHOD OF GAY-LUSSAC-A. W. HOFMANN.
35
which is immersed in mercury. This tube is surrounded by a
glass jacket, which is heated to constant temperature by means of
boiling vapors. Taking into account the pressure and temperature,
the volume occupied by the vaporized substance is read off, and
from this volume for a given weight of substance the vapor density
is calculated.
Apparatus.—An accurately calibrated * wide barometer tube,
A (Fig. 14), of about 76 cm. in
length, is set upright in a mercury
trough' and fastened below in a wider
glass jacket B by means of a cork.
The jacket is heated by means of
the vapors of boiling liquids (water,
anilin, etc.), which are conducted in
through the tube « and out through
the tube b, and finally condensed in a
coiled tube cooled with water.
The arrangement for reading off the
volume of gas consists of a metallic,
upright bar C. This is provided with
a nut in which are fastened, in vertical
positions, two metallic bars, one of
which is graduated in millimeters;
these can be raised or lowered by
means of the screw c. The second
bar ends in a point which forms the
zero of the scale, and is lowered
toward the surface of the mercury in
the trough w until the point seems to
Fig. 14.
touch its image formed by the reflection of the mercury, without
actually coming in contact with the surface of the mercury. The
height of the mercury in the barometer tube is determined by means
of cross-wires in two vertical metallic rings, the height of which is
so adjusted by means of the screw d that the two horizontal cross-
wires and the top of the mercury are brought into the same plane.
*For method of calibration, see Wiedemann and Ebert, Phys. Prakt. 1, p. 99,
1890. 36
DENSITY OF GASES.
The height of the mercury in the barometer tube is given directly
by the distance from the metallic point of the scale to the point
where the screw d is situated on the same scale.
The substance is weighed in a small glass-stoppered flask
(Fig. 15) which is placed on the balance in the small metallic or
glass vessel represented in the figure.
Method of Operation.—The barometer tube A, cleaned and
dried by means of alcohol, is filled with dry mercury free from air-
bubbles. The air-bubbles clinging to the sides of the tube are
removed by allowing the mercury to flow in and out several' times.
The tube, completely filled with mercury, is closed by means of the
finger, inverted and placed upright in the mercury trough, so that
a perfect vacuum is formed in the upper part of the tube. It is
then fastened in the glass jacket by means of a cork near the lower
end, and the weighed substance with the vessel is introduced into
the barometer tube. The quantity of substance is so
chosen that when vaporized it fills the tube almost to
the stopper at the lower end of the jacket. This
quantity is easily calculated from the formulas which
follow. The tube, owing to the danger of breaking
Fig. 15.
by the sudden vaporization of the substance, should
be slightly inclined when the substance is introduced. The stopper
must always be placed loosely in the small glass flask. After intro-
ducing the substance, which immediately vaporizes either wholly or
in part, the vapor jacket is fastened in position and connected with
the vessels attached to a and b. In the former is a liquid, the boil-
ing point of which is at least io° above that of the substance in the
tube A. Water or anilin (B. P. 183°) is usually employed. The
vapor of the hot liquid must be conducted in carefully at first.
When the temperature has become constant the height h of the
mercury in the barometer tube above the surface of the mercury in
the trough is carefully determined by the method already described.
The length hl of the barometer tube from about the middle of the
lower cork to the surface of the mercury in the trough is also
determined.
Calculation.—The vapor density d is calculated from the gen-
eral equation :
d g + 0.0 0367^)
0.00129 SVO W/0.001293 METHOD OF GAY-LUSSAC-A. W. HOFMANN.
37
g is the weight of the substance in grams, v 0 the volume of the
vapor at o° and 76 cm. pressure, 0.001293 the weight in grams of
1 c.c. of air, and v the observed volume of the vapor in the barom-
eter tube at the temperature t of the experiment and pressure p.
The pressure p is equal to the barometric pressure b reduced to
o° minus the column of mercury h reduced to o°. As the tem-
perature of the interior of the jacket and likewise the mercury
within the jacket is t and that of the lower part of the mercury
column tv the temperature of the room, we have :
b h. h h,
? 1 f
I -(- O.OOOISI fx I -j- O.OOOISI tl I -f- O.OOOISI^
where f represents the vapor pressure of mercury at the temperature
t, hx the height, and tx the temperature of the column of mercury from
the middle of the stopper to the surface of mercury in the trough,
and h /q the height of the column of mercury in the vapor jacket
at the temperature t. The above formula then can be written :
p—(b hx) (I 0.000181 q) (h kx) (l 0.000181 /) —f*
For exact measurements the expansion of the
barometer tube when heated must be taken into
account. As the tube is calibrated for 150, its vol-
ume vt at t° is :
Vt vl5 (i -f 0.000025 [t 15))
vt should therefore be substituted for v in the above
expression for finding d.
An appreciable error is also introduced by the fact
that the mercury column consists of two parts, which
are heated to different and not accurately measured
temperatures. For exact determinations, therefore,
the recent modification of the apparatus (Fig. 16)
is doubtless to be preferred. As the entire column
of mercury in this case is heated to the tempera-
ture t, the expression for p is much simplified.
Application of the Methods of Dumas and
Hofmann,—The advantage of the Gay-Lussac-
Hofmann method over that of Dumas consists prin-
Fig. 16.
* For the redaction of the mercury column to 13.596W
in millimeters. The variation in several measurements should not
amount to more than one unit in the fifth decimal place.
The tube should always be kept perfectly clean.
At the end of the investigation the tube should be closed with
black rubber ; from time to time it should be cleaned with concen-
trated nitric acid. After each observation the tube should be
cleaned and dried by sucking into it water and alcohol (not ether) ;
this is accomplished by connecting one end of the tube with a
sulphuric acid bottle and the other with the mouth or a pump. Saliva
or rubber should never be allowed to enter the tube.
If the necessary precautions are always observed, the same tube
can be used for several years.
An unclean tube is usually the cause of an imperfect wetting of
the walls by the liquid, and of the irregular, jerky movements of
the liquids. In such cases the cleaning can frequently be accom-
plished with nitric acid.
Method of Measurement.—The scale is placed in the sup-
port so that the tube stands as vertical as possible. The error
introduced by a slight inclination of the tube is inappreciable.
The vertical position is determined simply with the eye or by
means of a plumb-line.
The liquid is placed under the tube in a small glass vessel. The
dry points of the scale should touch the surface of the liquid simul-
taneously. The inclination, however, amounts to less than 0.1
mm. if the two points are not immersed simultaneously in the
liquid; it is then desirable to always bring the same point to the
liquid first.
When the points are adjusted, the liquid is slowly sucked up
into the tube. The operation should be conducted so as to pro-
duce a perfect wetting of the tube.
The liquid is sucked (carefully avoiding the entrance of saliva
into the tube) three times from 3 to 4 cm. above the final position 48
CAPILLARITY.
of the liquid meniscus, and is allowed to fall from 5 to 8 cm.
When the liquid has been sucked up three times, it is allowed to
fall in the tube, and the height assumed by the lower edge of
the meniscus after one-half to one minute is read off (care
being taken to avoid any error due to parallax). A microscope
may be advantageously employed; or a cathetometer may be used
in making the reading. Heating of the tube should always be
prevented.
Ordinarily, the position of the liquid remains constant during
one or several minutes, and then a gradual sinking begins, owing
to a lack of perfect wetting of the tube ; or a rising for volatile
liquids. For exact measurements, a small correction must be
applied to the observed height of the meniscus; the observed
value should be increased by yi r. The true value then is
= & + V.
Care should be taken in all observations that small air-bubbles
do not occur in the liquid in the tube, and that the column of
liquid should at no place be separated. Especially for the more
viscous liquids or with very narrow tubes it is important, after the
capillary rise has been determined according to the above method,
—by sucking the liquid up and allowing it to fall,—to confirm the
result by sucking the liquid up once, forcing it down, and allowing
it to rise of its own accord. The height attained by this capillary
rise should not be more than of a mm. lower than the height
attained by the first method.
The liquid and the tube should be warmed to the same tempera-
ture as that of the room before the experiment; it is also very impor-
tant, in most cases, that liquids should be sucked up only from the
surface ; a change of concentration influences the result.
The observations are always made at a definite temperature,
usually at 15 or 20° ; the temperature coefficient for most liquids
and for tubes of from o. 15 to o. 2 mm. radius amounts usually to only
0.1 to 0.2 mm. for i° Celsius.
The observations should be repeated after cleaning and drying
the tube with alcohol. The variations should not, at most, amount
to more than 0.2 to 0.3 mm. About twenty observations may be
made in an hour. THE STALAGMOMETER.
49
The constant a 2 cos ■& =r h is, for water at 150 :
= 15.09 (according to Volkmann),
= 14.7° ( “ Quincke),
= 14.88 ( “ Brunner),
= 15.12 ( “ Hagen),
= 15.24 ( “ Wolff),
= 14-77 ( “ Traube).
Weinberg, Zeit. phys. Chem. 10, p. 34, 1892 ; ibid. p. 38, literature.
Principle and Calculation.—If different liquids under defi-
nite pressures are allowed to drop from a horizontal, smooth sur-
face of from 6 to 8 mm. in diameter, the weights of the drops are
proportional to the weights of the liquids in the capillary tubes.
If, therefore, definite volumes of different liquids drop from the
same surface, the number of drops in the volume v are inversely
proportional to the rise of the liquids in capillary tubes.
2. THE DROP METHOD (The Stalagmometer).
If zw and zr represent the number of drops contained in the
volume v of water and some other liquid dropping from the surface
a (Fig. 20), and ajl cos -&w and ajl cos &r represent the corres-
ponding capillary constant (p. 39), we have from the above pro-
portion the equation :
COS &w • zw zw
ar2 cos xrr aw* = 14.90 ——,
and
yr cos &r = 7-45 >
zr sr
where sw and sr represent the specific gravities of the water and the
liquid.
Apparatus.—The apparatus consists of an outflow'arrangement
A as well as the pressure apparatus B, and is identical in its essen-
tial parts with Poiseuille’s apparatus for determining the constant
of viscosity; hence the constants of capillarity and viscosity may
easily be determined together.
The stalagmometer A consists of a tube bent twice into a knee
shape, the upper end of which expands into a globe in which a CAPILLARITY.
definite volume v, of 6 to 8 c.c. capacity, is divided off by the two
boundary lines b and c. The middle and lower limb of the tube
is a capillary tube, the outer diameter of which is from 6 to 8 mm.,
while the inner diameter is chosen according to the height of the
pressure column and length of the tube, so that the time of forming
Fig. 20.
a drop will be at least four to five seconds. The drop-surface a
(6 to 8 mm. in diameter) should be well polished, and the outer edge
made as conical as possible (see Fig. 20) to prevent any drawing
away of the liquid by the sides of the tube, so that only the under
surface where the drop is formed will become thoroughly wet.
The flow of liquid to the drop-surface must take place through a THE STALAGMOMETER.
51
capillary tube, otherwise an irregular whirling motion will be pro-
duced in the drop.
The conical grinding of the sides of the tube at the surface is
unnecessary; by carefully greasing the outer walls of the tube near
the surface the drawing away of the liquid can be prevented.
By means of the pressure apparatus the liquid can be made to
flow out under constant or any desired pressure.
A wide glass tube about one meter high is connected with a
Wulf bottle, in which the air is compressed, corresponding to the
height of the pressure column. The filling with water takes place
through the stop-cock d. The level of the water in the pressure
tube is kept constant by means of the water in the vessel f, which
gradually flows in, owing to the tilting of the piece of ground-glass
at g when the surface of the water in the
pressure tube is lowered. The stop-cock
e is connected with an air-pump, which
makes it possible to suck the liquid
through a into the apparatus. The glass
parts should be connected by means of
black or red rubber tubing.
If the apparatus is also to be used for
determining the constant of viscosity (p.
53), it is better to divide A into two
portions, connected by means of rubber
Fig. 21.
(as in Fig. 21). bis a capillary knee-
tube which must be removed in the determination of the con-
stant of viscosity, in case its inner radius is not considerably
greater than that of a. The knee-tube a (volume v, length and
radius of the capillary tube) is then carefully measured by means
of mercury and placed in a cylindrical glass water-bath. For
determining the capillary constant alone, the water-bath (Fig. 20)
is not necessary. For the simultaneous determination of constants
of capillarity and viscosity, see J. Traube, Ber. d. d. chem. Ges.
19, p. 871, 1886.
Method of Operation.—The liquid at the temperature of the
room and as free as possible from dust is sucked up into the
apparatus by connecting the stop-cock e with the pump, until the
level of the liquid reaches the mark b. The connection is then CAPILLARITY.
made with the pressure apparatus and the number of drops con-
tained in the volume v counted.
If the outflow is sufficiently slow, the operator with a little care
and practice can determine the exact moment when the lower edge
of the meniscus passes the marks b and c, and estimate the corre-
sponding quantity of liquid with certainty to o.i to 0.2 of a drop.
If the observation of the moment when the liquid passes the mark
b is not made sharp enough, connection is again made with the
air-pump, until finally for the mark b a whole drop separates.
This method leads to accurate results; repeated observations
should not show variations of more than 0.2 or 0.3 in the number
of drops contained in the volume v. The drop-surface and capil-
lary tube should be absolutely clean. A variation in the speed of
the outflow, due to the presence of dust in the capillary tube,
gives rise to appreciable errors; the rate of outflow, therefore, is
always fixed as nearly constant as possible. The larger air-bubbles
in the drop should be avoided.
For the majority of liquids, whose constants of viscosity and
rates of outflow do not differ more than fifty per cent, from the
corresponding values for water, the pressure, under which the
liquids flow out slowly (one drop in five seconds), can be kept
constant. If, however, very viscous liquids are to be compared
with easily flowing liquids (aqueous glycerin, cane-sugar solu-
tion with water), the pressure columns are to be shortened or
lengthened so that the speeds of outflow are not very different.
The error introduced by using equal pressures in such cases
seldom amounts to more than one to two per cent. The difference
between the capillary constants y calculated by the capillary-rise
method and the drop method amounts to less than one per cent.
The determination of the capillary constant at higher tempera-
tures is best accomplished by the drop method ; at the boiling point
by the capillary-rise method: R. Schiff, Lieb. Ann. 223, p. 47,
and Gazz. chim. Ital. 14, p. 1, 1884. Determination at the
melting point; J. Traube, Ber. d. d. chem. Ges. 24, p. 3074, 1891.
Application of Capillary Constants.—The constant of
capillarity has hitherto been of little use for chemical purposes.
On the relation to the constitution of homogeneous organic
liquids, see the work of Schiff, already cited. The constant of VISCOSITY.
53
capillarity is of still greater use in the domain of (aqueous) solu-
tions.
i. The constant for water is often considerably lowered by dis-
solving organic compounds in it. The constant is closely related
to the constitution of the dissolved substance; for isomeric com-
pounds it is frequently very different. The constant is of consider-
able value, therefore, in determining the constitution of com-
pounds. J. Traube, Lieb. Ann. 265, p. 28, 1891.
2. The capillarity constant is of importance from an analytical
standpoint.
Many compounds (especially electrolytes) in concentrated solu-
tion influence the constant of water very little, while other sub-
stances in dilute solutions often lower the constant considerably.
The capillarity constant makes it possible, therefore, to deter-
mine, often very accurately, the concentration of a solution, and
hence may be used in the approximate quantitative determination
of many substances present in small quantities in a solution which
may at the same time contain large quantities of other substances
(mineral acids and bases as well as salts). The constant is also of
value in determining the degree of purity of a dissolved substance.
Dudaux, Ann. chim. Phys. (5) 13, p. 76, 1878; J. Traube, Jour, pralct.
Chem., N. F. 31, p. 177, 1885. Application to the determination of the basicity
of acids, J. Traube, Ber. d. d. chem. Ges. 24, p. 3074, 1891.
IV. THE CONSTANT OF VISCOSITY.
I. METHOD OF POISEUILLE-OSTWALD.
Principle and Calculation.—The constant rj of viscosity may
be defined as the work required to move, in unit time, two layers
of liquid of unit surface in parallel and opposite directions ; the
distance moved being equal to the distance between the two layers
of liquid.
The constant is determined by different modifications of the out-
flow method of Poiseuille. The time required for a definite volume 54
VISCOSITY.
of liquid under a definite pressure to flow through a capillary tube
is determined, and the constant of viscosity calculated according
to the formula of Finkener : *
r4 7T h s vs I
v— t .
8/ v 87T g I t
where tj is the constant of viscosity of the liquid ;
s the specific gravity of the liquid ;
r and / the radius and length of the capillary tube (in cm.) ;
v the volume of liquid flowing out in the time t (cm. sec.) ;
h the height of the pressure column in centimeters, under which
the liquid flows out;
g the acceleration due to gravity = about 981.2 and tt the
known constant value.
As all the values except s and t are constant for the same appa-
ratus, the above formula may be written ;
, c, s
)/ = C St
t
The constants c and cx are to be determined for each apparatus.
The dimensions of the apparatus are so chosen that the value of
cx— is only a small per cent, of the value t]. Instead of ij, it is
frequently sufficient to determine the “specific viscosity ” z of the
liquid. By this is meant the time of outflow of the liquid (multi-
plied by 100) at any temperature, divided by the time of outflow
for water at o°. We have, therefore,
r 100 t
' tw
The determination of the constants of the apparatus is not
necessary in this case.
Apparatus (Fig. 22).—A vertical capillary tube b is fused at
the ends to the two wider tubes e and d, so that the change from
the capillary to the wider tubes is as sharp as possible. A bulb k
is blown in the upper tube d, in which a definite volume v of
liquid can be measured off by means of the two marks a and c.
* Gartenmeister, Zeit. phys. Chem. 6, p. 525, 1890; also Wilberforce, Phil.
Mag. (5) 31, p. 4°7, 1891. METHOD OF POISEUILLE-OSTWALD.
55
This simple apparatus is fastened by means of a rubber stopper in
a large glass bell-jar of 15 to 20 liters capacity, which is filled
with water and arranged so that the temperature may be determined
accurately to o.i°.
The pressure under which the liquid flows out in this apparatus
is found by multiplying the specific gravity
of the liquid by the varying height of the
pressure column during the investigation.
The mean height of the pressure column
may be placed equal to the height h of the
lower mark a above the lower opening of the
capillary =hn increased by half the distance
from ato c = hu, therefore h=. h, -j- hu.
For exact measurements it is desirable
to use two or three different outflow tubes.
The volume of the bulb and the dimen-
sions of the capillary tube are accurately
measured by means of mercury,—best be-
fore the apparatus is set up. For the meas-
Fig- 22>
urement of capillary tubes, see page 46.
The dimensions of the separate parts of the apparatus best
adapted to this work lie between the following limits ;
v =4to 8 c.c.
r = 0.025 to 0.030 cm
/ =3oto 40 cm.
hj, = 1 to 2 cm.
The time occupied in the investigation is determined either with
the help of an ordinary seconds watch or better, a chronograph;
in the latter case the time is measured to the fraction of a second.
Method of Operation.—After carefully cleaning the capillary
tube, the apparatus is filled with the clear liquid free from dust by
means of a pump from below. By closing the black-rubber tube
with a glass rod, the outflow of the liquid is prevented until the
temperature of the liquid is the same as that of the water-bath. It
is to be observed that the constant of viscosity, in most cases,
varies to a high degree with the temperature.
When the experiment is to be commenced the glass rod is re-
moved, and the time required for the passing of the meniscus from 56
SOLUBILITY.
the upper mark c to the lower mark b is measured by means of the
chronograph. The liquid is not allowed to drop from the lower
end of the tube, but the outlet end is immersed in a liquid con-
tained in a small vessel.
The experiment is always repeated. Greater differences than
0.2 per cent, in the values of t are usually to be traced to the
lodging of small solid particles at the top or in the capillary tube.
The tube is therefore frequently examined with a microscope.
Before using, the apparatus is first tested by experimenting with
water. The following table contains the constants of viscosity for
water at different temperatures :
Temperature.
Poiseuille.
Sprung-.
Traube.
V
V
V
o
0.018 142
0.018136
0.01 824
xo
I335I
13271
i 333
20
10 296
10 214
1 032
3°
08 212.
08 186
0819
40
06 718
06725
0 669
Poiseuille’s apparatus for the simultaneous determination of the constants of
viscosity and capillarity, see p. 43, and Ber. d. d. chem. Ges. 19, p. 872, 1886 ;
a recent form of apparatus especially adapted to high temperatures, see Ostwald,
Lehrb. allgem. Chem., 2. Aufl., Bd. I, p. 55°) J^px.
Relation of the constant of viscosity to the constitution of a liquid, see Garten-
meister, Zeit. phys. Chem. 6, p. 524> lB9°> and Handl and Prihram, ibid. 9,
p. 529, 1892. Constant of viscosity for solutions, Arrhenius, Zeit. phys. Chem. I,
p. 285, 1887; Reyher, ibid. 2, p. 744, 1888; Wagner, ibid. 5, p. 31, 1890;
Lauenstein, ibid. 9, p. 417, 1892. Influence of temperature, Gratz, Wied. Ann.
31, p. 25. 1888; Stoel, Phys. Revue I, p. 513, 1892. Tables and earlier literature,
Landolt-Bdrnstein’s Tables, p. 153? 1883.
V. SOLUBILITY.
The solubility is referred either to a constant quantity of the
solvent or, better, to a constant weight or constant volume of the
solution. It may also be referred to the number of molecules.
The solubility of a solid compound is determined by shaking the
solvent for at least two to three hours at constant temperature
with an excess of the powdered substance. SOLUBILITY.
57
The thermostat described by Ostwald (p. 65) may be used for
this purpose. The flask filled with the solvent is placed in the
thermostat; the Raabe turbine may be used to advan-
tage as a stirring apparatus. When the solution in the
thermostat has become perfectly clear, a definite portion is
removed by sucking up into the small pipette (Fig. 23)
proposed by Landolt. The pipette is closed by means of
a glass cap. If the solubility is determined at higher
temperatures, the pipette must be previously warmed.
The quantity of solution is determined from two weigh-
ings of the pipette ; for determining the quantity of dis-
solved substance, the contents of the pipette are washed
into a suitable vessel.
Fig. 23.
The accuracy of the result is determined by conducting a parallel
observation. The relation of the solubility and temperature is
generally represented graphically.
See also the apparatus of Reicher and Van Deventer, Zeit. phys. Chem. 5, p.
560, 1890; for carrying out a huge number of solubility determinations, see the
apparatus ol Noyes, Zeit. phys. Chem. 9, p. 606, 1892; see aLo Schroder, ibid.
11, p. 453 1893. 1 teterm nation of solubility by means of the electric conduc-
tivity. see F. Kohlrausch and Rose, Ber. Beil. Akad. 26, p. 453, 1893.
Solubility tables : Landolt-Bornstein’s Tai les, p. 154 1883.
Solubility of salts, see, among others, Engel, Ann. chim. Bhys. (6) 17, p. 338,
1889; Meyerhoffer, Zeit. phys. Chem. 5, p. 97, 1890; Bodlander, ibid. 7, pp.
315 and 358, 1891 ; Tresor, ibid. 7, p. 469, and Lobry de Bruyn, ibid. 10, p.
782, 1892.
Solubility of organic compounds: Carnelley and Thomson, Jour. Chem. Soc.,
p. 782, 1888.
Apparatus for determining the absorption of gases: Timofejew, Zeit. phys.
Chem. 6, p. X4l, 1S90; L. W. Winkler, Ber. d. d. chem. Ges. 24, p. 89, 1891 ;
Bohr and Bock, Wied. Ann. 44, p. 318, 1891.
Osmotic pressure. Apparatus ; Adie, Jour. Chem. Soc., p. 344, 1891; Tammann,
Zeit. phys. Chem 9, p. 103, 1892, and Walden, ibid. Ij, p. 699, 1892.
Diffusion. Apparatus Scheffer, Zeit. phys. Chem. 2, p. 391, 1888; Chabry,
Jour, der Phys. (2) 7, p. 115, 1888; Stefan, Wiener Monatshefte, 10, p. 201,
1889; Wiedeburg, Wied. Ann. 41, p. 675 ; Arrhenius, Zeit. phys. Chem. XO, p.
52, 1892, and Abegg, 11, p. 249, 1593; Pickering, Phil. Mag. (5) 35, p. 127,
1892.
Reaction, velocity, and chemical equilibrium. Recent literature: Warder,
Ber. d. d. chem. Ges. 14, p. 1361, 1881 ; Reicher, Lieb. Ann. 228, p. 257,1885;
Ostwald, Jour, prakt. Chem. (2) 35, p. 112, 1887; Landolt, Ber. d. d. chem. 58
THE ELECTRIC CONDUCTIVITY OF LIQUIDS.
Ges. 19, p. 1343, l 885; Arrhenius, Zeit. phys. Chem. I, p. 109, 1887, and 4,
p. 226, 1S89; Menschutkin, Zeit. phys. Cliem. i, p. 61 x, 18S7; 5, p. 589, and
6, p. 41, 1890; Bull. Ac. Belg. (3) 31, p. 559, 1891 ; Konowalow, Zeit. phys.
Chem. X, p. 63, 1887, and 2, pp. 6 and 380, 1888; Ostwald, Zeit. phys. Chem.
2, p. 127, 1888; Meyerhoffer, ibid. 2, p. 585 ; Spohr, ibid. 2, p. 194; Giersbach
and Kessler, 'ibid. 2, p. 676; Will and Bredig, Ber. d. d. chem. Ges. 21, p.
2777, 1888; Burchard, ibid. 2, p. 796; Bonz, ibid. 2, p. 865; Lengfeld, Amer.
Chem. Jour. 11, p. 40, 1889; Hecht, Conrad, and Bruckner, Zeit. phys. Chem.
3, p. 450, 1S89; 4, p. 273, 1889; 5, p. 289, IS9O, and 7, p. 274. 1891; Walker,
ibid. 4, p. 3x9, 1889; Fulda, ibid. 6, p. 491, 1890; Montemartini, Rendic. Acc.
Lincei 6, p. 263, 1890; F.vans, Zeit. phys. Chem. 7, p. 337, 1891; Schiikarew,
ibid. 8, p. 76, 1891; Bugarsgky, ibid. 8, p. 398, 1891; Wildermann, ibid. 8, p,
661, 1891; 9, p. 13, 1892 ; Muller and Hausser, Compt. rend. 114, pp. 549 and
760, 1892; Henry, Zeit. phys. Chem. 10, p. 97, 1892; Uno Collan, ibid, xo, p.
130; Trevor, ibid. 10, p. 321, 1892; Hjelt, Ber. d. d. chem. Ges. 24, p. 1236,
1891.
VI. THE ELECTRIC CONDUCTIVITY OF
LIQUIDS.
1. METHOD OF F. KOHLRAUSCH.*
Apparatus and Method in Generals—The method of Kohl-
rausch depends upon the use of alternating currents, in connection
with the Wheatstone bridge.
The element E (Fig. 24) is connected with the induction coil
J, the wires of which are fastened to the measuring bridge B by-
means of binding screws. The circuit of the bridge is made com-
plete by means of a metallic wire which passes through each of
the binding screws and finally to the resistance solution W and
the comparison resistance R. To the binding screw between W
and R is fastened a telephone wire, the other end of which leads
to a movable metallic slide on the bridge.
By closing the circuit the element is set in operation, and the
slide can be placed at such a position on the bridge that no cur-
* Kohlrausch, Wied. Ann. 6, pp. I and 145,1879; 26, p. 161, 1885 ; and 49,
p. 225, 1893; Ostwald, Zeit. phys. Chem. 2, p. 560, 1888. METHOD OF F. KOHLRAUSCH.
59
rent will pass through that part ©f the conductor in which the
telephone is introduced.
The interposed telephone furnishes a means of determining the
proper adjustment, instead of the galvanometer or dynamometer,
in that when the slide is at the proper position the telephone is
either silent or produces a minimum tone which is augmented by
moving the slide in either direc-
tion on the scale of the bridge.
From the position of the slide
corresponding to the minimum
tone, we deduce by means of
Kirchhoff’s laws* the propor-
tion W: R—a\b.
W is the resistance of the
liquid and the electrode vessel;
R is the interposed comparison
resistance ; a and b represent the
number of divisions on the scale
Fig. 24.
of the bridge, to the left and right of the slide when properly ad-
justed. The unknown resistance of the liquid or the reciprocal
value, the electric conductivity, may be calculated from the above
proportion according to page 69.
The Apparatus in Detail.
The Element,—A small Bunsen chromic acid element is
sufficient. For the preparation of 1 1. of solution, 92 gm. of
pulverized potassium bichromate (or a corresponding quantity of
the more soluble sodium salt) and 94 c.c. of concentrated sul-
phuric acid are rubbed together to a uniform pasty liquid ; 900 c.c.
of water are then carefully added while stirring.
The Induction Apparatus,—According to Ostwald, the
smallest induction coil used for medical purposes is best adapted to
this work. The rapidity of the vibration of the interrupter is
increased still further by filing the little block of iron on the
spring down to rather small dimensions (1 or 2 mm.). The mini-
* Ostwald, Ailgem. Chem. I, p. 537, 1885; and Kohlrausch, Prakt. Pliys.
VII, p. 255, 1895. THE ELECTRIC CONDUCTIVITY OF LIQUIDS.
mum tone of the telephone is sharper if the sliding brass tube is
removed from the apparatus.
The sharpness of the telephone depends largely on the nature of
the induction apparatus used,* especially on the speed with which
the current is alternated. If, therefore, the tone-minimum is not
sharp, different induction coils should be tested, and the most
suitable selected.
The Measuring Bridge.—lnstead of the cylindrical bridge f
proposed by Kohlrausch, the bridge which is ordinarily employed
maybe used. The simplest form Jof the same (Fig. 25) is con-
structed as follows;
A paper (or wooden) scale, graduated in millimeters, is fastened
on to a dry board of 110-120 cm. in length and 4—6 cm. in breadth.
A metallic wire is stretched along
the scale by means of the screws
a and ax on the ends of the board.
Two brass plates are fastened by
means of the screws b and b' on
to the board, perpendicular to
Fig. 25.
the scale, so that their inner
edges pass exactly through the
divisions o and xoo on the scale. The screws b and b' serve also
for fastening the wires from the induction apparatus and the resist-
ances.
The bridge wire, which is about 0.2 mm. in diameter, should be
made of perfectly clean German silver, or of platinum containing
iridium. The German silver wire, owing to its gradual oxidation
in the chemical laboratory, gives rise to irregular sounds in the
telephone; the wire should therefore be renewed from time to
time.
For all exact measurements the uniformity of the wire should be
tested and the wire calibrated before use. This may be done by
the method of Strouhal and Bams (p. 73).
* Kohlrausch, Wied. Ann. 6, p. 8, 1879.
f Kohlr.uisch, Wied. Ann. 11, p. 653, 1880.
J A modified form, see Ostwald, Zeit. phys. Chem. 2, p. 562, 1888 ; Wiede-
mann and Ebert, Phys. Prakt. I, p. 385, 1890. METHOD OF F. KOHLRAUSCH.
61
The slide s of the measuring bridge, in its simpler form, con-
sists of a rectangular, bent-down, metal frame with a small binding
screw c, with which the telephone is connected. It is adjusted to
the bridge so that it may be easily moved. In the middle of the
frame and in contact with the bridge wire, is an elastic German
silver needle, the flattened point of which is so constructed that it
is always in perfect contact with the wire. The sensitiveness of
the telephone depends on the kind of contact.*
The Telephone.—Care should be exercised in the choice of
the telephone. The Bell telephone is well adapted to this work.
Ostwald recommends the telephone of Ericsson, in Stockholm, as
being very sensitive.
The sounds proceeding from the induction apparatus are annoy-
ing at first to the unpracticed. A small bulb or some wadding
placed in the ear will remove this inconvenience. One learns
very quickly, however, without this, to distinguish between the
two sounds.
The Comparison Resistance.—Three resistances of 10, 100,
and 1000 units (Ohm or Siemens) are sufficient. More appro-
priate, however, and far more convenient is the use of a complete
resistance-box, the greatest resistance of which amounts to 2000
Siemens-units. By using greater resistances, better results are ob-
tained ; it is better to work with different electrode distances.
The best results are usually obtained with resistances of from 100
to 1000 units.
The resistances should be wound f bifilar, and should be com-
pared, at least twice a year, with a standard resistance; at all
events, one should satisfy himself by testing the apparatus, from
time to time, with solutions of known resistances.
As the resistance varies with the temperature, it is necessary for
accurate determinations to make the small temperature correction
(see p. 70).
The Electrode Vessels.—Three different vessels are used for
f A new kind of winding by Chaperon, Elsas, Wied. Ann. 44, pp. 675
and 678, 1891 ; and F. Kohlrausch, ibid. 49, p. 233, 1893.
* Elsas, Wied. Ann. 44, p. 668, 1891. 62
THE ELECTRIC CONDUCTIVITY OF LIQUIDS.
this purpose, according to the nature of the liquid to be investi-
gated.*
i. For liquids of rather high conductivity (concentrated aqueous
solutions of salts, mineral acids and bases).
For such solutions, use may be made of the vessels employed
by Kohlrausch f (Fig. 26).
Two cylindrical beakers, which are reduced in size at the lower
end, are joined together by means of a tube of about 9 mm. in
diameter. The vessel contains from 12 to 25 c.c. of liquid. The
electrodes consist of platinum, and are soldered to a copper wire
which is introduced through a cover of hard rubber.
2. For liquids of moderate conductivity (dilute aqueous solu
Fig. 26.
Fig. 27.
tions of salts, mineral acids and bases, about -gL to normal;
also concentrated solutions of many organic acids and bases).
The resistance vessel best adapted to such solutions is that pro-
posed by Arrhenius (Fig. 27).
Two circular plates of heavy sheet-platinum from 3to 4 cm. in
diameter are soldered, by means of silver solder and borax, to
heavy copper wires; the distance between the plates should be
about 1.5 cm. The wires are enclosed in narrow glass tubes
* [See also Kohlrausch, Wied. Ann. 51, p. 346, 1894, for special forms of
electrodes and vessels.—Tr.]
f Kohlrausch, Wied. Ann. 6, p. 6,1879. METHOD OF F. KOHLRAUSCH.
63
which are carefully filled with thick liquid asphaltum. The joint
between the platinum and the glass should be well covered with
the asphalt glue. The wires are introduced through a cover
of hard rubber which is fastened by means of a groove on to the
glass cylindrical vessel. It is advantageous to have two such
vessels with the electrodes, 1 and 2 cm. apart.
3. For liquids of low conductivity (most dilute solutions of
organic acids and bases, especially aqueous
solutions of neutral organic compounds, as
well as homogeneous organic liquids and
their mixtures).
For such liquids use is made of very
narrow electrodes with greater surfaces;
the apparatus of Pfeiffer* (Fig. 28) is well
adapted to this work.
Two glass tubes R and Rv of 3 and 3.6
cm. in their outer diameters, are covered to
a length of 13 cm. with platinum foils P1
and P, the smaller tube being covered on
the outside and the larger tube on the inside.
The platinum-foil must form complete
immovable cylinders; these cylinders are
fastened to the outer glass surface by means
of platinum wires. The larger platinum
cylinder (soldered together by means of
silver) is shoved into the wider tube. The
smaller tube, after fusing together at the
top, is then placed in the larger, so that the
two platinum surfaces form concentric cylin-
ders. On account of the large area, the sur-
face of the platinum need not be covered
with platinum-black (see p. 64).
Fig. 28.
The two tubes are then melted together at the bottom, as shown
in the figure; and at the opposite end the outer tube is drawn out
into a narrow neck, in which can be placed a glass stopper G
which, in turn, is covered by the glass covering H. D and D'
* Pfeiffer, Wied. Ann. 25, p. 233, ISBS. 6 4
THE ELECTRIC CONDUCTIVITY OF LIQUIDS.
are the two electrodes leading to the platinum wires fused into B
and Bv The whole vessel (30 cm. high) is supported by means of
the glass tubes fused in at the bottom, which are fastened to the
strong brass foot F.
If a resistance vessel is to be used, it is best to restrict one’s self
to the form proposed by Arrhenius (Fig. 27) which, by the
application of larger resistances, is sufficient for the majority of
liquids.
The electrodes must always have a sufficiently large surface; a
surface which is too small is accompanied by too great a current
density, which frequently produces the phenomenon of polarization ;
the sharpness of the minimum tone depends largely on the frequency
of the replatinizing of the surface.*
For this purpose the electrodes are immersed in a dilute solution
of platinum chloride acidulated with hydrochloric acid, and the
current of a single cell is conducted through, alternating fre-
quently the direction of the current between the electrodes; or a
small piece of zinc is brought in contact with the platinum surface
until the plates are covered with a coating of black, spongy plati-
num.
According to Grotrian,f the well-platinized electrodes should
be saturated with hydrogen by immersing them as kathode in
dilute sulphuric acid. It is especially necessary that the electrodes
be well platinized.
The Thermostat.—On account of the great influence of
temperature on conductivity,J an accurate measurement of the
temperature is very important.
Although Kohlrausch § has observed an influence of liquid
baths on the minimum tone, and therefore made his determinations
in air at the temperature of the room, yet the following, essen-
* Kohlrausch, Pogg. Ann. 148, p. 143, 1873, and ibid. 49, p. 235, 1893.
•(• Wershofen, Zeit. phys. Chem. 5, p. 486, 1890.
J For most electrolytes, a change of one degree Celsius changes the conduc-
tivity about two percent.
$ Kohlrausch, Wied. Ann. 26, pp. 172 and 184, 1885; Kohlrausch also ob-
served that the telephone, if too near the apparatus, was influenced by the
induction coil. See also Kohlrausch, Wied. Ann. 49, pp. 242 and 247, 1893. METHOD OF F. KOHLRAUSCH.
65
tially the arrangement proposed by Ostwald (Fig. 30), is to be
preferred for convenience.
The electrode vessel is supported in the iron water-bath A of
10 to 20 I. capacity, by means of a half-circular wooden cover.
A temperature regulator B, constructed in the ordinary manner,
is fastened to this water-bath as shown in figure 30.
The regulator consists of a U-tube in which is fastened, by
means of a rubber stopper, a cylindrical tube C. This tube (Fig.
30) is filled with oil or a concentrated solution of calcium
chloride, and then connected with the U-tube (Fig. 29). A
Fig. 29.
Fig. 30.
sufficient quantity of mercury is then conducted in through the
funnel, after which, by suitably inclining the U-tube, the air in
the part between the mercury and the funnel is completely
replaced by oil or calcium chloride solution. The inflow and
outflow of gas is indicated by the direction of the arrows.
To increase the sensibility, the inner portion of the gas-inlet
tube is cut off at right angles. A very small side-opening in the
same prevents the putting-out of the flame. By conducting in or
removing liquid, by means of the funnel, the position of the top of
the mercury column near the gas-inlet tube can be so regulated that
widely varying temperatures may be obtained. 66
THE ELECTRIC CONDUCTIVITY OF LIQUIDS.
As a motor, the windmill of Ostwald * may he used. It is
advantageous in this case to have the fans made of thin aluminium
plates.
The use, however, of Raabe’s turbine seems to me, in general,
to be more appropriate. The everywhere purchaseable turbine D,
after thoroughly oiling the parts of the apparatus, is connected by
means of a cork to a double wheel E, which turns on a brass
axis. From E the motion is transferred to a smaller wheel or, as
in the figure, directly to the stirrer which consists of a glass rod
fastened to E and provided at the lower end with a glass or
wooden paddle ; the glass rod rotates in a wider, well-oiled glass
tube. By employing this thermostat, it is possible to maintain the
temperature constant to 0.05°. For temperatures of 50° and over,
the water is covered with a layer of paraffin ; for temperatures above
Bo°, an altered thermostat is used as described by Bersch.f
The Contact.—The connection of the different parts of the
apparatus is made by means of strong copper wires, which are as
short as possible and fastened to suitable metallic clamps. A
perfect contact is, above all, very important. The places of con-
tact of the wires and the binding screws are carefully cleaned from
time to time with a file and sand-paper; the binding screws should
be well tightened, the stopper placed firmly in the rheostat, and the
needle of the slide brought in good contact with the wire of the
bridge. The contact with the electrode wires is made by means
of small cups of mercury which, like the electrode vessel, are
placed in the opening of the wooden cover of the thermostat. The
copper wire of the electrodes should be carefully cleaned, moistened
with hydrochloric acid and immersed in the mercury.
The Nature of Liquids to be Examined.
Water.—For establishing the conductivity, aqueous solutions
are of prime importance; it is necessary, therefore, to exercise
special care in the selection of the water to be employed. Water
exhibits very different degrees of conductivity, depending upon
* Ostwald, Zeit. phys. Chem. 2, p. 565, 18S8.
f Bersch, Zeit. phys. Chem. 8, p. 384, 1891. METHOD OF F. KOHLRAUSCH.
67
the manner of distillation and preservation, while perfectly pure
distilled water exhibits an extremely low conductivity.
The purest water obtained by Kohlrausch in a platinum appa-
ratus had a conductivity of /£ = 0.25 X xo~10, compared with the
mercury unit of o° = 108 ; however, it is sufficient, in general, to
have water for which k i.io-10 to 2. xo—I°. For the meaning of
k, see page 70.
in a distillation apparatus with a tinned coiled tube.* Such water
preserves (or diminishes) its conductivity if it is placed in a glass
'The distillation of water, according to Kohlrausch, is carried on
flask which has been used for a long time for distilled water.
In the investigations of liquids of high conductivity (concen-
trated salt solutions) the correction f for the conductivity of the
water employed may be neglected ; on the other hand, with dilute
salt solutions and other aqueous liquids of low conductivity, the
conductivity of the water must be first determined, just as that of a
solution (see p. 69), and taken into account. For solutions of
very low conductivity—e.g., neutral organic compounds—the cor-
rection, which can be only imperfectly determined, is so great that,
even with the greater sharpness of the minimum tone, an exact
determination of the conductivity is not possible.
Solutions.—The substances employed must be pure, as the
conductivity is often influenced by very slight traces of impurities.
The conductivity for acids, bases and salts is referred to the
number of equivalents in one liter of solution ; Ostwald denotes
with v 32, 64 1024 those concentrations which contain
¥2> wt • • • • ttjW equivalent weights in grams, in one liter of
solution. For chemical purposes, solutions of v—32to v 1024
are usually employed.
The introduction of the previously warmed solution into the
electrode vessel is best accomplished after the solution has been
* Kohlrausch, Wied. Ann. 26, p. 170,1885 ; Kohlrausch and G otrian, Fogg.
Ann. 154, p. 3, 1875; Kohlrausch, Wied. Ann. 6, pp. 36 and 49, 1879, and
11, p. 653, 1880. Nernst, Zeit. phys. Chem. 8, p. 120, 1891, obtained water of
k 2.10—10 by freezing ordinary distilled water; Van’t Hoff and Reicher, Zeit.
phys. Chem. 2, p. 778, ISBB.
j- Kohlrausch, Wied. Ann. 26, p. 191, 1885. 68
THE ELECTRIC CONDUCTIVITY OF LIQUIDS.
prepared ready for the experiment. However, the different dilu-
tions can be obtained (of course, somewhat less accurately) in the
resistance vessel. To accomplish this, half of the solution is
removed by means of a suitable pipette, and an equal quantity of
previously warmed water added. In this manner the dilution is
increased two-, four-, eightfold, etc.
All solutions must be investigated in a fresh condition, for the
conductivity of solutions of most organic compounds as well as
many mineral salts, acids and bases, after twenty-four hours,
shows, for unknown reasons, a variation.*
For dilute solutions of acids and bases (HCI, H2S04. C 2H+02,
KOH, NaOH, NH3), Kohlrausch f has shown that at the elec-
trode there is a noticeable absorption of the substance, which
apparently does not take place with neutral salts. This absorption
produces, after a time, a perfect constancy in the minimum tone.
If this phenomenon is of a general nature, and depends upon a real
change in the concentration of the liquid, the inconvenience can,
as suggested by Kohlrausch, be removed only by using larger
resistance vessels of about 500 c.c. capacity.
Method of Operation.—As soon as the liquid takes on the
temperature of the thermostat, the element is set in operation and
the slide given such a position that the telephone is either silent
or produces a minimum tone, the intensity of which increases with
the least movement of the slide in either direction. In general,
the adjustment is made so sharply that the two points on the scale
at which an increase of tone may be distinctly recognized are not
more than 2 mm. apart. Midway between these points is the
correct position which, after some practice, can easily be deter-
mined accurately to from 0.2 to 0.3 ram. The resistances are so
inserted that the slide, when adjusted, will be near the middle of
the measuring bridge ; an error of 0.3 mm. in the adjustment here
will produce an error of about o. 1 per cent, in the value of the
conductivity.
Each determination should be repeated by inserting different
resistances, and the mean value taken as the basis of the calculation.
* Kohlrausch, Wied. Ann. 26, p. 175, 1885.
f Kohlrausch, ibid. 26, p. 220, 1885. METHOD OF F. KOHLRAUSCH.
69
An indistinctness in the minimum tone may, as already sug-
gested, be due to very different causes. The difficulty is usually
removed by replatinizing the electrodes ; sometimes an increase in
the electrode surface is necessary, varying according to the concen-
tration and nature of the solution, as well as the amount of resist-
ance inserted; frequently also, a more rapid alternation of the
current is necessary, and in many cases the cause lies in the
amount of resistance. A resistance of from 100 to 1000 mercury
units gives, in general, the best results.
After a little practice, ten to twelve solutions may easily be
investigated in one-half an hour.
Calculation.—'The measurements for chemical purposes are
limited almost wholly, in recent times, to the determination of the
molecular conductivity represented by the constant // (or X, accord-
ing to Kohlrausch). For the meaning of this constant, see Ost-
wald, Allgem. Chem., 2. Aufl., Bd. 11, p. 640, 1893; and Kohl-
rausch, Wied. Ann. 6, p. 152, 1879, and 26, p. 163, 1885.
p. is calculated from the formula:
v b
Hv 7 ;
r a
or, for aqueous solutions, taking into account the conductivity of
the water employed, according to the formula:
/ b bw \ *
P* = vyl I,
\a 7■ a rw }
where p. represents the molecular conductivity at the dilution v;
v the volume in liters, which contains one gram equivalent f of the
electrolyte;
a and b the lengths of wire to the left and right of the slide;
aw and bw the corresponding lengths for water;
rand rw the resistances in mercury units of the solution and the
water;
y the resistance capacity of the measuring vessel.
* The formula follows directly from the proportion (p. 59b The correction
for the conductivity of water is somewhat uncertain ; for solutions of low conduc-
tivity the value of p is doubtful.
f It is better to refer the conductivity to a gram-molecule of the substance, as
i lis impossible to separate acids, bases, salts, eic., from indifferent substances. THE ELECTRIC CONDUCTIVITY OF LIQUIDS.
In order to determine the resistance capacity of the vessel,—i. e.,
the resistance which a liquid with unit conductivity would show in
the vessel,—a liquid is used whose conductivity is accurately known.
A normal calcium chloride solution which has kept for a long
time unchanged has, according to Kohlrausch, a molecular conduc-
tivity at xB° of 112.2, and at 250 = 129.7. This value placed in
the above formula will give the value of the constant y. For
liquids of low conductivity and narrow electrodes, it is better to
take a more accurately investigated solution of low conductivity,—
e.g., a solution of tartaric acid.
The molecular conductivity/* at 250 is according to Ostwald * :
v 16 32 64 128 256 512 1024 2048
p 11.40 16.03 22.47 3*-28 43-5° 59-51 81.64 109.50.
Other suggestions see Kohlrausch, Wied. Ann. 6, pp. 49 and
50, 1879, and Kohlrausch, Prakt. Phys. vn, p. 304, 1892.
The reduction of the specific conductivity k to terms of // fol-
lows from the relation p 107 k• v, where p and v have the meaning
given above (Ostwald, Jour, prakt. Chem. N. F. 33, p. 353, 1886).
The ratio ~ is given for a wire 1 m. long in the table of Obach.
An abbreviated form of this table is given at end of this book.
If the resistance of the wire is not uniform, the wire must be cali-
brated, and a corresponding correction applied to the above value.
The resistance r also requires a small correction. For most
ordinary German-silver wires, an increase of i° in temperature
increases the resistance on an average of 0.0004 parts of the whole
value. The necessary reduction to mercury units at o° is easily
made.
If one wishes (which is not always permissible) to establish the
value poo ,-—i. e., the conductivity at infinite dilution,—it is deter-
mined indirectly, inasmuch as it does not result from direct obser-
vation. Zeit. phys. Chem. 2, p. 843, 1888. For the calculation
of the Ostwald constant,—
K = . 100
(l m) v
(see Zeit. phys. Chem. 2, p. 278, 1888).
*Ostwald, Zeit. phys. Chem. 3, p. 272, 1889. METHOD OF F. KOHLRAUSCH.
71
The value of /j. is usually determined at the temperature 250
(the measurements of Kohlrausch were referred to 180 C.). On the
temperature influence or the calculation of the temperature coeffi-
cient, see Kohlrausch, Wied. Ann. 6, p. 14, 1879, and 26, p. 222,
1885. If the determinations are made at higher temperatures, the
error due to the dissolving of the glass must be taken into account.
It is therefore advantageous to boil water in the electrode vessel
several times before use. Arrhenius, Zeit. phys. Chem. 4, p. 96,
1889; Krannhals, ibid. 5, p. 251, 1891; and Sack, Wied. Ann.
43, p. 212, 1891.
For the calculation of the velocity of ions and the transport
numbers from the conductivity, see Kohlrausch, Wied. Ann. 6, p.
160, 1879, and 26, p. 170, 1885; Lob and Nernst, Zeit. phys.
Chem, 2, p. 948, 1888 ; Kistiakowsky, ibid. 6, p. 105, 1890; and
Bein, Wied. Ann. 46, p. 29, 1892.
Instead of the method of Kohlrausch, another method is usually
employed in France (Lippman’s capillary electrometer, Wiede-
mann, Elektrizitiit 1, pp. 468 and 480, 1882 ; Compt. rend. 83, p.
192, 1876 ; and Ann. chim. phys. (6) 3, p. 439, 1884, and ibid.-
(6) 23, p. 5, 1891).
Applications of Conductivity.—Organic liquids and their
mixtures show such a low conductivity* that this constant, in such
cases, is of little significance. The same is true for aqueous solu-
tions of most indifferent compounds ; here the imperfect correction
for the conductivity of water makes an exact determination very
difficult.
For chemical purposes, the conductivity of aqueous solutions of
inorganic and also organic salts, acids and bases is of special
importance.
1. The constant of molecular conductivity is, to a remarkable
degree, a constitutive property, i. e., it depends upon the manner
in which the atoms are linked together. Isomeric compounds
seldom show equal conductivities. Important discriminations are
also possible in stereochemical considerations. On the relation of
conductivity to constitution, see Ostwald, Jour, prakt. Chem.
N. F. 30, pp. 93 and 225, 1884 ; 31, p. 433, and 32, p. 300, 1885 ;
* Walden, Zeit. phys. Chem. 8, p. 434, 1891. 72
THE ELECTRIC CONDUCTIVITY OF LIQUIDS.
33, p. 352, 1886 ; Zeit. phys. Chem. : Ostwald, 1, pp. 74 and 97,
1887; 3, p. 170; ibid. p. 241; ibid. p. 369, 1889; Bethmann,
5» P- 385, 1890; Bader, 6, p. 289, 1890; Walden, 8, p. 453,
1891 ; 10, pp. 563 and 638, 1892 ; Berthelot, Compt. rend. 102,
p. 46, 1891, and Ann. chim. phys. (6) 23, p. 5, 1891.
2. The determination of the conductivity establishes, in most
cases, the basicity of the acid. The difference between the values
of p.wu and (v = 1024 and 32) amounts to:
for monobasic acids A = about 10
“ dibasic “ A = “ 18-20
“ triba-ic “ A = “ 28—31
“ tetrabasic “ A = “ 40
“ pentubasic “ A = “ 50
Walden, Zeit. phys. Chem. 1, p. 529, 1887, and 2, p. 19, 1888,
and Ostwald, Zeit. phys. Chem. 2, p. 901, 1888.
3. The remarkable degree to which this constant may be in-
fluenced, and the large differences of the same for different com-
pounds makes possible;
(<2) The determination of the presence of very small quantities
of impurities in a definite compound (example, water, p. 67) ;
(b) a very sharp determination of the concentration, often at*
very high dilutions (Kohlrausch, Ber. d. d. chem. Ges. 24, p.
3560, 1891) ;
(c) the approximate quantitative determination of small quan-
tities of electrolytes in mixtures or solutions with large quantities
of substances of rather low conductivity (Fock, Fresen. Zeit. 28,
p. 1, 1889, and 29. p. 35, 1890, and Reichert, ibid. 28, p. 7,
1889; Arrhenius, Zeitschr. phys. Chem. 9, p. 510, 1892) ;
(r/) the determination of the solubility of sparingly soluble com-
pounds in water. (F. Kohlrausch and Rose, Ber. Berl. Akad. 26,
P- 453> i 893-)
4. The conductivity is of special interest, on account of its
close relation to many other properties; examples: the reaction
velocity, dissociation phenomena, freezing point, vapor tension,
diffusion, capillarity, viscosity, etc. See :
Ostwald, Grundriss d. allgem. Chem. ir, p. 363, 1890; also Zeit. phys. Chem.
Bd. I—x ; van ’t Hoff, ibid. I, p. 481, 1887; Anhenius, ibid. p. 631.
Measurement of electromotive force; Kohlrausch, Prakt. Phys. vii, p, 311, CALIBRATION OF A WIRE.
73
1892; Wiedemann and Ebert, Phys. Prakt. I, p. 395, 1890; Ostwald, Lehrb.
Allgem. Chem. 11, p. 808, 1893 ; Ostwald, Zeit. phys. Chem. 1, p. 403, 1887 ;
Behrend, ibid. n, p. 469, 1893, and Brandenburg, ibid. 11, p. 552.
Measurement of current-strength : Kohlrausch, Prakt. Phys. vn, p. 262,1892 ;
Wiedemann and Ebert, Phys. Prakt. 1, p. 403, 1890; Glazebrook and Schaw,
Phys. Prakt. I, p. 387, 1888.
2. CALIBRATION OF A WIRE (Method of Strouhal
and Barus).*
Let E (Fig. 31) represent an element, and AMB the bridge
with the wire to be calibrated; I, 11, 111, IV, Y are a number of
nearly equal comparison resistances which, for a simple adjustment,
are supported in the following manner:
A German-silver wire of suitable thickness and length is divided
into n, in figure = 5, nearly equal parts, which are soldered into
Fig. 31.
short, heavy, amalgamated copper wires. The wires are connected
by means of the mercury cups 1, 2, 3 . . . , ; the — 1
and B 6 are made by means of heavy copper wires.
The one end iVof the wire M N, which passes through a sensitive
reflecting galvanometer, is placed successively in the cups 1 and 2,
and the two positions J/j and M 2 on the bridge, for which the
galvanometer shows no deflection, are determined. The wires I
and II are then exchanged, so that I is in the position of 11, after
* Strouhal and Bams, Wied. Ann. xo, p. 326, 18S0.
6 74
THE ELECTRIC CONDUCTIVITY OF LIQUIDS.
which the wire NM is placed in 2 and 3, and the positions M'„
and M% determined on the bridge, where the galvanometer shows
no current. The wire lis then moved farther up, in that it is
exchanged for 111 ; Wis immersed in 3 and 4, and the two posi-
tions M'3 and Mi on the bridge where the galvanometer shows no
current is determined.
In this manner the bridge wire is divided into n, in the present
case = 5 distances, Mx M 2; M'2 M 3; M\ .... which, with
the above arrangement of the circuit, are all proportional to the
same resistance I.
If these lengths of equal resistances are represented in scale
divisions by ax; a 2; a3 . . . an, the mean length
a\ ~t~ a 2 ~1~ aS ~t~ • • • an
n
The bridge scale is 1000 mm. in length, and the number of
resistances is so chosen that a = -°°° is a whole number; then the
n
values axa2a3 . . . differ from the calibration interval a only by
the very small values i\ d 2 d 3 . . .
We have then :
al = a -1-
a 9 = a + d 2
an a -f- 6n
and likewise the mean value of the observed resistances
a\ + +•• • an |
—i—l ?—! _L ~ a f a.
n
Then
a ~h ~h •• • tin.
n
and therefore the correction table for the wire is :
From o— a a
“ a— 2 a a— d 2
“ 2a 2>a a— 3, etc.
summation we have ;
For a the coirection a (5j
“2 a “ 2a dj <52
“ 3a “ 3a —(\— J2 etc. EXPANSION OF LIQUIDS.
75
For exact measurements," instead of five comparison resistances,
nis taken equal to 10 or 20. By representing the corrections and
the scale divisions graphically, it is an easy matter to determine
the correction for any point on the scale. Instead of a constant
current and galvanometer it is perhaps better to use an alternating
current and telephone.* Large variations in the temperature of
the room may occasion errors, f
VII. THE EXPANSION OF LIQUIDS.
The coefficient of linear expansion is the change in length per
unit length of a body at o° for a change of i° in temperature.
The coefficient of cubical expansion is the change of volume
per unit volume at o° for a change of i° in temperature.
The coefficient of cubical expansion of a body is very nearly
equal to three times the linear expansion /?c=r 3 /?,.
The coefficient of expansion usually increases with the tempera-
ture. By the mean coefficient of expansion of a liquid for the
temperature interval tx / is meant, the change per unit volume for
i°, on the supposition that the expansion is uniform for each tem-
perature interval. For expansion coefficients see Ostwald, Lehrb.
Allgem. Chem., 2. Aufl., Bd. 1, p. 279, 1891.
Expansion of solids, Kohlrausch, Prakt. Phys. vu, p. 95, 1892,
and Wiedemann and Ebert, Phys. Prakt., p. 134, 1890.
Expansion of gases, Wiedemann and Ebert, ibid. p. 78.
* Ostwald, Lehrb. Allgem. Chem. n, p. 629, 1893.
[f Closely related to the chapter on conductivities is the determination of the
dielectric constant of liquids, which in recent years has become of considerable
importance in chemistry. For the determination of this constant see especially
method XI of Drude, Zeit. phys. Chem. 23, p. 282, 1897.—Tr.] 76
EXPANSION OF GLASS AND LIQUIDS.
DETERMINATION OF THE COEFFICIENT OF
CUBICAL EXPANSION OF GLASS
AND LIQUIDS.
Let and sx represent the specific gravities, v and vx the volumes
of a liquid at the temperatures / and /, and let a represent the
coefficient of cubical expansion, then we have the equations;
vx v [l -)- a (/i /)] or
Vy V
a= 1 ,
v to o
and likewise
J S-,
a = L~.
h {*l—*)
Hence the coefficient of cubical expansion may be calculated from
two determinations of the density or specific volume for the given
temperature interval; on the other hand, the values vx and sx may
be calculated if v and and also a are known.
The coefficient of cubical expansion is usually calculated accord-
ing to the following equation :*
a= ZP A +_JL_
Pi h * Pi
where p and px represent the weights of the liquid contained in
the pyknometer (Fig. 32 or Fig. 33)f at the temperature / and the
higher temperature tx\ 3/5 is the coefficient of cubical expansion of
glass. If 3/? is known, then two weighings of the pyknometer at
the temperatures / and tx are sufficient for the determination of «.
For ordinary glass 3 /S can be placed, on an average, equal to
0.000025 ; for Jena glass, very nearly 0.0000237.
If 3/9 is to be determined, the pyknometer (Fig. 32 or Fig. 33)
is filled with pure mercury and weighed at two different tempera-
tures. If the coefficient of the cubical expansion of mercury is
placed equal to 0.000182, then from the above formula we have :
38— o . 000182 * tl
P tx —l p
* Kohlrausch, Prakt. Phys. vn, p. 97, 1892.
•j- The pyknometer described in the chapter on Specific Gravity may also be
used. COEFFICIENT OF CUBICAL EXPANSION.
77
To fill the pyknometer, the point is immersed in recently boiled
mercury ; by carefully heating and cooling the pyknometer, whereby
the mercury is slowly heated to boiling, the vessel is completely
filled.
If the pyknometer (Fig. 32) is used, it is placed in a thermostat
(p. 65) and heated to two different temperatures.
Fig. 32.
Fig. 33.
Fig. 34.
The pyknometer (Fig. 33), on the contrary, is heated in the
vapor of boiling ether and water in the arrangement shown in
figure 34 (= one-half natural size). (Method of R. Schiff.*)
The pyknometer is placed, by means of an iron spoon, in a pear-
shaped vessel, which is heated by the vapor of the boiling liquid in
* K. Schiff, Ber. d. d. chem. Ges. 18, p. 1539, 1885. EXPANSION OF GLASS AND LIQUIDS.
the vessel below. The pyknometer carries a covering with a glass
tube, the form of which is shown in the figure, and into which,
when lowered, the liquid passes which overflows from the pyknom-
eter. The side openings at the top of the vapor chamber are for a
thermometer and a return condenser.
The volume of the pyknometer at 34° is obtained from the
weight of the mercury contained in it after heating in boiling
ether;* and then by weighing a second time after heating in
aqueous vapor, the coefficient of expansion 3 /9 can be calculated.
The volume at o°, v 0 can be approximately calculated from the
formula:
».= V-
I + 3^-t
If the coefficient of expansion of the vessel is known, the coeffi-
cient of the cubical expansion of the liquid to be investigated is
calculated according to page 76. The filled pyknometer is heated
in the vapors of liquids adapted to this work.
The determination of the coefficient of the cubical expansion of
glass can also be made by the use of the same formula with water
free from air. The mean coefficient of expansion of water between
the temperatures t and t1 is calculated j according to the equation ;
Vx V S 5*2
v(tx —t) ~sx (ifa t)
The pyknometer and method (p. 28) are also applicable.
On the dilatometric method see, among others, Kohlrausch,
Prakt. Phys. vn, p. 97, 1890; Lachowitz, Ber. 21, p. 2206, 1888;
Bremer, Zeit. phys. Chem. 3, p. 424, 1888; Knofler, Dissert.,
Erlangen, 1888, and Thorpe, Jour. Chem. Soc. 63, p. 262, 1893.
The pyknometric methods, however, are in general to be preferred.
General.—If the expansion of a liquid is to be established, the
coefficients of expansion for different temperature intervals are
determined, and the relation of a and t represented by means of
equations of the form a. = a -j- b t and a— a -|- b t -j- c /2, in
which the constants a, b, and c are determined by substituting the
corresponding values of a and t.
* Landolt-Bornstein, Phys. chem. Tabellen, pp. 36 and 37, 1883.
f Landolt-Bornstein, ibid. pp. 33-35, 1883. MELTING POINT AND SOLIDIFYING POINT.
79
It is frequently the case that only the specific gravities and
specific volumes are given, and the dependence of these two
values upon the temperature represented by the interpolation
formulas st (i -j- a t -f- b t2) and vt =vQ (i -f- a t -|- b t2),
where st and vt represent the specific gravity and volume at t°, and
j-0 and t0 the corresponding values at o°. The calculation of the
constants is best made by the method of least squares.* The
true coefficient of expansion then is ;
1 d v , „, , ,
- • a 2b t -f- .
v„ at
Frequently the calculation is made according to the formula of
Mendelejeff:
v 0
Vt = T=Tf
in which k is a characteristic constant which can be determined by
substituting the values of vO, vt, and t. The results, however, from
this formula do not agree in all cases. Konowalow, Zeit. phys.
Chem. i, p. 39, 1887, and 2, p. 1, 1888; Grimaldi, ibid. 1, p.
550, 1887, and 2, p. 374, 1888, and Heilborn, ibid. 6, p. 578,
1890, and 7, p. 367, 1891. Ibid., see tables of the expansion of
organic liquids; for tables of the expansion of salt solutions see
Gerlach, Spez. Gewichte der Salzldsungen, Freiburg, 1859, and
Tschernai, J. russ. Ges., pp. 430 and 486, 1888 ; reference, Zeit.
phys. Chem. 4, p. 483, 1889.
VIII. THE MELTING POINT AND SOLIDIFYING
POINT, f
Method I.—For large quantities of substance use is made of
the following arrangement:
A cylinder about 3 cm. wide, which is provided with a carefully
*Kohlrausch, Prakt. Phys. VII, p. 10, 1892.
j Landolt, Zeit. phys. Chem. 4, p. 353, 1889. MELTING POINT AND SOLIDIFYING POINT.
tested thermometer and a stirrer, and containing at least 15 to 20
gm. of the substance, is placed in a large beaker glass which con-
tains a suitable heated liquid (water, concentrated solutions of
sodium chloride or calcium chloride, paraffin, oil).
The hot liquid is heated for some time to a temperature above
the probable melting point, estimated, if necessary, by a previous
investigation of the substance. As soon as a portion of the sub-
stance is melted, the stirrer, a glass rod bent into a glass ring, is
moved constantly. If a thermostat with a stirring arrangement *
is used instead of an ordinary water-bath, the temperature may be
regulated still more accurately.
The thermometer (as long as sufficient quantities of solid sub-
stance is found with the molten material) is kept at a constant
temperature for several minutes, or for a longer time when larger
quantities of material are used. The necessary corrections to the
observed melting point (due to the thread of mercury which pro-
jects above the surface, etc., must not be neglected ; an accuracy
of o.i° C. or less may be easily attained.
The solidifying point which comes into question, especially with
mixtures of substances, is determined in the same apparatus.
After melting the substance the temperature of the surrounding
water-bath (thermostat) is kept constant for some time at from 1 to
20 below the melting point of the substance. By throwing a small
crystal into the molten substance, the solidification is brought about
and the temperature is then read off. The determination of the
solidifying point requires that the temperature be held constant for
a longer time, and, in general, that larger quantities of material be
used than for the determination of the melting point. Twenty gm.
are here scarcely sufficient.
By using from 100 to 1000 gm. of substance, the melting point
as well as the solidifying point can be kept constant for an hour.
The least impurities frequently have great influence on the melt-
ing point; the substances should therefore be carefully purified.
Substance for investigation : Naphthalene, melting point = sol-
idifying point = 80.03° C.
Method II.—It frequently happens that only a small quantity
* Page 65, and Kiister, Zeit. phys. Chem. 8, p. 578, 1891. DEPRESSION OF THE FREEZING POINT OF SOLUTIONS.
of the substance can be, had for the investigation. In such cases
it is better to make use of the following much used but inaccurate
method for determining melting points :
A vessel A (Fig. 35) is filled to the height shown in
the figure with pure concentrated sulphuric acid, in which
is immersed a thermometer on which is fastened, by means
of platinum foil and platinum wire, a capillary tube
closed at the lower end ; the two are so joined that the
small portion of substance introduced into the bottom
of the small tube lies in the immediate vicinity of the
mercury bulb of the thermometer.
The vessel is slowly and carefully heated, and the
temperature at which the substance begins to melt away
from the walls of the tube is taken as the melting point.
The values observed for the melting point show varia-
fig. 35-
tions of from Ito 20, depending upon the width of the tube; with
very narrow tubes the results are too high. The results are some-
what concordant if the tubes used are always of the same diameter,
about 1.5 mm. at the lower part.
IX. DEPRESSION OF THE FREEZING POINT
OF SOLUTIONS.
Principle.—The freezing point of the solvent and the solution
of known concentration are determined; the difference between
these two temperatures is the depression of the freezing point, from
which the molecular weight of the dissolved substance may be
calculated according to page 89.
1. METHOD OF BECKMANN.*
Apparatus (Fig. 36).—The inner tube A, which is provided
with a thermometer and stirrer, and also a side tube, contains the
liquid, the freezing point of which is to be determined.
* Beckmann, Zeit. pliys. Cliem. 2, pp. 638 and 715, 1887, and 7, p- 323> *B9l. 82
DEPRESSION OF THE FREEZING POINT OF SOLUTIONS.
A is fastened by means of a cork in the wider tube B, which in
turn is supported, by means of a metallic cover, in the outer glass
vessel C (from 2 to 3 1. capacity).
The vessel C, which is provided with
a stirrer, contains the freezing mixture.
Between B and A is a layer of air which
separates the liquid to be frozen from
the freezing mixture, and consequently
allows the liquid to cool uniformly and
gradually.
For accurate determinations the ther-
mometer must be graduated to or yiy
of a degree. A Beckmann thermometer
is well adapted to this work. The mer-
cury reservoir at the top is so large that
the thermometer will also answer for deter-
minations according to the boiling point
method. The stirrer for the inner vessel
should be made of platinum; a ring of
platinum foil is soldered to a thick plati-
num wire. A glass stirrer, however, may
be used without any special disadvantage.
If the inner vessel is to be closed at the
top, the stirrer may be moved through a
cork or rubber stopper.
Method of Operation.—For accu-
rate determinations the apparatus should
be set up in a room, the temperature of
which differs not more than one degree
from the freezing point of the solvent.
A temperature difference of io° may
influence the depression of the freezing
point as much as o.oi°.
Fig. 36.
The temperature of the freezing mix-
ture should be from 3 to 40 below the freezing point of the liquid to
be investigated. The result is influenced if the temperature for one
observation is allowed to vary more than 1 to 20 from that of the
other observations with the same solvent and solution. METHOD OF BECKMANN.
83
For aqueous solutions, suitable mixtures of snow or ice and salt
water may be used for cooling; when working with benzene (melt-
ing point about 5-4°) a mixture of water and ice is sufficient,
regardless of the concentration of the solution ; for acetic acid
(melting point 16.70) the temperature of the surrounding water
may be lowered by means of small pieces of ice; for solutions in
phenol (solidifying point 40° to 410) and naphthalene (solidifying
point 80.o°), use is made of a thermostat (p. 65) or a beaker
glass, by means of which the solidifying point of the molten sub-
stance may be determined according to page 79.
The freezing point of the solvent is determined in the following
manner:
Tube A is provided with a sharp-edged piece of platinum, tared,
and supplied with about 15 gm. of the solvent, so that the upper
part of the tube remains dry. The quantity of solvent is then
accurately weighed to one centigram.
After placing in the apparatus the liquid, during constant stir-
ring, is cooled to near the freezing temperature, and the freezing
induced by means of a crystal of the solvent. The thermometer
falls usually several tenths of a degree below the freezing point,
rises immediately after the beginning of the crystallization, and
after thirty to sixty seconds—with sufficient separation of ice—
attains a maximum which is taken as the freezing point of the
solvent.
The degree of over-cooling may slightly influence the accuracy
of the result (to 0.02°); the over-cooling, therefore, for the
parallel observations with the solution and solvent should be regu-
lated as uniformly as possible (about o.i° below the freezing
point). This is usually accomplished by introducing the ice
crystal which induces the freezing, at correspondingly equal tem-
perature intervals from the freezing point. For water and dilute
aqueous solutions it is desirable that the over-cooling should be
0.50, on account of the otherwise insufficient separation of ice;
for concentrated aqueous solutions, on the other hand, the over-
cooling must not be more than 0.20.
If acetic acid is used, its hygroscopic properties must be taken
into consideration for accurate determinations. Tube Ais then
provided with a stopper. The error, however, introduced by the 84
DEPRESSION OF THE FREEZING POINT OF SOLUTIONS
absorption of water amounts to scarcely more than o.oi° in the
reading of the thermometer.*
The solvents, especially acetic acid, benzene, and others should
be used only in a pure condition.
After determining the freezing point of the solvent, which
should be done before and after each series of observations, the
substance to be dissolved is introduced through the side tube into
the tube A.
Solids are weighed off in small glass tubes, by means of which
they are introduced into the solvent, or they may be introduced in
Fig. 37.
the form of pastilles, which are prepared by means of a pastille
press.
For the introduction of liquids, the pipette (Fig. 37) may be
used. By means of this arrangement the liquid is blown into the
freezing tube. If the capillary tube is very thin-walled and
ground off sloping at the outlet, no drop will remain hanging; the
pipette then needs only to be weighed before and after the removal
of the liquid. The determination of the freezing point of the
solution follows, just as for the pure solvent.
*The use of the recent complicated apparatus of Beckmann (Zeit. phys.
Chem. 7, p. 324, 1891) is unnecessary in this case. For difficultly soluble sub-
stances the solution is prepared (if necessary with exclusion of the outer air), and
observed according to the method of Raoult (p. 86). METHOD OF BECKMANN.
85
The introduction of crystals to induce the freezing is, especially
during the warm months, attended with difficulty. Small crystals
melt too quickly and larger crystals give rise to too great a change
in concentration. Beckmann recommends for that purpose the
contrivance (“ Impfstift ”) represented in figure 38.
A portion of the liquid in A is sucked up into the narrow tube
B, which is open at the lower end and closed at the upper end by
means of a pinch-cock, and the whole placed
in a freezing mixture and brought to freezing.
B is then removed from A, and the substance
thawed a little by slightly warming the walls of
the tube at the bottom and afterward above.
A momentary opening of the pinch-cock C is
sufficient to remove the cylindrical substance
from the open end of the tube. The small
quantity of projecting substance may be
brought into the freezing liquid by means of
the stirrer.
The method of Beckmann is used if an ap-
proximate determination of the molecular
weight is desired; the limit of accuracy is
about five per cent, of the calculated value
of the molecular weight. The change of
concentration gives rise to errors; over-cool-
ing of more than o.i° is, therefore, especially
for concentrated solutions, to be avoided.
An advantage of the method is the small
quantity of substance required for a molecular
weight determination.
Inasmuch as a concentration which lowers
the freezing point from 0.05 to o. i° can be in-
Fig. 38.
vestigated, per cent, solution, corresponding to one centigram
of the dissolved substance, is sufficient for carrying out a molecular
weight determination. 86
DEPRESSION OF THE FREEZING POINT OF SOLUTIONS.
This method is employed for all accurate determinations. A
thick-walled open beaker of 120 to 150 c.c. capacity is placed in
the vessel containing the freezing mixture.’
2. METHOD OF RAOULT.
The (Beckmann) thermometer is so placed in the middle of the
glass vessel that no ice freezes on the lower end of the mercury
reservoir situated near the bottom of the vessel. The stirrer con-
sists of platinum foil and heavy platinum wire soldered together.
The quantity of liquid employed should always be the same,
from 100 to 120 c.c. The solutions are previously prepared by
weighing—with the greatest possible exclusion of air in the case of
acetic acid. Each solution should be used only for one observa-
tion ; the freezing point of the pure solvent is determined before
and after each series of experiments.
The temperature of the freezing mixture should always be kept
constant to within i°; this temperature should be from 3 to 40
below the freezing point of the liquid. The temperature of the
room should be, at most, not more than 50 above the freezing point
of the solvent. Especially does the temperature of the room in-
fluence the result if, as with water, the ice separates as a solid
cylinder on the glass. The error in such cases, for rather high
temperatures of the room, may amount to 0.02°.
The over-cooling should be as uniform as possible—about 0.05
to o.i°; only for water and its dilute solutions, in order to obtain
loose and finely divided ice, should this value amount to 0.50.
The freezing is induced by the introduction of an ice crystal at a
temperature very near the freezing point, or about o.i° above.
The temperature is read off by means of a microscope accu-
rately to 0.002°.
The more concentrated the solution, the more rapidly the ther-
mometer thread sinks, on account of the change of concentration
due to the separation of ice. A small error is also introduced with
concentrated solutions for the highest position of the mercury
thread. The value of the necessary correction may be determined
by observing, from minute to minute, the sinking of the mercury
thread for solutions of different concentrations, for a period of ten
to twenty minutes, and then calculating the time consumed from METHOD OF RAOULT.
87
the beginning of the Reparation of ice to the reading of the highest
position of the mercury thread. This correction is sufficient,
inasmuch as it is usually very small (at most o.ox to 0.02°), and
really not so large as would be expected from the quantity of ice
separated out.
The liquid, during the separation of the ice and previously,
must be well stirred. If a large number of determinations are to
be made, the use of Raabe’s turbine (p. 65) is recommended.
The stirrer is moved in a vertical direction.
If aqueous solutions are to be investigated in midsummer when
the temperature of the room is considerably above o°, sufficient
quantities of loose ice are formed in the liquid in that the mercury
reservoir of the thermometer is loosely surrounded by a platinum
or silver net, and the thermometer fastened to a turbine (with the
necessary care) is set in rapid motion.
By exercising considerable care, the depression of the freezing
point may be determined, by this method, accurately to from
to yyVo of a degree; the further complications of the method
(Raoult, Compt. rend. 114, p. 218, 1892, and Zeit. phys. Chem.
9, p. 343, 1892, as well as Loomis, Ber. d. d. chem. Ges. 26, p.
797, 1893) may be omitted.
According to Jones (Zeit. phys. Chem. n, pp. no and 531,
1893, as well as Ber. d. d. chem. Ges. 26, p. 547, 1893) it is
advantageous, for a high degree of accuracy, to experiment with at
least one liter of solution ; also to make use of a thermometer
graduated to degree.*
Choice of Concentration and Solvent for Freezing
Point Determinations.—The determinations in general, espe-
cially molecular weight determinations, should not be limited to a
single concentration. After investigating various concentrations
and noting the calculated molecular weight as well as the concen-
trations in a system of coordinates, certain reference points regard-
ing the molecular weight of the dissolved substance are obtained :
especially if the investigations are to be extended to dilute solu-
tions. By the method of Beckmann, using always the same
* [See also the investigations of Loomis, Wied. Ann. 51, p. 500, 1894; 57, p.
495, 1896; 60, 523, 1897, and Ber. d. d. chem. Ges. 26, p. 794.—Tr. ] 88
DEPRESSION OF THE FREEZING POINT OF SOLUTIONS.
quantity of solvent, the concentration of the solution to be inves-
tigated is successively increased by the addition of small quantities
of substances through the side tube (Fig. 36) into the thawed
solution.
Care should also be exercised in choosing the solvent, especially
for molecular weight determinations. In doubtful cases the inves-
tigation should be made with several solvents.
Water may be used, so far as the conditions of solubility admit,
excellent as solvent for organic compounds of an indifferent nature
(not conductors). Considerable care is necessary for acids, bases,
and salts; also for certain organic compounds (especially for high
dilutions) the molecular weight found is too large.
Acetic acid has perhaps the most general application. The con-
stants are here much less dependent upon the concentration than
with other solvents ; the calculated values for the molecular weights
are usually normal.
The following solvents may be used with similar results ; formic
acid, lauric acid, stearic acid, thymol, phenol, etc.
The acid character of these solvents, however, must always be
taken into account.
Benzene, which can be used only in the purest condition, is well
adapted on account of the relatively large depression which is pro-
duced, even by dissolving a minimum quantity of substance.
However, substances dissolved in this solvent have a special
tendency to form more complex molecules, which are broken up
only at high dilutions; even then, values calculated for the molecu-
lar weight are sometimes too large.
This is especially true for compounds containing the hydroxyl
group, particularly hydroxyl compounds of acid nature.
Similar to benzene may be mentioned the solvents nitro-benzene,
ethylene-dibromide, and naphthalene ; the high melting point and
strong dissociative properties of the last-named compound must be
taken into consideration.
In regard to the influence of concentration and solvent on the freezing point
and molecular weight, see, among others, Arrhenius, Zeit. phys. Chem. 2, p.
491, 1888; Beckmann, ibid. 2, p. 715; Fabinyi, 3, p. 39, 1889; Magnanini,
ibid. 3, p. 347, 1889; Eykman, ibid. 4, p. 487, 1889; Paterno, ibid. 5, p. 94,
1890, abstract. CALCULATION OF MOLECULAR WEIGHTS.
89
On the use of Beckmann’s apparatus for solvents which do not
solidify, see Nernst5, Zeit. phys. Chem. 6, p. 573, 1890; also F.
Bauke, The Raoult Freezing Method and its Use for Chemical
Investigations, Berlin, 1890. For substances suited for these in-
vestigations, see references already cited.
CALCULATION OF MOLECULAR WEIGHTS.
The calculation of the molecular weight from the depression of
the freezing point is based upon the empirical facts established by
Raoult and the thermodynamical considerations of van ’t Hoff,*
according to which one molecule of any substance dissolved in a
definite quantity of a solvent lowers the freezing point of the
solvent by a constant quantity.
According to Raoult, the characteristic constant for each solvent
may be calculated from the equation :
ME _>
M is the molecular weight of the dissolved substance, E the
depression of the freezing point, P the number of grams of sub-
stance contained in 100 gm. of solvent, and C is the characteristic
constant (the molecular depression).
According to van ’t Hoff, we have ;
ME 0.02 T2
= W ’’
M and E have the same values as above, p represents the num-
ber of grams of dissolved substance contained in 100 gm. of
solution (not solvent), T is the absolute melting point of the
solvent, and W the heat of fusion of the solvent.
O 02
The constants C and are found to be very nearly equal.
* van ’t Hoff, Zeit. phys. Chem. 1, p. 497, 1887. BOILING POINT AND VAPOR PRESSURE.
O 02 'T
The mean values calculated for C and ——- are as follows :
w
Solvent
C
0.02 T2
Tv
Water,
. . - 18.5
18.9
Acetic Acid,
. . - 38-6
38.8
Benzene,
. . — 5°-°
53-o
Phenol,
76.0
Naphthalene,
. . ■— 69.0
69.4
Formic Acid,
. . — 27.7
28.4
Nitro-benzene,
. . — 70.7
69-5
Ethylene-bromide, . . .
. , — xiS.o
117.0*
The calculation of the molecular weight is usually made by
o 02 T
substituting the values of the constant in the formula of
van ’t Hoff.
On the relation of the freezing point to the electric conductivity,
and the calculation of the van ’t Hoff coefficient i from the freezing
point, see, among others, Zeit. phys. Chem. 1, pp. 497 and 633,
1887, and 2, p. 491, 1888. Application of the freezing and
boiling method, see page 108 of this work.
X. THE BOILING POINT AND VAPOR
PRESSURE.
General.—The normal boiling point is the temperature of the
vapor which rises from the liquid boiling under a pressure of
760 mm. of mercury.
In the broader sense, the boiling point is the temperature at
which the vapor pressure of the liquid is great enough to overcome
the external pressure.
The boiling point, therefore, is a function of the external pres
sure.
* Constants for other solvents see, among others, Eykman, Zeit. phys. Chem.
4, p. 515, 1889, and Raoult, Compt. rend. 95, pp. 188 and XO3O, 1882. ORDINARY METHOD FOR DETERMINING BOILING POINTS.
91
Distinction between the static and dynamic methods is made
according as the pressure of a vapor above its liquid is measured at
different temperatures, or the boiling temperature determined
which corresponds to a definite pressure.
In general, the determination of the normal boiling point is
sufficient.
i. ORDINARY METHOD FOR THE DETERMIN-
ATION OF BOILING POINTS.
The three forms of apparatus (Figs. 39-41) are especially appli
cable for boiling-point determinations.
Fig. 39.
Fig. 40.
Fig. 41.
Figure 39 represents the arrangement of Berthelot.* An outer
wide tube surrounds the neck of the flask in which the thermometer
is placed. The flask is connected with a simple condenser.
* Berthelot, Mec. chim., Bd. I, p. 288, 1879. 92
BOILING POINT AND VAPOR PRESSURE.
The apparatus figure 40 (O. Schumann *) has
the advantage of being made entirely of glass.
The flask figure 41 (L. Meyer) is provided
with a return condenser at a and a stopper and
thermometer at b. The narrow side tube has an
arrangement to prevent the liquid which flows back
in the cooler from coming in contact with the ther-
mometer.
The thermometer, which has been carefully tested,
(see under 3, chap, xx), is, whenever possible, intro-
duced into the vapor chamber so far that the correc-
tion for the projecting thread of mercury may be
neglected.
The bumping of liquids should be prevented.
This may be done by throwing in small pieces of
platinum or some porous clay or soap-stone; also
by means of a capillary tube in the stopper, through
which a slow current of gas is conducted into the
boiling liquid. Also by the arrangement on page
98.
The barometric pressure (4, chap, xx) must always
be observed simultaneously with the determination
of the boiling point.
If the barometric pressure is b mm. of mercury,
the boiling point at 760 mm. is obtained very
closely by adding 0.0375 (760—b) degrees to the
observed temperature.
If the boiling point is to be determined accu-
rately to the of a degree, the method should
be carried out as described on page 97 and follow-
ing; and the Beckmann apparatus (p. 104) should
be employed. See also the simple apparatus of
Glazebrook and Shaw, Physik. Prakt, p. 183,
1888.
Fig. 42.
* Schumann, Ber. d. d. chem. Ges. 18, p. 2086, 1885. METHODS OF SIWOLOBOFF AND JONES-SCHLEIERMACH ER.
93
2. DETERMINATION OF THE BOILING POINTS
OF LIQUIDS IN SMALL QUANTITIES.
(a) Method of Siwoloboff.*
The glass tube A is fastened to a thermometer as shown in figure
42, and in it is placed one or two drops of the liquid whose boil-
ing point is to be determined.
In A is a capillary tube which may be prepared by drawing out
a wider tube. The drawn-out portion is
fused together in the middle and then (see
figure) broken off above the place melted
together.
If the apparatus is placed in an outer tem-
perature-bath (glycerin, water, sulphuric
acid), small bubbles are produced in the
capillary tube before the boiling begins ;
these bubbles are quickly increased to a
uniform chain of small vapor bubbles. The
corresponding temperature is taken as the
boiling point. Errors of 0.5 to i° are
liable to occur with this method.
Method of Jones-Schleiermacher.|
By this—static—method, the temperature
is determined at which the vapor pressure of
the substance is equal to the atmospheric
pressure. This temperature is the boiling
point of the substance for the given pressure.
Fig. 43. Fig. 44.
A U-shaped barometer tube is formed from a clean, dry, glass
tube of about 50 cm. in length and 6—B mm. in width, as shown
in figure 44, so that the shorter limb ends in a hair-like capillary
opening as in figure 43.
About one decigram of the liquid or solid substance is introduced
* Siwoloboff, Ber. d. d. chem. Ges. 19, p. 795, 1886.
f Schleiermacher, Ber. d. d. chem. Ges. 24, p. 944, 1891, and Jones, ibid. p.
2251. 94
BOILING POINT AND VAPOR PRESSURE.
into the dry tube through the opening of the longer limb. By
inclining the tube (after heating a solid substance until liquefied)
the substance can be conducted over into the shorter limb. Dry
mercury is then allowed to flow in slowly until it stands, in both
limbs, about 2 cm. below the closed end ; in this way the liquid
or liquefied substance is collected above the mercury in the short
limb. A portion of the substance which may remain in the longer
limb will have no influence on the result. The liquid is then
heated to faint boiling until the air clinging to the walls of the
tube or absorbed by the liquid is completely removed through the
capillary opening. Mercury is then carefully introduced until the
liquid fills the shorter limb up to the wider portion of the capillary.
The fine capillary tube is then melted off by means of a small
pointed flame. Only a small gas-bubble remains then in the point of
the capillary tube, the influence of which on the accuracy of the
result may be neglected.
The mercury in the open limb is then removed down to the
upper end of the bend in the tube, by simply inclining the U-tube
downward to a horizontal position. If the tube is narrowed some-
what at the bend, the entrance of air-bubbles into the closed limb
is prevented.
The apparatus with a thermometer is then fastened in the (not
too narrow) pear-shaped vessel of V. Meyer. The thermometer is
placed as shown in figure 44. The liquid bath may be water, sul-
phuric acid, paraffin, etc.
The apparatus is slowly heated, and the use of a stirrer is advan-
tageous.
The temperature at which the mercury assumes the same height
in the two limbs is the boiling point for the atmospheric pressure.
If the thermometer is reliable, and the mean of several observa-
tions is taken (also by cooling the hot liquid to the boiling temper-
ature), an accuracy of from 0.2-0.3° maY be attained by this-
method. DETERMINATION OF THE BOILING POINT.
95
3. DETERMINATION OF THE BOILING POINT
AT DIFFERENT PRESSURES.
In order to establish the relation between the vapor pressure and
the boiling temperature, the dynamic method is preferable.
A boiling-vessel, as represented in figure 40 or figure 41, is con-
nected with an air-tight pressure regulator.
A simple form of apparatus* is represented in figure 45.
Fig. 45.
The Beckmann boiling apparatus described on page 98 (which can
be made air-tight by closing the boiling apparatus) is connected
through the cooler K with the air-chamber W and the manometer
O. At Tis a branch tube with a pinch-cock Q, which connects
the apparatus with an air-pump or gas generator, so that the pres-
sure in the apparatus can be increased or decreased at pleasure.
The manometer is filled with pure, clear sweet oil, the specific
gravity of which (for different temperatures) has been determined.
The air-chamber W, which is interposed for the adjustment of
♦ Roloff, Zeit. phys. Chem. ir, p. 25, 1893. 96
BOILING POINT AND VAPOR PRESSURE.
small pressure-fluctuations in the apparatus, has a capacity of at
least 12 1. If the manometer still shows irregular variations, a
capillary tube 10-20 cm. long is inserted.
The closing of the apparatus absolutely air-tight from the outer
air is accomplished (1) by surrounding the stoppers of the manom-
eter and boiling apparatus L M R with rubber capsules fastened
by means of wire; (2) by connecting the glass parts with thick-
walled rubber tubing; and (3) by placing a layer of mercury q at
the top of the cork in the air chamber.*
The regulator is protected from the heat by placing a screen
between it and the boiling apparatus.
A cathetometer (2, chap, xx) is used in reading the manometer
and thermometer; fluctuations in frequent readings of barometric
pressure are to be taken into account. In order to eliminate the
influence of the possible barometric variations, it is better to deter-
mine the boiling point at normal pressure before and after each
series of observations.
Before making the experiment, the apparatus should be tested
for its air-tightness by varying the internal pressure. Liquid for
investigation, water, see Landolt-Bornstein’s Tabellen, p. 47,
1883 ; also Schmidt, Zeit. phys. Chem. 7, p. 433, and 8, p. 628,
1891 ; ibid. 7, p. 441, boiling apparatus with pressure regulator.
Other pressure regulators, see L. Meyer, Lieb. Ann. 165, p. 303 ;
Stadel and Hahn, Lieb. Ann. 195, p. 218, and Ber. d. d. chem.
Ges. 13, p. 839, 1880; O. Schumann, Wied. Ann. 12, p. 44, and
Ber. d. d. chem. Ges. 18, p. 2086, 1885; Brown, Phil. Mag. (5)
7, p. 411, Perkin, Jour. Chem. Soc., p. 689, 1888, and Obach,
Zeit. f. angew. Elektr. von Carl, p. 69, 1880.
Apparatus for the static method, see Schmidt, Zeit. phys. Chem.
8, p. 629, 1891 ; Kahlbaum, Ber. d. d. chem. Ges. 19, p. 2954,
1886; Bremer, Rec. Pays-Bas 6, p. 121, 1887; Emden, Wied.
Ann. 31, p. 145, 1887 ; Tammann, Akad. St. Petersburg, Mem.
35, Nr. 9, 1887 ; Ref. Zeit. phys. Chem. 2, p. 42, 1888 ; Raoult,
Zeit. phys. Chem. 2, p. 354, 1888 ; Beckmann, ibid. 4, p. 532,
1889.
The relation of pressure and temperature is represented graphi-
* The apparatus may also be made air-tight by means of rubber stoppers. ELEVATION OF THE BOILING POINTS OF SOLUTIONS.
97
cally, or expressed by interpolation formulae of the form, log E
a -(- b d and log. E= a b d -f- cft (Ostwald, Lehrb. Allgem.
Chem., 2. Aufl., Bd. i, p. 313, 1891, and Schmidt, Zeit. phys.
Chem. 7, p. 444, 1891).
Relation of the boiling point to the constitution of organic com-
pounds, see Marckwald, Verlag von Friedlander & Sohn, Berlin,
1887.
Tables of vapor pressures of solutions, see, among others, Tam-
mann, Ref. Zeit. phys. Chem. 2, p. 42, 1888.
Critical temperature and pressure. Method of determination.
Pawlewski, Ber. d. d. chem. Ges. 15, p. 2460, 1882, and
Schmidt, Lieb. Ann. 272, p. 273, 1891.
Galitzine, Wied. Ann. 41, p. 614; Cailletet and Colardeau,
Compt. Rend. 112, pp. 563 and 1170, 1891 ; Altschul, Zeit. phys.
Chem. 11, p. 577, 1893, and Battelli, Ann. chim. phys. 29 (6),
p. 400, 1893; Tables of critical data, Heilborn, Zeit. phys. Chem.
7, p. 602, 1891 ; ibid, complete literature.
XI. ELEVATION OF THE BOILING POINTS
OF SOLUTIONS.
Principle.—The boiling points of the solvent and the solution
are determined in a suitable apparatus, and, from the elevation of
the boiling point thus found, the molecular weight of the dissolved
substance is calculated according to the formula on page 107.
This method finds special use when the boiling point of the
solvent is less than ioo° (at the highest 130°).
i. METHOD I OF BECKMANN.*
Apparatus,—The boiling-vessel consists of a three-tubed glass
flask A, as shown in figure 46.
* Beckmann, Zeit. phys. Chem. 4, p. 533, 1889, and 6, p. 437, 1890. 98
ELEVATION OF THE BOILING POINTS OF SOLUTIONS.
In the one tube is fastened a Beckmann thermometer, graduated
to To or tot a degree, by means of a tightly fitting cork. In
the middle tube b is introduced the reflux tube from the condenser
Fig. 46.
B, which can be employed, for most liquids, in the form given by
Soxhlet; the opening at the top of this metallic cooler is provided
with a calcium chloride tube, which is filled with not too finely METHOD I OF BECKMANN.
99
divided granules of perfectly anhydrous calcium chloride. The
lower part of the' tube from the reflux condenser is provided at d
with a vapor-hole, which is situated in the vapor chamber, and
through which the evolved vapor rises to the condenser. The tube
C, which is closed with a cork during the investigation, serves for
the introduction of the substance into the boiling solvent.
In order to protect the apparatus from side-heating, it is placed
in an asbestos jacket m, which can be protected at the top from
the heat influence of the surrounding air by covering over with
clay. This jacket, with the boiling-apparatus, for further protec-
tion against the flame, rests on two asbestos plates; in the middle
of the upper one is a hole, the diameter of which is equal to that
of the asbestos jacket.
To prevent the liquid from bumping, a short piece of thick plat-
inum wire j is fused into the bottom of the boiling-vessel;
whereupon the boiling takes place uniformly with the formation of
small bubbles of vapor only at the surface of this wire, owing to
its greater conductivity of heat.
The boiling-vessel is filled to the middle with glass-wool or glass
pearls 3 to 4 mm. in diameter. Through the introduction of
these, previously cleaned with con. hydrochloric acid, the temper-
ature is regulated uniformly in the interior of the liquid, and over-
heating is avoided. The subsequent cleaning of the pearls, in case
the substance has adhered closely, is best accomplished in Soxhlet’s
extraction apparatus.
The substance to be dissolved is introduced, during the boiling,
through the opening in the tube C, which is opened and closed as
quickly as possible; whereby the evaporation, even for highly
volatile solvents (as ether), is scarcely perceptible on account of
the length of the tube.
Substances which are easily liquefied are blown into the solvent
by means of a pipette of the form represented in figure 47.
The pipette is suitably graduated in cubic centimeters, and, when
necessary, is provided with a calcium chloride tube. The pipette
is introduced into the tube C. Before reweighing, the liquid is
sucked back out of the capillary tube.
Viscous liquids may be introduced into the apparatus by means-
of the valve-tube represented in figure 48. ELEVATION OF THE BOILING POINTS OF SOLUTIONS.
This tube, filled with the substance, is weighed and allowed to
slide through the tube C into the solvent. At the bottom of the
boiling-vessel the valve at the lower end of the tube opens and
allows the liquids to mix.
As far as possible, the introduction of glass into the boiling-
vessel is to be avoided, inasmuch as any change in the level of the
liquid in the boiling-vessel influences the vapor pressure and the
boiling point of the liquid.
The raising of the level i mm. corresponds to 0.002° in
the elevation of the boiling point. The introduction of several
tubes, as well as larger quantities of dissolved substance, will pro-
duce a small error by decreasing the volume of the vapor-chamber.
Fig. 47.
Fig. 48.
It is undesirable, therefore, to introduce solid substances in a
vessel. Powdered substances are made into pastilles, the size of
which depend upon the solubility of the substance (Pharm. Cen-
tralhalle 30, p. 132, 1889).
Method of Operation.—The boiling-vessel, together with its
pearls, is tared on a balance which weighs accurately to i cgm.;
it is then filled with the pure solvent to the height indicated in
the figure, and the quantity of the same determined by weighing.
Inasmuch as, for not too violent boiling, the temperature of the
vapor and the pure solvent are the same in this arrangement, the
thermometer is so inserted that the mercury reservoir is completely
covered with the liquid without coming in contact with the pearls.
The lower part of the tube from the reflux condenser is bent to METHOD I OF BECKMANN.
one side, and is fastened in the boiling-vessel so that the lower
portion is removed as far as possible from the thermometer, thereby
preventing any direct influence, of the somewhat cooler liquid
flowing back, on the reading of the thermometer. The lower end
of each tube immersed in the liquid stands about i cm. from
the pearls; hence the back-flow is not hindered through the evolu-
tion of vapor-bubbles.
The prepared boiling-vessel, after being wrapped with asbestos,
is heated by means of a Bunsen burner. For ethereal solutions
the point of a luminous flame is used; for alcohol, etc., the non-
luminous flame of the burner is employed. If the asbestos pack-
ing is properly adjusted, the difference in the highest reading of the
thermometer for ether heated with the small point of the flame
and the full Bunsen flame amounts to, at most, i° C. In
general, it is important in the investigation of a solvent and
its corresponding solution that the size of the flames should be as
nearly as possible the same in the two cases. The use of a regu-
lator-cock or the membrane gas pressure regulator of Elster * is
advantageous, if not indispensable. Investigations in the evening
should be avoided, on account of the irregular gas pressure at that
time.
The boiling should be so regulated that for ether and carbon-
disulphide, one drop every two to five seconds, for alcohol, benzene,
or acetic acid, one drop every five to ten seconds, falls from the con-
denser at B.
The boiling is then made somewhat more vigorous by means of
a larger flame ; if, however, the boiling point has been reached or
passed, the liquid is cooled to one-tenth of a degree below the
boiling point and again heated, so that there is always a moderate
boiling. After a time, the mercury assumes a constant position,
which can be taken as the boiling point (of the solvent) only
when it remains constant to 0.002° for at least five to ten minutes.
The thermometer should always be gently tapped before reading off
the temperature, as this frequently produces a slight change in the
position of the mercury. The boiling point should always be
determined by allowing the mercury thread in the thermometer to
* Beckmann, Zeit. phys. Chem. 4, p. 546, 1889. 102
ELEVATION OF THE BOILING POINTS OF SOLUTIONS.
rise, as the definite positions of the mercury attained through the
rising and falling of the thread show small variations.
After reading off the boiling point, without removing the flame,
a weighed quantity of substance is introduced through C into the
boiling-vessel by means of the arrangements described on page 100.
The thermometer sinks immediately, and after the complete solution
of the substance the temperature again becomes constant, which
is taken as the boiling point of the solution. A known quantity of
substance is again added, as the investigations here should not, in
general, be limited to a single concentration. The investigations
of the same substance should succeed each other without loss of
time. At the end of the experiments the quantity of solvent which
has been vaporized during the investigations should be determined
by repeated weighings of the apparatus.
The accuracy of the results is influenced by the barometric pres-
sure and the temperature of the room.
A difference of i mm. in the barometric pressure corresponds,
on an average, to a difference of 0.03° in the boiling point.
If the use of the pressure regulator (p. 95) is omitted, care
should be taken that no essential variations occur in the barometric
pressure while the experiment is being carried out. For unsettled
weather a second apparatus, with the pure boiling solvent, can be
set up during the experiment. From the readings of the thermom-
eter in the latter apparatus, the necessary corrections for the change
of barometric pressure may be easily calculated.
Sometimes it is recommended to work under reduced pressure to
prevent decomposition, or under increased pressure to increase the
solubility. In this case use may be advantageously made of the
simple pressure regulator described on page 95. For this purpose
the apparatus of Beckmann (Zeit. phys. Chem. 6, pp. 463 and
464, 1890) should be used.
The influence produced by the temperature of the room is
greater, the higher the boiling point of the liquid. Changes in
the temperature of the room during an experiment should be
avoided.
In order to insure a perfect adjustment of the temperature it is
necessary, for boiling-point determinations of pure solvents, to
first maintain the boiling from one to two hours before the ther- METHOD II OF BECKMANN.
mometer is read. The second method of Beckmann, described
below, is uninfluenced by the temperature of the room, and there-
fore specially adapted to solvents of higher boiling points.
Finally, it should be noticed that the recent Beckmann ther-
mometer, graduated to of a degree, and that of F. O. R.
Gotze, in Leipzig, adapted equally well to freezing points and
boiling points, experience a slight change in the value of the
degree, owing to the separation of large quantities of mercury.
The degrees are smaller for high temperatures, thereby diminishing
the elevation of the boiling point and increasing the molecular
weight. The error at most for benzene amounts to 1.3 per cent.*
2. METHOD II OF BECKMANN.f
Apparatus and Method of Operation (Fig. 49).—The
boiling-vessel A consists of a rather long tube about 2.5 cm.
in width, in the side tube of which is fastened a coiled con-
densing tube Kv and through the upper stopper of which is intro-
duced a Beckmann thermometer.
A platinum wire is fused in the bottom of the tube A, which
is then filled with glass pearls to a height of 3 to 4 cm.
This boiling-vessel, as shown in the figure, is placed in a vapor
jacket B, which is made of glass or, for high boiling points, of
copper. The jacket is provided with a side tube in which the
reflux condenser is fastened.
The boiling-vessel A is fastened in the vapor jacket by means of
a cylinder of asbestos a, while the space above, between the tube
and the jacket, is filled with asbestos wool.
The boiling-tube and the vapor jacket contain the same solvent.
The results are thereby made independent of the temperature of
the outer room. A small piece of clay may be introduced into the
vapor jacket to lessen the boiling.
The vapor jacket with the boiling-tube rests on a small box C
* Beckmann, Zeit. phys. Chem. 6, p. 443, 1890.
f Beckmann, Zeit. phys. Chem. 8, p. 223, 1891. The Beckmann apparatus
is furnished by the firm of F. O. R. Gotze, in Leipzig. 104
ELEVATION OF THE BOILING POINTS OF SOLUTIONS.
composed of asbestos board and water glass. A vertical section is
represented in the figure.
Where the flames fall upon the hot surface is a sickle-shaped
opening, covered with wire gauze and asbestos board; the opening
is arched over with the edge d of an asbestos covering.
The boiling-vessel is pro-
tected from the direct action
of the flame, from the Bunsen
burners placed to the sides,
by means of the asbestos rings
hx and hr A small flame un-
der the boiling-vessel is neces-
sary only for water (on ac-
count of its high specific heat
and heat of vaporization).
For all other liquids the boil-
ing of the outer liquid is suf-
ficient to maintain the boiling
of the inner liquid.*
The arrangements j and s
serve as outlets for the flame
gases.
If the apparatus is to be
used for solvents of low boil-
ing points (under 6o°), small
Liebig condensers may be
substituted for Kx and K\;
for hygroscopic solvents a
small calcium chloride tube
is attached to the condenser.
The solvent in the inner
tube is either weighed in the
tube or measured by means of a pipette ; the substance (p. 100) is
Fig. 49.
V V
* Parizek and Sule hasten the operation by elevating the temperature of the
vapor chamber a few tenths of a degree above the boiling point of the inner
liquid, through the addition of a few drops of a substance of higher boiling
point. APPLICATION OF METHODS I AND 11.
introduced by means of a pipette or in the form of pastilles.
Twenty gm. bf solvent is sufficient for the vapor chamber.
A small correction should be applied, owing to the evaporation
and condensation in the cooler. According to Beckmann, the quan-
tity of liquid suspended in the vapor chamber amounts to, for very
mobile liquids, from 0.15 to 0.2 gm.; for water about 0.35 gm.
For further details of the method see the manipulations given for
method 1.
APPLICATION OF METHODS I AND ll.*
Method i is applicable for solvents with boiling points up to
about 130°. In general, the method is preferable for solvents
with low boiling points. For solvents with high boiling points
(anilin, phenol, etc.) method 11 is preferable; this method is also
preferable for water.
Besides its independence of the temperature of the room,
method 11 has come into special prominence on account of,—
1. The small quantity of the solvent and substance required for
the experiment;
2. The more rapid attainment of a constant boiling temperature
(thirty to sixty minutes) ;
3. The more convenient method for heating. A gas pressure
regulator is unnecessary.
In reason 1, however, there is also a slight disadvantage, inas-
much as the accuracy is always influenced by the quantity of
solvent.
Choice of Concentration and Solvent (for the boiling-point
method).—The investigation is begun with a concentration which
produces an elevation of about o. lor 0.20 in the boiling point, and
the content of the solution is gradually increased to ten or twenty
per cent. The relations between the percentage content and the
calculated molecular weights are represented graphically, and then,
in most cases, definite conclusions are drawn regarding the magni-
tude of the molecular weight.
* [A more recent form of apparatus has been described by Orndorff and Cam-
eron, Amer. Chem. Jour. 17, p. 507, 1895.—Tr.] ELEVATION OF THE BOILING POINTS OF SOLUTIONS.
The choice of the solvent should always he carefully considered,
the choice depending largely on the solubility of the substance and
also its boiling point ; in general, only such substances are investi-
gated* whose boiling point is at least 130 to 1400 above that of the
solvent.
If, for the use of a definite solvent, there is any uncertainty in
regard to the dissociation of the complex molecules, the substance
should be investigated with several solvents.
Substances, especially hydroxyl compounds, dissolved in benzene,
chloroform, and carbon disulphide, have a tendency to form com-
plex molecules, which decompose more and more with increasing
dilution.
The molecular weights obtained with such solvents as acetic acid,
formic acid, thymol, phenol, ether, alcohol, ethyl-acetate, and
acetone at higher concentrations are more normal.
In general, ethyl-ether is best adapted to this work. Its low
price, its high dissolving capacity, its chemical indifference, and
the ease with which the dissolved substance can be obtained again,
give it preference over other solvents; also, the volatility and dis-
sociative power are very advantageous for the convenience and
accuracy of the determination ; in like manner, the large molecu-
lar elevation is of special importance. Water is less suitable for
the purpose. The number obtained for electrolytes should be care-
fully tested ; the low solubility of non-electrolytes is objectionable.
The high boiling point and the small molecular elevation are also
a disadvantage.
On the influence of concentration and solvent, see the work of
Beckmann, Zeit. phys. Chem. 4, p. 532, 1889; 5, p. 76, 1890;
6, p. 437, 1890; 8, p. 223, 1891.
* Nernst, Zeit. phys. Chem. 8, p. 128, 1891; also 11, p. 1, 1893. Nernst
shows that the boiling apparatus may be used for determining molecular weights
of very volatile substances. CALCULATION OF MOLECULAR WEIGH TS.
CALCULATION OF MOLECULAR WEIGHTS.
According to van ’t Hoff,* the following formula holds good :
M{rx-TJ) = 00277,
/ w
M represents the molecular weight of the dissolved substance ;
p the number of grams of dissolved substances in 100 gm. of solvent;
Tx and T0 are the absolute boiling points of the solution and sol-
vent = the observed 273.20. Tx T0 is therefore the elevation
of the boiling point ; Wis the heat of vaporization of the solvent.
o 02 T
The constant —(the molecular elevation of the boiling
point) may be determined from the known molecular weight of the
dissolved substance, or calculated from the heat of vaporization
and the boiling point of the solvent.
The following table (according to Beckmann) f contains the
values of this constant for a number of solvents ;
o mux Boiling Molkcular Elkvation
solvk t. Point. of the Boiling Point.
Ethyl-ether, ....
. • 34-97
21.1
Carbon disulphide,
. . 46.2
23-7
Acetone,
• • 56.3
16.7
Chloroform, ....
. . 61.2
36.6
Ethyl-acetate, . . .
- - 74-6
26.1
Ethyl-alcohol, . . .
• - 78.3
ir-5
Benzene,
. ■ 80.3
26.7
Water,
. . 100.
5-2
Acetic acid, ....
. . x 18.1
25-3
Ethylene-bromide, . .
. . 131.6
63.2
Phenol,
. . 182.3
30.4
Anilin,
. . 183.7
32.2 +
If a solvent is to be used, the constant of which is unknown,
the same may be determined by dissolving in the solvent a sub-
* Beckmann, Zeit. phys. Chem. 4, p. 533, 1889.
V V
f According to Parizek and Sule (Ber. d. d. chem. Ges. 26, p. 1410, 1893)
this constant for methyl-alcohol = 9.20, and for iso-propyl-alcohol = 12.9.
J In regard to the change of these constants with the bo ling point of the sol-
vent for diminished pressure, see Beckmann, Zeit. phys. Chem. 6, p. 463, 1889. ELEVATION OF THE BOILING POINTS OF SOLUTIONS.
stance of known molecular weight (ligroin, petroleum, ether,
aqueous alcohol, etc.).
APPLICATION OF THE BOILING-POINT AND
FREEZING-POINT METHODS.
In general, the chemical nature of the substance to be investi-
gated, especially its solubility and volatility, determines which of
the two methods is preferable.
The freezing-point method, it is true, is no more convenient to
operate than the boiling-point method; but it requires less time,
and is also (not considering the investigation of concentrated solu-
tions) capable of greater accuracy. The constants of the molecu-
lar depression of the freezing point are greater than the correspond-
ing constants of the molecular elevation of the boiling point. The
freezing-point method is preferable for substances which have a
tendency to decompose at high temperatures, although the boiling
point can be lowered by the use of a pressure-regulator.
The freezing-point method is independent of the barometric
pressure, and may be used for the investigation of volatile sub-
stances, while the simple boiling-point method has hitherto been
limited to substances whose boiling points were at least 130° above
that of the solvent (p. 106).
On the other hand, the boiling-point method admits of a larger
number of excellent solvents, as ether, alcohol, carbon disulphide,
etc. An important advantage is the greater solubility of sub-
stances at higher temperatures, and the greater tendency toward
the decomposition of the complex molecular groups. For the
investigation of concentrated solutions the temperature-reading is
more accurate, for no essential change of concentration occurs, as
in the freezing method. SPECIFIC HEAT.
109
XII. SPECIFIC HEAT.
General.—The unit of heat is the calorie.
The calorie is that quantity of heat required to raise the temper-
ature of 1 gm. of water from o to i° (gram-calorie).
If 1 gm. of water is heated to i° above the temperature of the
room, the quantity of heat required is not equal to 1 calorie, but
probably somewhat less (a fraction of a per cent.).
Inasmuch as the specific heat of water depends upon the tempera-
ture, and as experiments on heat capacity are frequently made at
the temperature of the room t° (usually 180), the calorie at t°
(180) is selected as the unit, so far as the method of mixtures
(p. no) is concerned. It is the quantity of heat required to
raise the temperature of 1 gm. of water at t° (180) i°.
For the method of melting ice (p. 121) the mean calorie—i. e., the
hundredth part of the heat required to raise the temperature of
water at o° to ioo°—is usually taken as the unit.
The mean calorie and the calorie at 180 differ, at most, not
more than one per cent. The exact relation, at present, is not
known with sufficient certainty.
In regard to the large calories for thermo-chemical measure-
ments, see page 132.
The specific heat of a body is the quantity of heat, measured in
calories, required to raise the temperature of the unit-mass = 1 gm.
of the substance i°. As the specific heat in general varies some-
what with the temperature, the temperature at which the specific
heat is determined should always be specified.
By the method of mixtures, and also the method of melting ice,
only the mean specific heat is obtained—i. e., the mean value of
the quantity of heat required to raise 1 gm. of the substance i° in
temperature for a given temperature interval t—tx.
If Q is the quantity of heat necessary to raise the temperature
of 1 gm. of substance from tx to t°, then is the average
specific heat for that temperature-interval.
The mean specific heat increases, in most cases, proportionally SPECIFIC HEAT.
with the temperature, and can be represented by the equation
Ct tl = a -f- b (/-f- /j) ; ci and b are constants which can be cal-
culated from two determinations of the mean specific heat for
different temperature-intervals. Then the quantity of heat sup-
plied from o to t° is Qt = atJrbt'1, from which it follows that
—i. e., the true specific heat at t°isKt = a 2b t.
Usually, a determination of the average specific heat is sufficient.
The product of the specific heat and the atomic or molecular
weight is called the atomic or molecular heat.
1. THE METHOD OF MIXTURES.
Principle and Calculation.—A liquid or solid heated to a
definite temperature is intimately mixed with a liquid of known
specific gravity at a lower temperature. Mixtures involving chem-
ical action must always be excluded. Then the quantity of heat
given up by the first body in cooling is placed equal to that taken
up by the liquid in the calorimeter on heating, as the heat given
out by the system through radiation and conduction is inappre-
ciable.
If P represents the weight (in grams) of the liquid or solid
heated to the temperature T, C the unknown specific heat of the
same, p the weight of the liquid in the calorimeter at the lower
temperature t and of unknown specific heat c, and r the final tem-
perature assumed by the mixture, then the quantity of heat given
up by the heated body is P C ( T—r), and the quantity taken up
by the liquid in the calorimeter is pc (r t). Therefore P C
(T—r)=pc (t —/).
Inasmuch as the parts of the calorimeter (vessel, stirrer, ther-
mometer) take up a portion of the heat, a correction must be
applied to the above equation.
The quantity of heat c (r —t) must be multiplied hyp-\-w
instead of p, where w represents the heat capacity of all the parts
of the calorimeter. It is the number of grams of water which
corresponds in thermal value to the parts of the apparatus—i. e.,
the quantity of heat required to raise the temperature of the ap-
paratus i°. If the specific heat of the metallic portion
of the apparatus, the weight of which is k gm., then the product it y METHOD Of' MIXTURES.
is the water-equivalent and zy (r t~) the quantity of heat neces-
sary to raise the temperature from tto r°. The specific heat of the
substance, therefore, is,—
_f/ + w)c (t t) .
P{T-t) ’
or if, as is usually the case, water is employed in the calorimeter,
then
r__(P + w) (r t)
’
since c may be placed approximately equal to unity (p. 109).
(a) Specific Heat of Solids.
Heating Vessel.—A vessel of the form of figure 50 may be
employed. The substance is heated by means of the vapor of
Fig. 50.
Fig. 51.
boiling water (and other liquids) until the temperature of the ther-
mometer is constant. If no thermometer is at hand, the boiling
temperature is calculated from the barometric pressure.*
Very advantageous also is the short-necked retort A (Fig. 51)
composed of copper or glass, in which water, nitrobenzene, di-
phenylamine, etc., may be kept vigorously boiling.
Not too small a quantity of the substance is placed in the small
tube C. The heating of the retort is so adjusted that the vapor of
the liquid condenses, for most part, at D. At a given moment the
* Landolt-Bornstein, Physik. Chem. Tab., pp. 48 and 49, 1883. SPECIFIC HEAT.
substance in the calorimeter is introduced into the retort, so that
none of the heating liquid flows out.
The substance, especially if it is a poor conductor of heat, is
used in small pieces and weighed in the tube. As a portion of the
substance frequently clings to the tube, the tube is reweighed after
the experiment.
Pulverized substances or small granules, as well as substances
which act chemically on the liquid in the
calorimeter, are enclosed in a small metallic
vessel made of platinum gauze, or in a plati-
num shell soldered with gold. The weight
of the platinum, multiplied by the specific
heat = 0.0324, is the water-equivalent of the
small vessel.
The Calorimeter (Fig. 52).—The calo-
rimeter consists of a cylindrical, thin-walled
vessel, made of platinum, silver, or brass.
Glass vessels * are used only for very rough
determinations.
The outer surface of the vessel is polished
to prevent radiation. The length of the
cylinder is somewhat greater than the diam-
eter ; the capacity should be at least 200 c.c.,
and, better, 500 c.c.
To prevent a considerable loss of heat to
surrounding bodies, the calorimeter, resting
on three pieces of cork, is placed in a larger
double-walled brass vessel. The space be-
tween the walls is filled with water, and the
size of the vessels so adjusted that the dis-
tance between the inner and outer vessel is about 5 cm. at all points.
During the investigation the vessel is provided with a cover.
For accurate determinations the inner calorimeter vessel, resting on
pieces of cork, is placed in one or two larger brass vessels, and
these in turn placed in the outer double-walled vessel.
Fig. 52.
* Nernst, Zeit. phys. Chem. 2, p. 24, 1888; Bersch, Zeit. phys. Chem. 8, p.
388, 1891; and Kohlrausch, Prakt. Phys. vil, p. 119, 1892. METHOD OF MIXTURES.
The calorimeter is provided further with a small, suitable stirrer
(platinum, brass, etc.) and a carefully tested thermometer (see under
3, chap. xx).
The stirrer may have the form represented in figure 52. A me-
tallic wire, movable in a vertical direction, is soldered to a metallic
gauze, which is provided with a slit for the thermometer; or a
metal ring is soldered to a metallic wire at an angle of 90°. The
stirrer may also have the form of a screw (Fig. 58, p. 131).
The thermometer, for accurate observations, is graduated to
°r tet of a degree, and is read by means of a microscope accu-
rately to -g-Jj-g- of a degree.
The heating vessel and calorimeter should be separated by means
of a cardboard screen.
Method of Operation.—When the substance has been heated
to the desired temperature, and the temperature of the water in
the calorimeter has been accurately determined, the substance is
allowed to fall into the calorimeter with the necessary precaution,
and, during constant stirring, the maximum temperature ris read off.
The stirring must be carefully done. In using the stirrer repre-
sented in figure 52, care should be taken not to remove any portion
of the substance above the liquid.
If water can not be employed, use may be made of such liquids
as turpentine (sp. H. = 0.43), toluene (sp. H. = 0.40), and ani-
lin (sp. H. = 0.49).
The corrections to be applied are: (x) That for the water-
equivalent of the calorimeter, stirrer, and thermometer; (2) for
the loss of heat by radiation.
The water-equivalent of the metallic portions is obtained by
weighing the calorimeter vessel, together with the stirrer. Only
the portion of the stirrer, however, which is immersed in the liquid
is to be taken into account. Let the combined weights =tt and
the specific heat of the metal =y, then tt y is the water-equivalent
(y for platinum = 0.032, for silver = 0.057, and for brass, with
sufficient accuracy = 0.094). If the combined weights are not
more than 20 gm., the wTater-equivalent Try for platinum is only
0.64, and for brass 1.88 gm.
The water-equivalent of the portion of the thermometer im-
mersed in the liquid is determined most simply by estimating the SPECIFIC HEAT.
volume of the same by sinking into a graduated vessel. Inasmuch
as i c.c. of glass has the same water-equivalent, 2.5 X 0.19 = 0.47,
as 1 c.c. of mercury = 13.6 X 0.034 = 0.46, it is only necessary
to multiply the volume v in cubic centimeters, of the portion of the
thermometer immersed, by 0.46 to obtain the water-equivalent.
The total water-equivalent of the apparatus, then, is w r. y -)-
0.46 v.
The water-equivalent of the thermometer may be determined
somewhat more accurately by heating the same in a flame or in a
mercury bath to 40-50° and then immersing it in the water in a
calorimeter. If mis the weight of the water in grams, /2— tY the
increase of temperature, and tz—12 the decrease in the temperature
of the thermometer, then,—
m (
\k~tJ
is the water-equivalent of the thermometer.
The loss of heat through radiation is easily understood, for it is
evident that, when the calorimeter is heated above the temperature
of the surroundings, a continual loss of heat takes place, which
increases with the difference in the temperatures of the calorimeter
and the surroundings. The final temperature, then, is too small by
an amount J.
The influence of the radiation can be neglected as inappreciable
only when the adjustment of the temperature takes place quickly,
and the maximum temperature is not more than 2-30 above that
of the surroundings. It is also necessary that the capacity of the
calorimeter should be at least 500 c.c. The larger the calorimeter,
the less the influence of radiation.
Before the investigation is begun, the calorimeter, etc., should
be left in the observation room for some time, until the calorimeter,
the water content of the surrounding jacket, and the liquid to be
employed have assumed the temperature of the room.
The method of Rumford, in which the initial temperature of
the calorimeter is adjusted (from a previous experiment) so as to
be as much below the temperature of the surroundings as the final
temperature is above, can lead, in some measure, to accurate
results only when the temperature adjustment takes place quickly METHOD OF MIXTURES.
and the temperature change amounts to not more than 4 to 50.
To preveqt the condensation of moisture on the outer wall of the
colorimeter, the same should be cooled, before the experiment, to
at least 20 below the temperature of the room.
If the investigation requires considerable time, or if there is a
considerable increase or decrease in temperature, then the influ-
ence of the radiation must be fully taken into account. For
determining this correction, the method of Regnault-Pfaundler *
is, perhaps, most free from objection.
1. The Fore-period.—Before the investigation is begun, the
temperature of the calorimeter is observed at equal intervals of
time, from minute to minute, for a period of ten minutes.
Let these temperatures be &0 .. . #lO. If the ex-
periment is begun at the moment when # must be read off, then
#lO can not be determined directly, but it is ;
//
10 9 ' g
$
—s is the average temperature change per minute for the first
nine minutes of the fore-period.
2. The Principal Period.—The principal period begins at the
moment when the experiment is begun. An increase of tempera-
ture follows, which is observed to a maximum temperature; after
which the temperature decreases, on account of the radiation. The
decrease at first is not uniform, as would be the case if the substance
had given up all its excess of heat to the calorimeter immediately
after reading off the maximum temperature.
It is assumed that the principal period continues through ten
minutes—i. e., after ten minutes the decrease of temperature from
minute to minute is uniform.
Then /0 is the temperature at the beginning of the investi-
gation, and /4 . . . /10 the temperatures observed from minute
to minute during the principal period.
3. The After-period.—Finally, /10 = rO, and r1r2rsri . . . tlO
are the temperatures observed from minute to minute during the
after-period—i. e., the period in which the temperature change, due
* Other corrections, Berthelot, Mec. chim. I, p. 208, 1879; Wiedemann and
Ebert, Phys. Prakt., pp. 187 and 2x5, 1890. SPECIFIC HEAT.
to radiation, has become uniform. Let the temperature changes
during the fore-, principal, and after-periods be represented by
A&, Al, At, then the mean temperature changes of the fore- and
after-periods correspond to the mean temperatutes and r5 of the
two periods ; that is,—
and jr
5 XO 6 IO
It can be assumed, then, that the differences in the temperature
changes A stand in the same ratio as the differences in the corre-
sponding temperatures; if, therefore, tn and A* represent any given
values for the principal period, we have the following proportion :
(4-4) :0»'-jf) = (z.-».)
or,
At=(t -,<> ) + j*.
5 5
If for 4 is substituted the mean value of the temperature read off
at the beginning and end of the nth minute, and for n all values
from n= o to n= xo, the loss by radiation for each of the ten
minutes of the principal period is obtained. If the sum of these A’s
is added to the final temperature tw, we obtain /10+ as the cor-
rected final temperature free from the influence of radiation.
It is calculated in the following manner:
SA =U,+ A\ + A[+ . ■ • zf')
The following example* will serve to illustrate the method.
The temperature of the room is 23.5, and the temperature of the
calorimeter is read off every twenty seconds. The observed tem-
peratures of the calorimeter are as follows :
Time.
Temperature.
Time.
Temperature.
O. 20"
19.78°
9.2o//
24.22°
1.20//
19.80°
I0.20//
24.22°
2.20"
19.82°
IX.20//
24.22°
3.20//
19.84°
I2.20//
24-215°
4. 20//
(Beginning of Experiment.)
13. 20"
24.2x5°
5-2o//
23-54°
I4.20"
24.2X0°
6.20"
24. IO°
15.20"
24.207°
7.20//
24.I90
16.20"
24.204°
8.20"
24.21°
1J.20//
24. 200°
*Wiillner, Physik. 3, p. 407, 1875. METHOD OF MIXTURES.
117
From the 14th interval the temperature decreases uniformly,
o.oi° in 3.20". The value 0.003° corresponds here to Ars in the
formula, and the temperature 24.2050 corresponds to the value r5.
In the fore-period the temperature increases by 0.02° each in-
terval. The temperature immediately before the experiment,
therefore, is 19.86°; the temperature 19.82° corresponds to the
value $5, and 0.02° corresponds to A'K The negative sign must
be taken into consideration. If the calorimeter before the investi-
gation, as in this case, is at a lower temperature than that of the
surroundings, the value is negative, otherwise positive. Hence :
IA = 24.10-j- 24.194- 24.21 4- 24.22 4- 24.22
. , , , 19.86 + 24.21 \
+ 24.22 + 24.215 + 24.215 4 10 X 19-02 j
(0.003 + 0.02 \
——) 10 X 0.02;
24.205 —19.82/ ’
or,
SA = 0.015,
and the corrected temperature,—
= 2 4-210° -f- 0.015 = 24.225°.
(b') Specific Heat of Liquids.
Method of Kopp and Schiff.—The specific heat of a liquid
may be determined in the manner already described, except that
the liquid must be enclosed in a suitable vessel, which, after heat-
ing, is immersed in the water of the calorimeter. The form and
size of the calorimeter, as well as the stirrer, should conform, as far
as possible, with the heating vessel. A ring-shaped stirrer is best
adapted to this work. If wx is the water equivalent of the heating
vessel, the calculation may be made from the following formula:
(PC+a/j) {T— t) =(/ + «/) (j f),
in which w has the same meaning as on page no.
According to the method of Kopp, small, thin-walled, glass
vessels, about 6 cm. high and 1.5 cm. wide, and provided with a
narrow neck about 10 cm. in length, are used as the heating
vessels. The filling is accomplished by means of the arrangement 118
SPECIFIC HEAT.
described on page 30 (Fig. 11). The vessel is heated in a mercury
bath. The mercury during constant stirring is heated uniformly
on a water-bath or, better, in an oil-bath, which-, in turn, is
placed in a sand-bath covered with cotton. Simple beaker glasses
may be used to contain the mercury and oil. The wide portion of
the heating vessel is completely immersed in the mercury, and the
thermometer, which has been previously adjusted, is placed in the
immediate vicinity of the vessel. By regulating the flame, the tem-
perature of the bath may be kept constant to within o. 1 to o. 2 of
a degree.
The water-equivalent wx of the heating vessel of the weight tt gm.
is approximately equal to 0.19 tt.
The method leads to more accurate results if the calorimeter
and heating vessel are of the form proposed by R. Schiff.*
The inner-vessel of the calorimeter, which is best constructed of
platinum, has a capacity of about 600 gm., and contains 500 gm.
of water. The total water-equivalent (including thermometer)
may amount to about 5 gm. (sp. H. of platinum = 0.0324).
A platinum vessel of the form represented in figure 53 with the
cross-shaped outline may be used as a heating vessel. Its capacity
is about 70 c.c., the inner width of an arm is about 1 cm., and the
water-equivalent about 4 gm.; the vessel is filled to five-sixths of its
capacity with water. Of special advantage is its large, good-
conducting, cooling surface; for an elevation of 50 in the tempera-
ture of the calorimeter, the maximum temperature is attained in
from one and one-half to two minutes. Another advantage lies in
the fact that the vessel itself serves as stirrer.
The vessel is heated in the vapor of a suitable liquid (acetone,
methyl-alcohol, benzene, water, toluene, xylene, and mixtures) in
the apparatus represented in figure 54.
A funnel-shaped copper vessel is heated in the vapor of a boiling
liquid in the heating flask, and is connected above with a reflux
condenser by means of two symmetrical tubes joined together in the
form of aY. In the upper portion of the vessel is soldered a
cross-shaped copper shell, about 10-12 cm. in length, and closed
at the lower end; the platinum vessel of corresponding shape can
* R. Schiff, Ann. Chem. Pharm. 234, p. 302, 1886. METHOD OF MIXTURES.
be easily introduced into this shell. The vessel, after heating with
a spirit-lamp, is provided with a thermometer, placed in a copper
shell, covered with a perforated copper plate, which in turn is cov-
ered with flannel, and heated for about twenty to thirty minutes,
until the temperature has become constant for some time, and then
quickly introduced into the calorimeter, which is protected by
means of a wood or cardboard screen.
The thermometer is removed, however, before introducing into
Fig. 53.
Fig. 54.
the calorimeter, and can be replaced by a small calcium chloride
tube. In order to remove the thermometer easily, and have a con-
venient handle for introducing the vessel into the calorimeter, a
thin-walled glass tube, as wide as possible and about 6-8 cm. in
length, is fastened in the neck of the vessel by means of a cork
ring, so that the tube does not project below the cork into the
vessel. The thermometer is then loosely placed in, and when it is
read, the projecting thread must be taken into consideration. 120
SPECIFIC HEAT.
The observation error of the method influences the result only
from 0.5 to, at most, 1 per cent.
Method of Andrews.—When somewhat larger quantities of
a liquid are at hand, this method may be advantageously used.
A heating substance, heated to a definite temperature, is im-
mersed (1) in the liquid to be investigated, (2) in water; then, as
the substance gives up equal quantities of heat to the two liquids,
we have the following equation :
{fc+w) (T-o = (A+ tv) (7;-o,
in which P, C, and T t represent the weight, specific heat, and
temperature elevation of the liquid, Pv Tx tx the weight and tem-
perature elevation of the water, and w the water-equivalent of the
calorimeter (pp. no and 113).
The heating substance consists of a thin-walled glass globe of
sto 10 c.c. capacity filled with mercury. Onto the globe is fused
a capillary tube (50 cm. in length and from 0.6 to 1 mm. in
diameter) provided with two marks and supplied with a funnel at
the top. The distance between the marks is such that the mercury
thread reaches the two marks when heated to about 30 and Bo°.
In regard to the filling of the glass globe, and its heating in a
mercury bath, see pages 77 and 118. The globe is introduced into
the calorimeter at the moment when the cooling mercury passes
the upper mark, and as soon (with constant stirring) as the lower
mark is reached the vessel is removed from the calorimeter, the
temperature of which is then read off.
Tables of specific heats, see Berthelot, Mec. chim. I, pp. 434, 456, 467, and
495, 1879; Thomsen, Therm. Unters. I, p. 46, 1882; Landolt-Bornstein,
Tabellen, pp. 174 to xB6, 1883. Specific heats of organic compounds, R.
Schiff, Lieb. Ann. 234, p. 300, 1886. Specific heats of gases, Wiillner, Exper.
Physik. 111, p. 423, 1875; E. Wiedemann, Pogg. Ann. 157, p. I, 1876, and Wied.
Ann. 2, p. 195, 1877. THE ICE-CALORIMETER.
DETERMINATION OF SPECIFIC HEAT WITH
THE ICE-CALORIMETER.
Method of Bunsen.
Apparatus and Method in General.—A heated substance
is introduced into the calorimeter (Fig. 55) where a definite
quantity of ice is melted. The quantity of ice melted is calcu-
lated from the change of volume, and from this the quantity ot
heat given up by the substance can be calculated.
The calorimeter, which is made of glass, consists of an inner
tube fused to an outer cylin-
drical or oval glass mantle V.
This glass mantle is nar-
rowed at the bottom into a
smaller tube, which is bent
upward and provided, at the
upper end, with a small fun-
nel, and connected, by means
of a forking arrangement,
with the capillary tube A.
The wider portion of the
glass mantle V is filled with
water and the lower part with
mercury. The mercury also
completely fills the tube S,
the outlet of which is immersed in a small vessel filled with mercury.
The water in Vis in part brought to freezing, and the apparatus
i and J filled with ice and ice-water, so that the whole system
assumes the temperature o°. The introduction then of a heated
substance into the inner tube will convert a definite quantity of ice
at o° to water at o°. This melting process is accompanied by a
decrease in volume, which is evident from the fact that the capillary-
tube sucks in a definite quantity of mercury from the small vessel.
Dig. 55.
Calculation.—If this quantity of mercury, obtained by weigh-
ings of the mercury basin, is a gm., then the corresponding vol-
ume at o° is
13-596 C-°- 122
SPECIFIC HEAT.
This represents the decrease in volume due to the melting of the
ice. According to Bunsen, i gm. of ice at o° has the volume of
1.09082 c.c., and 1 gm. of water at o° the volume of 1.00012 c.c.
The melting, therefore, of x gm. of ice produces a decrease of
0.0907 c.c. in the volume.
As the volume has been decreased by
the quantity of ice melted is
13-596 °-c-’
a
i3-596X°-°9°7 gm'
The melting of one gm. of ice requires 79.9 calories (heat of
fusion).
The melting of
a
13-596X0-0907 gm‘
of ice is equivalent, therefore, to
—— = a mean calories (p. 109) of heat.
*3-596 x 0.0907 0.01544
This quantity of heat has been added to the calorimeter by the
heated substance. If the quantity of substance = p gm., its
temperature in Celsius degrees = t, then the mean specific heat of
the substance between o and t° is
a *
0.01544/ t ■
Apparatus and Method in Detail.—The filling of the
glass mantle V with previously boiled water and mercury may be
accomplished in the following manner :
The upper end of the tube, which extends from the bottom of
the apparatus, is immersed in recently boiled water, whence the
glass mantle, by careful heating, is filled to about one-third of its
length with water. The liquid which has been sucked in is heated
to boiling, and the open end of the tube immersed in boiling
* The quantity of mercury corresponding to a mean calorie can be determined
directly by introducing known quantities of water at t° in small glass bulbs into
the calorimeter. (Schuller and Wartha, Wied. Ann. 2, p. 359, 1877.) THE ICE-CALORIMETER.
water. When the water in the glass mantle is for the most part
evaporated, the liquid is allowed to rise again, and the vessel is
in that way completely filled with water free from air. Previously
boiled mercury is then poured in until it has the same height in
the two limbs of the tube (see the wider tube in figure). The
water in the narrower tube is then removed by means of a pipette,
the walls are dried, and it is then filled with mercury by means of
a capillary-tube, so that no air-bubbles adhere to the sides.
The funnel and the capillary suction-tube £ must be fastened in
the mantle-tube mercury-tight.* The latter is a bent tube (Fig.
56), which widens into a pear-shaped opening at the end which is
immersed in the small basin. This widening is necessary to main-
tain a perfect contact between the inner and outer mercury, which
might otherwise be disturbed by the influence of capillarity.
The tube may be prepared in the fol-
lowing manner : The tube is filled with
colored liquid and fused together at one
end, which is then ground off with gly-
cerine and a fine oil-stone, until the
opening is about 0.5 mm. in diameter.
The well-cleansed suction-tube is fast-
ened to the glass mantle, when the ice-
formation in the same has taken place.
A beautiful cylinder of ice can be produced in V (see the shading
in the figure) in the following manner:
Two flasks from one-half to one liter capacity, one of which
contains a large quantity of alcohol, are surrounded by a freezing
mixture (salt and snow) at about 150 to —2o°. The flasks are
then connected, by means of doubly perforated corks, with the
inner tube of the calorimeter, so that the strongly cooled alcohol,
by means of a pump, can be sucked through the tube a number of
times, changing from one flask to the other. The calorimeter is
placed at the same time in snow or ice-water (better, not in freez-
ing mixtiire).
Fig. 56.
There is formed then, after two to three hours, from the interior
* The funnel is not necessary. The tube may be closed with a stopper; the
apparatus is then less liable to be broken. 124
SPECIFIC HEAT.
outward, a clear ice-mantle, which may easily be obtained from
5-10 mm. in thickness, and which will suffice for a large number
of investigations. The ice-mantle should not adhere too tightly
to the inner wall. The ice, therefore, in immediate contact is
thawed by repeatedly filling the tube with water some degrees
above o°.
After obtaining the ice-mantle, the apparatus is packed. If per-
fectly clean, frdshly fallen snow is at hand (kept in a clean box),
the calorimeter is packed as completely as possible in a larger ves-
sel, which is provided with an outflow-cock for the molten ice.
When snow is lacking, use is made of the arrangement repre-
sented in the figure.
The two vessels J and i are made of zinc-plate. An ice-mantle
is formed in the inner vessel from pure distilled water. This man-
tle surrounds the walls of the vessel to a thickness of 2 to 3 cm.
The surface of the water in J is covered with a finely pulverized
ice, and the vessel then provided with a well-closed metallic cover.
The outer vessel is filled with pieces of ordinary ice, provision
being made for the water which is formed to escape.
If the apparatus is so packed and placed in an ice-chest or a
specially cold room, a large number of determinations can be
carried out at long intervals without difficulty.
If the snow or ice-water in the vessel J is not perfectly pure,
the thickness of the ice-mantle in V changes continually. The
accompanying volume change will influence the results more or less.
For the use of pure snow and ice-water a continual decrease in
the melting of the ice-cylinder in V takes place. This is stirred,
therefore; for, on account of the mercury pressure, the melting
temperature in V is a little below o°, and hence a continually less
supply of heat from without takes place.
The investigation is made by connecting the calorimeter with a
suitable pressure apparatus, extension of the suction-tube from
below, or by occasioning an increase or decrease in the ice-cylinder
through the introduction of traces of common salt into the ves-
sel/.
The thawing of the ice-mantle can usually be regulated by raising
or lowering the point of the suction-tube in the mercury basin, so
that the amount of mercury in the basin decreases only a few railli- THE ICE-CALORIMETER.
1 25
grams per hour. This change of weight for the period of the inves-
tigation—usually twenty to thirty minutes—must be taken into
account. Two mercury basins are necessary, which, changing
every half hour, are weighed and connected with the calorimeter
(gently tapping the suction-tube). If the thawing of the ice-
mantle in equal intervals of time is uniform, the investigation may
be commenced. The small corrections are then calculated from
weighings before and after the time of the investigation.
The investigations are carried out in a room the temperature of
which, at most, should not be more than 5 to xo° above o°.
The inner tube of the calorimeter contains some glass-wool on
the bottom, and is partially filled with water (or some other suitable
liquid). Its cork is removed only for the introduction of the sub-
stance. The latter is heated to a constant temperature in a heating
vessel (p. m). The heating vessel and calorimeter are separated
by means of a cardboard screen, and set up so that an easy and
quick transfer is possible.
Pulverized solids are introduced in platinum shells (specific heat
= 0.0324) ; liquids are introduced in small glass globes, which are
filled, almost completely, at the temperature of the heating vessel,
and then fused together. The specific heat of the glass (on an aver-
age 0.19) should be determined by a previous investigation, and the
water-equivalent (pp. no and 113) taken into consideration. Three-
tenths to one gm. of substance is sufficient for most determinations.
calorimetric method has the advantage over the mixture-calorimeter
of a greater and even extraordinary accuracy for the use of small
quantities of substances ; the substantially lower cost of the appa-
ratus, in comparison with the better mixture-calorimeter, should
also be mentioned. On the other hand, extreme care is required
in working with the ice-calorimeter.
Ice-calorimeter and Mixture-calorimeter.—The ice-
In regard to the ice-calorimeter, see: Bunsen, Pogg. Ann. 141, p. I, 1870 ; *
Schuller and Wartha, Wied. Ann. 2, p. 359, 1877; Bliimcke, ibid. 25, p. 154,
1885; Dieterici, ibid. 33, p. 425, 1888, and 38, 1889. Literature on the use of
the ice-calorimeter for measuring the heats of solution, neutralization, vaporiza-
tion, and combustion, see the following chapters.
* This method of measuring the mercury in a graduated tube is less accurate
than the modified method of Schuller and Wartha. 126
HEAT OF FUSION.
XIII. HEAT OF FUSION.
By the heat of fusion is meant that quantity of heat, measured in
calories, which is required to melt i gm. of a substance.
The heat of solidification is the quantity of heat set free when
i gm. of a substance is changed to a solid state.
The molecular heat of fusion or solidification is the product
of molecular weight and the heat of fusion or solidification, there-
fore the heat of fusion or solidification referred to one molecular
weight in grams.
Principle and Calculation.—The method of mixtures is
usually employed.
i. If the melting point of the substance is below the tempera-
ture of the room (benzene, etc.), the substance is allowed to
solidify and is introduced, in a suitable vessel, into the calorimeter,
which contains at least enough liquid, so that the final temperature
is above the melting temperature of the substance.
The quantity of heat which the introduced substance takes up is
the sum of three values :
(a) The quantity of heat taken up in heating from the tempera-
ture /, the temperature of the solid substance when introduced into
the calorimeter, to the melting temperature /0. A knowledge,
therefore, of the specific heat cx of the solid is necessary.
(b) The quantity of heat taken up in changing from the solid to
the liquid state at the temperature /0 (heat of fusion).
(c) The quantity of heat required to heat the liquid from the
temperature /0 to the final temperature of the calorimeter r. The
specific heat c 2 of the liquid substance must therefore be known.
Let L represent the heat of fusion of the substance, px the weight
in grams of the substance used, p2 the weight of the water in the
calorimeter, the initial temperature of which is T; wx the water-
equivalent of the vessel containing the substance, w2 the water-
equivalent of the different parts of the calorimeter ; then the
quantity of heat given up by the calorimeter and contents HEAT OF FUSION.
127
= (/2+ w2) (T —r), and the quantity of heat taken up by the
substance and vessel
—P\ l>i (4) —O+P' + ci (T —Ol "t" w\ (r
equating these two values we obtain
(A + T~ T) iT Q —P\ Ol — *1) + C‘l iT —Q]
A
2. If the melting point of the substance is below the tempera-
ture of the room in general, the heat of solidification is determined.
The procedure is the reverse of that just described.
The substance is heated above the melting point f0 to the tem-
perature tv and introduced into the calorimeter, the temperature r
of which lies below the temperature /0. Then, if Eis the heat of
solidification of the substance, and the remaining letters have the
meaning given above, the quantity of heat given up by the intro-
duced substance (-(- vessel) is
—P\ (A —O + +A(A T)1 + (A —T)
and the quantity of heat taken up by the calorimeter
= (A + w2)(r— T)-
Therefore
„ _ (A + w2)(r —T) —r)— A 02 (/i —V+
and the heat of combustion for constant volume is
Qv = (p + w'>
The heat of combustion is usually referred to constant pressure.
This reduction of the heat at constant volume to constant pres-
sure at 180 can be made, for solids and liquids of the formula
CmHreOr, according to the formula:
QP =Qv + 0.291 ( r),
where Qp and Q„ are the heats of combustion at constant pressure
and constant volume, and n and r the number of hydrogen and
oxygen atoms.
The following formula is of general application :
Qp : Qv 0.02 (j T,
q represents the number of gram-molecules of gas which dis-
appear in the reaction, and T the absolute temperature;
0.02 X 291 K— 5.82 K must therefore be added to the observed
heat of combustion at 180 for each gram-molecule of gas which
disappears, and the same number of calories subtracted for each
gram-molecule of gas formed.*
Apparatus.— i. The Calorimeter.—The calorimeter is placed
in the experimental-room, the temperature of which must be care-
fully regulated.
The inner cylindrical brass vessel (20 cm. high and 15 cm. wide
and 500-600 gm. in weight) rests in a larger double-walled vessel
of the same material, which is filled to a height of 10 to 15 cm.
with water. The two vessels are isolated by means of pieces of
ebonite, which are fastened together by means of glass rods. The
stirring arrangement (about 200 gm. in weight) may be made of
*Ostwald, Allgem. Chem., 2. Aufl., Bd. 11, pp. 81 and 370, 1892; Berthelot,
Mec. chim. I, p. 116, 1879; and Ann. chim. phys. (5) 23, p. 168, 1881. HEAT OF COMBUSTION.
143
three ring-shaped brass plates, which are firmly fastened together
by means,of wires, so that the cylindrical discs lie one above the
other, and so that the wires are united at the top of, and in the axis
of the cylinder.
The stirrer should take up the entire space between the outer
wall of the bomb and the inner wall of the calorimeter vessel. For
a bomb, therefore, of 10 cm. and a calorimeter of 15 cm. in diam-
eter, the discs should be 10.5 cm. and 14.5 cm. in diameter. The
stirrer must be moved uniformly and in a vertical direction. The
wires, therefore, at the point where they are joined together, are
fastened to a slide which moves in a vertical direction, owing to its
being fastened eccentrically on a disc which is rotated by means
of a turbine.
This movement must take place so that, for the deepest position
of the stirrer, the lower plate must come almost in contact with the
bottom, and for the highest position the upper plate must come
almost to the surface of the water.
The upper discs of the stirrer are provided with two openings for
the introduction of the thermometer.
The (Beckmann) thermometer must be carefully tested. It is
graduated to or yTy of a degree, so that, by means of a micro-
scope, it may be read accurately to 0.002°. (The tapping of the
thermometer must not be forgotten.) The contrivance which sup-
ports the stirring apparatus is fastened to the outer calorimeter
mantle.
2. The Bomb (Fig. 60).—The bomb consists essentially of a
cast-steel vessel A, which is closed air-tight by means of the steel
cover B. The interior of the vessel and cover is lined with plat-
inum. For a bomb with a capacity of 300 cm., about 1200 gm.
of platinum and 2700 gm. of steel* should be used, so that, with
the addition of the brass contrivance which supports the bomb in
the calorimeter, the combined weight amounts to about 4 kgm.
The manner in which the bomb is closed by the cover is evident
from the figure.
* These are the approximate weights for the bomb of Stohmann ; Berthelot’s
bomb of 200-250 cm. capacity requires not more than half this quantity of platinum.
The calorimeter is correspondingly smaller. 144
THERMOCHEMICAL CONSTANTS.
Fig. 60. HEAT OF COMBUSTION.
The platinum edge of the cover is carefully slipped into the con-
ical opening of the vessel A. The cover is pressed down firmly
by means of a large screw, which surrounds and screws tightly to
the outside of the vessel. In the upper surface of the screw are
two holes, in which are placed two iron pegs (not shown in the
figure). By means of these the screw C can be tightly turned.
The bomb, after filling with oxygen and the substance, is firmly
fastened in a steel ring consisting of two halves covered with white
lead, and tightly closed by means of the steel pegs. Previously,
however, the upper portion of the conical part of the cover should
be carefully covered with grease.
The contrivance a in figure 60 is used for filling the bomb with
oxygen and the gases to be combusted ; likewise for the subsequent
removal of the gases resulting from the combustion.
It consists of a hollow, thick-walled, steel cylinder, which can be
so adjusted by means of the screw arrangement, which is from 3
to 4 cm. long, that the conical valve below is either tightly closed,
or that the opening for the outflow and inflow of gases is in direct
communication with the short platinum tube, bent at a right angle,
which extends from the lower end of the screw arrangement into
the interior of the bomb.
When the screw is turned down as far as possible, the bomb is
closed air-tight; half a turn upward then is sufficient to allow the
gases to enter.
For solid and liquid substances there is situated in the interior
of the bomb a small platinum vessel b resting in a platinum ring,
which can be raised or lowered on a heavy platinum wire, which is
fastened to the cover. This arrangement is necessary so that the
substance can be placed just below the wires c c', by means of
which the combustion is induced.
Inasmuch as the wire c, which is firmly soldered to the plati-
num support of the vessel, is connected with the bomb, thus forming
a conductor, c' must be carefully insulated. This can be accom-
plished by means of a small platinum cone which is connected
with c' and inserted, air-tight, in the cover. The cone is covered
with thin black rubber. (A shellac covering is less durable). A
small ivory ring, at the outlet through the cover, is shoved over
the platinum rod which supports the cone; the ring is made air- 146
THERMOCHEMICAL CONSTANTS.
tight by means of a screw, which simultaneously exerts a pressure
on the rubber, thus forming a very thin membrane. Care should
be taken (especially before the first combustion) that small pieces
of rubber do not fall into the interior of the bomb during the
tightening of the screw; otherwise the pieces must be removed.
The danger from the burning of rubber can be prevented by
placing a piece of mica, through which a hole has been bored,
between the cover and the rod of the cone.
The burning of the substance is brought about by means of fine
iron wire (Blumendraht) which is melted off at a glowing heat.
The wire is rolled spirally on a strong needle and is fastened to c
and c' by means of fine platinum wires. In order to remove the
thin coatings of non-conducting iron oxide which may be formed
on c and c' during the combustion, the ends of the wires are
immersed from time to time in molten potassium bisulphate.
As equal lengths of the iron wire have approximately equal
weights, a correction may be easily calculated for the iron which
burns to iron oxide; equal lengths of wire = 5 cm. are always
taken so that the weight (about 0.006 gm.) need be determined
only once.
The wire is heated by means of three Bunsen chromic-acid
elements; the glowing particles of oxide from the burning wire
fall upon the substance immediately under the wire and start the
combustion.
3. Contrivance for the Introduction of Oxygen.—The oxygen to
be used should be free from chlorine and carbon monoxide. Any
chlorine present may be removed by passing the gas through
potassium hydrate, while the carbon monoxide can be best removed
by means of palladium chloride. Combustible gases and small
particles of oil from the pump are rendered harmless, in that the
oxygen is first passed through a copper tube heated in a com-
bustion furnace, and after cooling is introduced through a narrow
spiral tube into the bomb. The main portion of the oil from the
pump is held back mechanically, in that a large number of fine
wire gauzes are placed at very small distances from each other in a
metallic cylinder immediately behind the pressure-valve of the
pump. The presence of carbonic acid causes no inconvenience.
To avoid corrections, the oxygen should not be dried, but should
be saturated with water vapor. HEAT OF COMBUSTION.
147
It is very convenient to make use of the commercial oxygen
tanks, in which the oxygen exists under a pressure of about 120
atmospheres. The gas can best be pumped from an ordinary
gasometer into the calorimetric bomb by means of a good suction-
or pressure-pump; the tube of the pump should be surrounded
by a mantle of flowing cold water; otherwise the heat from
friction may occasion explosions between oil and compressed
oxygen.
The pump should be provided with a manometer which indicates
Jg- atmospheres.
Details of the Method of Operation.—The water-equiva-
lent of the calorimeter and stirrer (pp. no and 113) can be
determined simply by multiplying the weight in grams by the
specific heat of brass = 0.094. However, it is perhaps better to
determine the specific heat of the particular kind of brass used in
the calorimeter. The weight of only that portion of the stirrer
which is immersed for the highest position in the water of the
calorimeter can be taken into account.* A further determination
of the water-equivalent of the calorimeter and stirrer, so far as the
latter comes into account, may be made by quickly pouring a
quantity of tvater, from a protected vessel heated to a constant
temperature (about 6o°), to the necessary height in the calorimeter
(containing the stirrer and thermometer). The water-equivalent
of the metallic portions (including the thermometer) can be calcu-
lated from the quantity of heat given up to these portions, by
multiplying the temperature difference of the water by its weight
and dividing the product by the temperature elevation of the
metallic portions. For the dimensions and weights given for the
calorimeter and stirrer, the combined water-equivalent amounts to
about 60 to 70 gm. For the water-equivalent of the portion of
the thermometer immersed see also page 114.
The water-equivalent of the bomb with brass foot can be accu-
rately determined by several methods ;
1. The number of grams of steel, platinum, and brass used are
* A direct and perhaps more accurate way of determining the water-equivalent
of apparatus, see Stohmann, Jour, prakt. Chem. 39, p. 528, 1889. 148
THERMOCHEMICAL CONSTANTS.
multiplied by the corresponding specific heats (specific heat of steel
= 0.1097, platinum = 0.0324, and brass = 0.094).
2. The bomb, together with the stirrer, can be introduced into
the calorimeter vessel, and water, previously heated to exactly t°
(6o°), added until the bomb is immersed. The sum of the water-
equivalents of the bomb, calorimeter and stirrer can then be calcu-
lated (see p. 147).
3. The bomb is heated for some time in a water-bath to
about 30° until the temperature becomes constant to about y-l-g-
-of a degree; it is then introduced as quickly as possible into the
calorimeter containing sufficient water at a constant temperature
equal to that of the room. The temperature elevation of the con-
tents of the calorimeter, multiplied by the total water-equivalent of
the same, and divided by the decrease in temperature of the bomb,
gives the water-equivalent.
A small correction is to be introduced on account of the water
which adheres to the bomb during the heating. The approximate
weight of the same is determined from several weighings of the wet
bomb. If the outer surface of the bomb is covered with a trace of
grease, the adhering water amounts to only a few grams, and it is
necessary simply to subtract the number of grams from the observed
water-equivalent of the bomb.
The water equivalent of the bomb, which for the weight given
would amount to about 350 gra., can be determined by the preced-
ing methods to from 1 to 2 gm.
In carrying out the experiment, the bomb is immersed in the
water so far that only the handle of the closing screw a remains
uncovered. The calorimeter, for the dimensions of the apparatus
given, should contain about 2500 gm. of water.
The preceding is subject to some variation, depending upon
whether the substance to be combusted is a solid, liquid, or a gas.
A large excess of oxygen must be used in the case of solids.
The oxygen is pumped into the bomb until the manometer shows a
pressure of about 25 atmospheres. A bomb of 300 c.c. capacity
should contain from 10 to 11 gm. of oxygen. The quantity of
substance to be burned is so chosen that, after the combustion, the.
remaining oxygen occupies at least one and a half times the volume HEAT OF COMBUSTION.
149
occupied by the gases formed in the combustion. For 10 gm. of
oxygen usually 3 gm.; i. e., 30 per cent, of the quantity may be used
in the combustion ; then, on the assumption of complete combustion
to C02 and H2O, the quantity of substance to be used in the com-
bustion can be calculated (. g., 1 gm. of naphthalene corresponds
to about 3 gm. of oxygen).
If one is not certain that the combustion is complete, the com-
bustion gases are slowly conducted through a solution of palladium
chloride. The least quantity of CO will produce a black precipi-
tate, and may thus be detected.
For many substances, in oxygen under a pressure of 25 atmos-
pheres, the combustion is not induced by the molten iron wire.
The combustion may be facilitated in such cases by covering the
substance with a small weighed quantity of an easily combustible
substance (a few grams of naphthalene) ; the heat set free in the
combustion of that substance will start the combustion in the
original substance. Of course, a small correction must be intro-
duced in this case. The heat of combustion of the substance used
to induce the reaction is multiplied by the quotient of the weight
used, divided by the molecular weight, and the product subtracted
from the total heat of combustion. Only a few substances (oxalic
acid, mellitic acid) show difficulties in their combustion according
to this method. Solid substances should be made as compact as
possible for the combustion—in the form of pastilles, or, when the
substance can be fused without decomposition, in the form of a
solidified fusion.
A steel arrangement, constructed on the plan of the diamond
mortar used in crushing minerals, is used as a pastille press. The
inner part has a suitable width and the bottom can be removed.
The substance is previously weighed. A press of the hand is fre-
quently sufficient to produce the necessary compactness in the
pastille.
If the substance to be combusted is a volatile liquid (aldehyde,
ether, benzene, etc.), a correction relative to the heat of vaporiza-
tion must be introduced, for a portion of the substance is com-
busted in the gaseous and a portion in the liquid condition. For
the calculation of this correction, see Stohmann, Jour prakt. Chem.
40, pp. 78 and 342, 1889. THERMOCHEMICAL CONSTANTS.
The heat of combustion has reference entirely to the liquid
state.* The liquid is introduced into a small glass globe, which is
closed by fusion, and which is so thin-walled that a slight move-
ment of the bomb, immediately before the beginning of the experi-
ment, is sufficient to break the globe. Berthelot, Pierre, and
Matignon,f however, have proposed that the liquid be contained in
a small platinum capsule, which is surrounded by an envelope of
gun-cotton, closed at the top by means of a thread of the same
material.
Gaseous substances should be mixed with no more oxygen than
is necessary for their combustion to carbonic acid and water. At
all events, only a very slight excess of oxygen is to be recom-
mended (about i per cent.). The combustion in this case is
almost always complete for atmospheric pressure. The gases
formed in the combustion should be tested for carbon monoxide.
The weight of the combusted gas may be determined at the end of
the experiment by slowly conducting the gases contained in the
bomb through dissolved and over solid potassium hydrate. The
apparatus is most conveniently filled (in case it is not necessary to
mix the gases outside of the bomb) as follows ; After exhausting
the bomb, the gas to be combusted is first introduced, then the
volume of oxygen necessary for the combustion is calculated, and
the same, by observing the pressure indicated by the manometer, is
introduced into the bomb in slight excess.
The combustion of the substance introduced into the bomb
takes place almost instantaneously. Some minutes (three to four),
however, are required for the equalization of the temperature in
the calorimeter. The experiment is begun after the bomb has
remained for some time in the calorimeter. The temperature of
the apparatus at the beginning of the experiment should be about
as much below the temperature of the room as it is above the
temperature when the experiment is completed. The temperature
* For the comparison of the heats of combustion of different substances it is
necessary to refer them to the same state (better, the gaseous state). Then the
heats of fusion and evaporation must be considered. See Ostwald, Lehrb. Allgem.
Chem., 2. Aufl., Bd. 11, p. 371, 1892.
f Berthelot, Compt. rend. 115, p. 201, 1892. HEAT OF COMBUSTION.
151
elevation usually amounts to several degrees. The influence of
radiation, therefore, should be taken into account according to
page 115.
From the observed thermal effect the heat of combustion of the
substance is calculated according to page 142. First of all, how-
ever, small corrections are to be deducted from the number of
calories calculated from the experiment.
1. If a is the weight in grams of ferrous oxide formed by the
burning of the spiral, and if, according to Berthelot, the oxidation
of 1 gm. of iron to ferrous oxide sets free 16.01 X of heat, then
a 16.01 X must be deducted from the observed thermal effect.
2. The nitrogen of the air which was not removed before the
introduction of the oxygen, and which still remains in the bomb,
is burned to nitric acid. The acid formed is taken up by the con-
densed water, and, after being completely washed from the bomb,
its quantity can be determined by titration (dilute sodium carbonate
and methyl-orange). For each gram-molecule of aqueous nitric
acid (63 gm. FIN03aq) formed 143 X, according to Berthelot, are
to be deducted.
3. A bomb of 300 c.c. capacity, and at a pressure of 25 atmos-
pheres, contains somewhat more than 10.5 gm. of oxygen. This
oxygen must go through the temperature change. As the specific
heat is 0.2175, number of grams of oxygen (10.5) must be
multiplied by this number, and the product, which is the water-
equivalent of oxygen, must be added to the total water-equivalent
of the colorimeter and bomb.
The sum of all these corrections has only a slight influence on
the result.
The correctness of the bomb should next be tested, naphthalene
being used in the combustion.
The quantity of heat set free in the combustion of 1 gm. naph-
thalene, at constant volume, according to the investigations of
Berthelot, is 96.94 X.
(The values for nineteen determinations vary between 97.43 and
96.51 X.)
The bomb of Berthelot, Stohmann, and others is made in Paris
(by Golaz).
The high price of the apparatus, owing to the large quantity of THERMOCHEMICAL CONSTANTS.
platinum used in its construction, has hindered somewhat its intro-
duction into the laboratory.
Mahler * has recently described a bomb which is analogous to
that just described, and made of half-tempered steel. The interior,
instead of being covered with platinum, is furnished with a layer
of strong enamel, which must be renewed occasionally. This
bomb can be used not only for technical, but also for scientific
purposes. Other investigations in this direction, however, are
desirable.
On heats of combustion, see Thomsen, Therm. Unters., Bd. IV, p. X; Ost-
wald, Allgem. Chem. 11, p. 361, 1892; Armstrong, Phil. Mag. (5) 23, p. 73,
1887 ; Briihl, J. pr. Chem. (2) 35, pp. 181 and 209, 1887 ; Thomsen, Zeit. phys.
Chem. I, p. 369, 1887, and 7, p. 55, 1891; Dieffenbach, ibid. 5, p. 566, 1890.
Tables of heats of combustion : Stohmann, Zeit. phys. Chem. 2, p. 29, 1888 ;
6, p. 335, 1890, and 10, p. 410, 1892; ibid.. Literature on heats of combustion.
Determination of heats of combustion with the ice-calorimeter: Schuller and
Wartha, Wied. Ann. 2, p. 371, 1877.
Heat of Formation.—The heat of formation of an organic
compound,—i. e., the quantity of heat set free or absorbed in the
formation of 1 gram-molecule of the substance, can be calculated
from the heat of combustion of the compound. The calculation
can be made according to the principle of Hess, by subtracting
the heat of combustion of the compound from that of its elements.
We have then :
or, in large calories K :
c, H4 =C, 02 + 2(II2) O) - CH4, 04;
223 = 976 + 2 X 683 2“9-
See, among others, Ostwald, Allgem. Chem. 11, p. 215, 1892; Berthelot, Mec.
chim. 1, 329, 1879.
* Mahler, Compt. rend. 113, p. 774, 1891. CRYSTAL MEASUREMENTS.
153
XVI. CRYSTAL MEASUREMENTS.
1. THE REFLECTION GONIOMETER OF
WOLLASTON.
Principle.—The goniometer is used chiefly for measuring the
angles of crystals,—i. e., those angles which the crystal faces form
with each other.
Let the angle which two crystal faces form with each other be
represented by a—on in (Fig. 61). A is a small mirror, so
placed that the image of a suitable object at F, when viewed past
the edge of the crystal by the eye situated at A, will appear in
the direction A E. The crystal is
then placed in such a position (om n)
that the image of F reflected from the
crystal face 0 n appears in the same
direction A n as the image formed by
the mirror E. For this position of
the crystal the two images of F re-
flected from the crystal surface on
and the mirror E to the eye of the
observer coincide. The crystal is
then rotated about the crystal edge
n as axis until the two images again
coincide, when the crystal will have
Fig. 61.
rotated through the angle a'=iBo°—a and taken the position
no' in' (Fig. 6x). The image of F, in this case, is reflected from
the surface nm = n in'. The desired angle then is a 180°
Apparatus I.—The apparatus in its simplest form is represented
in figure 62.
A circle E graduated to half degrees is provided with a vernier
(p. 218), and is movable about the axis G. The instrument is
provided with a double axis. If the knob Gis turned, the circle
E and also the jointed arrangement KL M, which carries the
crystal, are rotated. If, however, the inner axis is turned by means
of the knob J, the crystal support alone is turned. The graduated CRYSTAL MEASUREMENTS.
circle may be firmly clamped by means of the pressure screw
UTS.
The crystal a is fastened in a suitable position on the small disc
Q by means of wax. The adjustment of the same (p. 155) is
made possible, first, by the fact that the axis O which carries the
disc Q may be turned in its support JVhy means of the knob P ■
Fig. 62.
and, second, by the fact that the arrangement ML K is movable at
the joints.
Yrepresents a small mirror which is usually fastened to the foot-
plate Aof the instrument, and is movable about an axis. For a
definite position of the mirror the image of a suitable object is
visible.
As signal, use may be made of a mark x on the window or (if
not too near) the cross-bars of a window, the edge of a roof, etc. THE REFLECTION GONIOMETER.
Or the window may be darkened and then, at a sufficient distance,
provided with a signal, which is a cross-formed slit about 5 cm. long
and 0.5 cm. broad, and which is lighted by means of a gas-flame.
Method of Operation.—The apparatus is set up so that the
plane which passes through the middle of the signal on the window
and perpendicular to the plane of the window is parallel to the
graduated circle EE. If the mirror yis fastened to the foot-plate
so that the edge next to the window is parallel to the axis of the
measuring circle, then, for the proper adjustment of the instrument,
the image of the horizontal bar of the window must be parallel to
the same edge of the mirror.
The crystal is fastened to the small disc Q by means of wax, so
that the edge to be measured, for a suitable adjustment of the joint
L, falls as nearly as possible in the line of prolongation of the axis
of the measuring circle. To facilitate the centering of the crystal
the axis K should be moved in a slide (not shown in Fig. 62, see
p. 157). If the crystal is approximately centered, then, on rotating
the knobs G or J through 360°, the edge to be measured should be
displaced from its position only very slightly.
The crystal must then be adjusted. For this purpose the mirror
y is placed so that the horizontal and vertical bars of the window
are visible in the middle of the field of view. If the eye is placed
near the approximately centered crystal, then, on rotating the knob
J, the image of the window-bars reflected from the mirror is seen in
the two crystal surfaces, the angle between which is to be measured.
If the horizontal and vertical bars of the window appear inclined in
the image from the crystal, and at the same time appear normal in
the mirror and parallel to the edges of the mirror, the adjustment
is inaccurate.
The image then reflected from the crystal and that reflected from
the mirror y are not brought to perfect coincidence on rotating J.
If the attempt be made to perfect the adjustment by turning the
knob Pon its axis or by a movement of the jointed contrivance
K L M, it will be seen in most cases that a movement of either of
these is not sufficient of itself to cause the images from the two crys-
tal faces to appear in the same direction as that from the mirror.
By combining these two movements, however, such an adjustment,
after a little practice, is readily made. CRYSTAL MEASUREMENTS.
After the adjustment has been made, it is only necessary to deter-
mine the angle through which the divided circle must rotate in
bringing the images from the two crystal faces successively in coin-
cidence with that from the mirror y. The observed angle, of
course, is the complement of the angle to be measured. During
the observations on the two surfaces the eye should remain as
nearly as possible at the same position.
With careful adjustment and well-formed crystals, this method is
Fig. 63.
accurate to within two to three minutes, which is sufficient for most
chemical purposes.
Apparatus II.—A more complete form of apparatus is repre-
sented in figure 63.
K is the divided circle with a double axis A a and Bb\ n is
the vernier, which is illuminated through the white paper r by
means of a small flame and read by means of the microscope /;
is a micrometer screw, the threads of which turn in the
grooves of the circular head B, so that the turning of the knob p THE REFLECTION GONIOMETER.
produces a very slight rotation of B, thereby increasing the ac-
curacy of the adjustment. In order that B may be free to move
until approximately adjusted, the knob p is pressed down until the
small projection on the spring below enters the opening in the
frame i, which holds the screw in the lower position.
The centering and adjustment contrivances are essentially differ-
ent from those of apparatus I.
The contrivance for centering consists of two slides lying one
above the other and joined to the axis of rotation. By means of
the screws yy these slides can be moved in parallel planes in direc-
tions which are perpendicular to each other. Attached to this is
the adjusting apparatus, which consists of two cylindrical sections
movable, by means of the screws x x, in planes perpendicular to
each other. A small disc, which serves as the crystal support, is
fastened to this contrivance by means of the screw v.
The instrument is also provided with a telescopef with cross-wires
fastened to the support T. By means of the screw q and bar t the
telescope may be moved parallel to itself, and may also be rotated
in a plane perpendicular to t, so that it can be directed exactly
toward the axis of the divided circle K.
Method of Operation.—The apparatus is first placed in the
proper position, which may be determined by means of a mirror
(p. 154) or by means of the telescope.
The telescope, which is provided with cross-wires, is focused by
moving the eye-piece 0 sharply on the signal (the cross-bars of a
window at the opposite end of the room, etc.). When the image
of the object and the cross-wires lie exactly in the same plane, then
a movement of the eye will produce no change in their relative
positions.
After the apparatus has been set up, the crystal, which is fast-
ened on with wax, is centered.
For this purpose the telescope is changed to a microscope, either
by removing the eye-piece or by'placing a lens in front of the objec-
tive. The microscope thus formed is focused on the crystal, which
can be regarded as centered only when the edge to be measured
remains in the same position during the rotation of the crystal.
The crystal is fastened on the disc, so that the edge to be meas-
ured is approximately centered. One of the two screws y should 158
CRYSTAL MEASUREMENTS.
be placed parallel to the telescope. The edge to be measured is
then raised or lowered by means of the second screw y until it
appears in the middle of the field of view. If the axis Ais now
rotated through 90° and the centering screw turned, which is placed
perpendicular to the telescope, then the edge must remain in the
same position, and therefore be centered.
The adjustment, which is made by means of the screws xx, is
accompanied by certain difficulties until the operator has had some
experience.
The microscope is again converted into a telescope, and, after
focusing on the cross-wires and the crystal, the latter is rotated by
turning the axis A a around the approximately centered edge which
is to be measured. The reflected image of the window-bars and
the crystal surfaces, if necessary with the help of the screws x x, are
brought into the field of view in the telescope. The adjustment is
inaccurate as long as the directions of the reflected window-bars
appear inclined to those of the cross-wires.
The image reflected from the surface, which is parallel to one of
the adjustment screws, is brought into the field of view first and
the other screw turned until the image coincides with the middle
of the cross-wires ; the image from the second face is then brought
into view and corrected by means of the first screw ; the adjust-
ment of the first face is thereby slightly changed, the change being
smaller the nearer the face is parallel to the screw. By small sub-
sequent corrections the adjustment is easily obtained, so that the
images from the two surfaces, as well as from all other surfaces in
the same zone, move along the vertical wire when the crystal is
rotated.
After some experience, the operator, regardless of any special
rules, can easily make the proper adjustments. The turning and
reading of the divided circle is accomplished by means of the knob
B (see p. 155).
Measurement of Crystal Angles in General.—The crys-
tals should be carefully selected, and the faces which are to be
observed should not come in contact with the fingers. They are
rubbed off with soft leather and placed on a ball of soft wax, care
being taken not to allow the wax to come in contact with any face
which is to be measured. THE REFLECTION GONIOMETER.
159
In most cases it is desirable to measure all the angles of a given
zone, so far as the condition of the crystal will permit. If the
crystal is §mall, one centering is sufficient for all the measurements
of the angles of parallel edges. It is placed, then, in the middle
of the zone to be measured ; otherwise each edge is to be sepa-
rately centered, whereby the adjustment remains unchanged. As
the accuracy of the results depends upon the condition of the
crystal faces, it is desirable, first of all, to project as carefully as
possible, on the plane of a paper, a sketch of the crystal, repre-
senting the separate faces by the letters a, b, c, etc., and then note
down, with the measurements of the faces referred to, the necessary
remarks on the condition of the reflected image, etc. From the
different measurements of the angles of equal value then is selected
a mean v'alue, taking into account the accuracy of the various
measurements. In many cases it is advisable to repeat the measure-
ments, using different crystals.
If the crystal face is not uniform, but uneven, curved, or broken,
several images, or parts of images, are usually seen in the reflec-
tion. The measurements, of course, are then more or less inaccu-
rate, depending upon the sharpness of the image.
Care should be taken, especially for clear, transparent crystals,
that the somewhat colored images produced by total reflection from
the interior of the crystal and thrown into the field of view of the
telescope, are not mistaken for the desired images.
In case of doubt it is only necessary, during the rotation, to
observe the crystal with the microscope, formed as previously
explained, to determine whether the illuminated surface is turned
from or toward the signal, and to determine, therefore, whether
the rays from the interior of the crystal or those from the outer
surface are reflected into the telescope.
Substances for investigation : Quartz-crystal, prism angle 120°;
Iceland spar, rhombohedral angles 740 44' and 105° 16'; alum,
octahedral angle 109° 28'.
Goniometers with horizontal measuring-circles, see Groth, Phys.
Krystallographie 11, p. 560, 1885 ; goniometer as refractometer,
ibid. p. 585. CRYSTAL MEASUREMENTS.
2. THE MICROSCOPE, WITH POLARIZING
ATTACHMENTS.
Apparatus.—The microscope of Fuess, represented in figure
64, consists, in its essential parts, of the tube b, with a system of
lenses movable in the double-walled tube p, the objective-stage T,
the mirror below, and the polarization attachments j and r, which,
for investigations in polarized light,* can be fastened above the
eye-piece and below the objective-stage.
The objective-table T consists of a plate which can be rotated
around the vertical axis of the instrument. This plate is graduated
in degrees and can easily be moved with the fingers. The plate i
firmly fastened to the stand below projects over the true stage. On
the upper surface of this projection is a mark which serves as an
index for reading the divisions on the movable plate T.
The tube ris firmly fastened to the plate i. The polarization-
tube, closed by means of a lens, can be shoved into this tube from
below. The polarizing-tube contains a Nicol prism (or Prazmowski
prism, p. 203), and is rotated in the outer tube r, so that the
zero point coincides with a definite mark on r. For this position
the principal section of the prism falls in the plane of the sketch.
Two springs are fastened to the movable plate by means of the
screw q, in order to hold the substance to be investigated firmly to
the stage.
The tube b can be moved in a vertical direction on the outer
tube p.
The instrument is roughly adjusted by taking hold of the tube
on the edge f and pressing down ; the finer adjustment is accom-
plished by means of the micrometer screw m. The head of this
screw is usually graduated, thus making it possible to measure the
vertical movement of the microscope accurately to the thousandth
of a millimeter.-j-
The double-walled tube p consists of two tubes, the inner of
which can be turned through a small angle by means of the two
*On polarized light, etc., see the section Rotation of the Plane of Polariza-
tion, p. 203.
f Groth, Physik. Krystallographie, pp. 33 and 648, 1885. 161
MICROSCOPE WITH POLARIZING ATTACHMENTS.
Fig. 64. 162
CRYSTAL MEASUREMENTS
screws n and m (Fig. 65), the axes of which are mutually perpen-
dicular.
This makes it possible to center the tube b, a cross-section of
which is represented by the innermost double ring (Fig. 65), so
that its vertical axis coincides exactly with the axis of rotation of
the stage, and hence so that an object brought into the middle of
the field of view of the objective does not change its position on
rotating the stage—a condition which is necessary for the measure-
ment of plane angles.
Of the different Hartnack objectives 4, 7, and 9, the first, which
magnifies, according to the eye-piece, from 90 to 200 diameters, is
most frequently used ; if the magnification is still to be diminished,
the lower lens of the objective must be removed. The instrument
is provided with three eye-pieces, the form of which is represented
Fig. 65.
Fig. 66.
in figure 66. Between the upper and lower lenses of the eye-piece
is a cross-wire or glass micrometer, which can be brought sharply in
focus by adjusting the inner tube A. A small screw aof the eye-
piece passes through a vertical slit of the tube b, thus making it
possible to keep the cross-wires always in the same position, namely,
that parallel to the two polarizers when the zero points of their
scales correspond respectively with the fixed marks on the tubes.
Inasmuch as the position of the principal section undergoes slight
change in time, it must be tested from time to time by determining
the directions of vibration in a crystal plate (. g., a rhombohedral
crystal of prismatic form).
The tube s for the analyzer can be placed on the eye-piece (see
p. 203). This tube, which contains a second Nicol or Prazmowski
prism, is provided with a circular scale which can be rotated past
the fixed mark on the plate f. MICROSCOPE WITH POLARIZING ATTACHMENTS.
163
If the analyzer and polarizer are adjusted so that their zero points
coincide with their corresponding fixed marks, then the two Nicols
are crossed and their principal sections coincide with the lines of
the cross-wire.
The slit tt represented in figure 64 serves as a receptacle for the
slide zz, which contains a Biot quartz-plate. This plate is intro-
duced to recognize, through the change of tint of the quartz-plate,
a slight double refraction in the object, and to determine the direc-
tions of vibration in the crystal under investigation.
(a) Measurement of Plane Angles.
By plane angle is meant that angle which the two edges of a
crystal face, lying horizontally on the objective-stage, form with
each other.
For the measurement of this angle the Nicols are unnecessary ;
the analyzer should always be removed in such cases.
The crystal must be centered as accurately as possible; i. e., the
point of intersection of the two edges whose angle is to be measured
must be brought into the puddle of the field of view, so that on
rotating the objective-table it remains in the same position,—at the
middle point of the cross-wires (see p. 162). This centering, after
a little practice, is accomplished easily and quickly if, when the
centering has once been approximately made, the stage be rotated
and the axis of the tube suitably adjusted by means of the screws
m and n (Fig. 65), so that the point of intersection of the edges
during the rotation of the stage describes each time a smaller circle
around the middle point of the cross-wires. By careful movement
of the object then the complete centering is easily accomplished.
One of the two edges is then placed parallel to one of the cross-
wires, an adjustment which can be accurately made if, instead of
bringing the edge and wire into complete coincidence, the edge is
placed slightly to the side of the wire.
The position of the stage is then read, and afterward rotated
until the second edge is brought into the position which the first
had occupied. This angle, through which the objective-stage was
turned, is, of course, equal to the plane angle to be measured.
If the measurements are to be made on larger crystals, then the
least possible magnification should be used. 164
CRYSTAL MEASUREMENTS.
See Groth, Phys. Krystall., p. 551, 1885, on the significance of
the measurement of plane angles.
(t>) Testing for Double Refraction and Determination of
the Directions of Vibration in Crystals.
The polarizer, analyzer, and cross-wires are given the positions
as outlined on page 163. The Nicols are then crossed and the
field of view becomes dark.
With this adjustment of the instrument, the objective-table with
the object is turned through 360° ; if, then, the substance is amor-
phous, or belongs to the regular system, the field of view will
remain dark during the rotation of the object. If, on the other
hand, a doubly refracting uni-axial or bi-axial crystal is examined,
the uniform darkness for all positions of the stage is observed only
for certain few positions of the object—namely, only when the two
parallel faces, natural or artificial, of the crystal are perpendicular
to the optic axis (or to an optic axis).
On the contrary, for all other positions of a doubly refracting
crystal, and therefore in general, the field of view during the rota-
tion of the stage through 360° is dark only in four different posi-
tions, which are go° apart; in the intermediate positions the field
appears colored (Groth, Physik. Krystall., pp. 71 and 105, 1885).
If the crystal shows only a slight double refraction, the change
of intensity between the darkness and the light is very slight, and
it is necessary in such cases to use the Biot quartz-plate (p. 163),
which can be shoved into the instrument.
For special exceptions with reference to the above phenomena,
see Groth, Physik. Krystall., p. 650, 1885.
If these four positions, for which the plate is dark, have been
determined for a doubly refracting crystal which appears colored
between crossed Nicols, they represent those positions for which
the plane of vibration of one of the two rays in the crystal is
parallel to the plane of polarization of the one Nicol. If the
direction of the planes of polarization of the three Nicols is given
by the position of the cross-wires (p. 163), then the angles which
the planes of vibration of the two rays in the crystal plate form
with the crystal edges is easily determined. It is only necessary to
place a crystal edge parallel to one of the cross-wires (p. 163) and MICROSCOPE WITH POLARIZING ATTACHMENTS.
165
to determine with crossed Nicols, by rotating the stage, that posi-
tion which causes darkness in the field of view. A second reading
of the divisions on the stage gives directly the angle which the
planes of vibration form with the crystal edge. With mono-
chromatic light, the observation will be sufficiently accurate for
chemical purposes if, instead of determining the position of maxi-
mum darkness, the arithmetric mean is taken of two positions
which appear equally removed from this maximum. The determi-
nations should be repeated several times, and the crystal should be
carefully examined at the end of each series of observations, to deter-
mine whether the crystal edge still remains in the proper position.*
The determination of the vibration-planes is one of the most
important measurements in crystallography, and is of itself suffi-
cient in many cases to enable one to distinguish between the crys-
tal forms which come into consideration. It is especially necessary
to determine whether the vibration-planes form angles with certain
crystal edges (inclined extinction), or whether they are parallel to
the same (parallel extinction).
The latter case never occurs in the asymmetric system; in the
monosymmetric system the parallel extinction occurs only for cer-
tain sections of the crystal; while in the orthorhombic system
extinction occurs parallel or perpendicular to each of the three
crystallographic axes, in the hexagonal and tetragonal systems par-
allel and perpendicular to the principal axis.f
Substances for investigation : Alum and sodium chlorate (regu-
lar) ; potassium ferrocyanide (tetragonal); iodoform and sodium
nitrate (hexagonal) ; potassium chlorate and ammonium sulphate
(orthorhombic) ; ferrous chloride and ferrous sulphate (monosym-
metric); copper sulphate and potassium bichromate (asymmetric).
The microscope represented in figure 64, page 161, can be used for
investigations not only in parallel but also in convergent polarized
light. %
(c) Investigations in Convergent Light.
* Groth, Physik. Krystall., p. 651, 1885.
f O. Lehmann, Krystallanalyse, Leipzig, 1891, pp. 33 and 34.
I Groth, Physik. Krystall., p. 69, 1885. 166
CRYSTAL MEASUREMENTS.
In order to change from measurements in parallel light to
measurements in convergent light it is sufficient, in general, to
remove the eye-piece and use a higher-power objective; then
the characteristic interference figure will be visible instead of the
crystal.
The change from one kind of light to the other is still more
convenient if a Bertrand lens (an achromatic lens of 3-4 cm.
focal length) is attached to the microscope. The removal of
the eye-piece is then unnecessary, and it is sufficient for ob-
servations in convergent light to place this lens in the open-
ing above the objective (microscope of Fuess, Berlin, Stall-
schreiberstr., Yoigt and Hochgesang, Gottingen).
When a plate of a tetragonal or
hexagonal crystal, cut perpendicu-
lar to the optic axis, is observed
in convergent polarized light with
crossed Nicols, a dark cross with
a system of colored rings, the in-
terference figure represented in
figure 67 is seen. This charac-
teristic interference figure (see
theory of Groth, Phys. Krystall.,
p. 75, 1885) is elliptical in shape
when the surfaces of the crystal
section are inclined to the optic
axis.
Fig. 67.
If, on the other hand, a section of a bi-axial crystal (orthorhom-
bic, monosymmetric, or asymmetric), cut perpendicular to the line
bisecting the optic axes, is observed, the interference figure ap-
pears as represented in figures 68 and 69. The figure has the appear-
ance of figure 68 when the section is placed between crossed
Nicols, so that the plane of its optic axes is parallel to the plane
of polarization of one of the Nicols. Figure 68 a(a black cross
with colored lemniscates) is the form shown by thick crystal-plates,
while the form figure 68 b (a black cross with elliptical rings) is
characteristic of thin plates. If the section between the crossed
Nicols is turned so that the plane of the optic axes forms an angle
of 450 with the plane of polarization of the Nicols, then the form MICROSCOPE WITH POLARIZING ATTACHMENTS.
167
of the figure changes and takes on the appearance of figure 69,
thick plates showing the form 69 a and thin plates the form 69 b.
The principal difference between uni-axial and bi-axial crystals
consists in the fact that the interference figure for the former re-
mains closed on rotating the objective, while for the latter it opens
Fig. 68.
and divides into two hyperbolas. For details of these phenomena,
see Groth, Physik. Krystall., p. 104, 1885.
Determination of the angle between the optic axes, see Groth,
Physik. Krystall., p. 115, 1885; distinction between the positive
and negative character of a doubly refracting crystal, I. c., p. 122.
Stauroscopic measurements, ibid. p. 618. Cutting, grinding,
and polishing crystals, ibid. p. 667.
Fig. 69
Isomorphism, Retgers, Zeit. phys. Krystall. 3, p. 497, 1889;
ibid., earlier literature; the same Zeitschr. 4, pp. 189 and 593,
1889; 6, p. 193, 1890; 8, p. 7, 1891; 9, pp. 266 and 386; and
10, p. 529, 1892 ; Krister, Zeit. phys. Chem. 5, p. 601, 1890, and
8, p- 577, 1891 ; Muthmann, Zeit. f. Krystall. 19, p. 357, 1891. REFRACTIVE INDEX.
CRYSTAL MEASUREMENTS IN GENERAL.
When a chemist wishes to obtain measurements of a crystal he
usually seeks the assistance of a crystallographer. In most chemical
investigations the measurement of crystals is entirely omitted and
the crystal form referred to only in a general way.
In fact, the more accurate goniometric and stauroscopic measure-
ments require more practice than most chemists have had. On the
other hand, it is advantageous for the chemist to be able to under-
take, for simple crystal forms, the measurement of the most important
angles (with a Wollaston goniometer), as well as the surface angle
under the microscope, also the determination of the vibration
planes, and even to make observations in convergent polarized light.
These simpler measurements offer no great difficulty to a chemist
who understands the principles of crystallography. These measure-
ments become all the more necessary in recent times, owing to the
importance of crystal form in the domain of stereochemistry, as
well as for deciding problems of isomerism in general.
XVII. REFRACTIVE INDEX.
i. THE REFRACTOMETER OF ABBE.*
Principle, Method, and Apparatus (Fig. 70).—The light
reflected from the mirror g passes through the glass parallelepiped
C, which consists of a specially formed combination-prism (Fig.
71), into the cross-wire tube J O.
The telescope is fastened to the divided sector A, and the double
prism C with the arm B, so that the position of the prism, with ref-
erence to the axis of the telescope, can be changed. The telescope
can also be moved by means of the screw K and fastened in the
desired position.
* Abbe, Apparatus for Determining Refraction, Jena, 1874, and Sitzungs-Berichte
d. Jenaischen Gesellsch. f. Medic, u. Nat., Febr. 21, 1879. 169
REFRACTOMETER OF ABBE.
If a liquid (or a suitable substance of smaller refractive index than
the glass) is placed between the prisms, then the light which enters
the prisms will, for a definite position of the prism, be totally
reflected at the surface of the liquid and glass, and will no longer
enter the telescope in parallel rays. The field of view of the tele-
scope will then appear more or less darkened, depending upon the
Fig. 70.
position of the prism. For a definite adjustment of the prism one-
half of the field of view will appear bright and the other half dark.
For this position the refraction due to the liquid can be calculated
from the angle of total reflection and the index of refraction of the
prism by a simple formula.*
* Loc. cit, Abbe, Apparatus, etc., p. 44. 170
REFRACTIVE INDEX.
To shorten the calculation, the divisions of the sector A are
experimentally chosen, so that the index of refraction of the liquid
for sodium light can be read off directly from the scale.
In many cases white light is employed. The fact that the differ-
ent colors do not experience total reflection simultaneously must
then be taken into account. The dividing line between the light
and dark portions of the field of view appears colored for white light.
This dispersion can be corrected by means of the compensator D.
This compensator consists of a direct-vision prism arrangement
(p. 182), the two parts of which can be rotated in opposite direc-
tions by means of the screw t. The adjustment is so made that
the rays of sodium light experience no divergence.* The influ-
ence of dispersion is eliminated for certain
positions of the screw t, which are read off
on the scale c. The dividing line between
the dark and light portions of the field of
view then appears sharp and uncolored.
The scale c serves for the simultaneous
measurement of the dispersion.
Method of Operation.—The apparatus
is turned by means of the knob K until the
sector at e comes in contact with the experi-
ment-table. With the instrument in this
position, the movable prism is carefully re-
moved by pressing down the spring (Fig. 71); the prism surfaces
are cleaned (with alcohol, water, etc.), and, after placing a narrow
piece of thin paper on the short side, a drop of the liquid to be in-
vestigated is brought onto the hypothenuse-surface of the fastened
prism.
Fig- 7I-
The movable prism is then replaced and the telescope so adjusted
that the arm B stands at the first division of the scale. The mir-
ror is then turned toward the window or some artificial light, so
that the whole field of view of the telescope appears light. The
arm is then moved on the scale until the lower half of the field of
view appears dark. Usually, a broad, colored border appears at the
dividing line between the dark and light portions.
*Abbe, Apparatus, etc., /, c., p. 50. REB’RACTOMETER OF ABBE.
On turning the screw t, the colored border disappears, and the
colorless dividing-line between the dark and light portions is then
brought as sharply as possible onto the cross-wires by means of the
arm B. The positions of the arm and compensator are read off;
the screw t is then turned until the dividing-line at the middle of
the cross-wires appears colorless a second time, the arm is read-
justed, and the positions of the arm and compensator again read off.
The mean value of the two positions of the arm give directly the
refractive index for the sodium line D. Inasmuch as the scale is
graduated to thousandths for refractive indices, the results can be
estimated, by means of a microscope, to the fourth decimal place.
The dispersion* between the Fraunhofer lines D and Fcan be
calculated from the two positions of the compensator by means of
a table which usually accompanies the apparatus.
Inasmuch as the refractive index nD and the dispersion np nD
are known, the refractive index for any wave-length can easily be
calculated from the Cauchy formula (p. 176). However, a knowl-
edge of the refractive index for sodium light is usually sufficient.
The apparatus can also be used for determining the index of
refraction of solids.
A thin, polished plate of the substance, together with a drop of
a chemically indifferent, highly-refractive liquid, is placed between
the prisms.
The following highly-refractive liquids are well adapted to these
measurements; Oil of cassia (n=i.6o), cinnamic aldehyde
{n— 1.62), sulphur chloride (n— 1.654), selenium chloride (n =
r.653), phenyl-sulphide (//= 1.623), phosphorus bromide {n
1.68), monobrom-naphthalene (;z=i.66), and arsenic bromide
(« 1.781).
The index of refraction of the liquid compared with air is first
accurately determined, then the refractive index of the liquid com-
pared with the solid is determined in the manner described above.
The first value divided by the second gives directly the index of
refraction of the solid compared with air.
To test the accuracy of the instrument it is sufficient to make a
series of observations with a substance of known refractive index,
* Abbe, Apparatus, etc., pp. 48 and 75. 172
REFRACTIVE INDEX.
with white and also with sodium light. Any necessary correction
should be applied to the readings on the scale.
The following are refractive indices for sodium light:
Water at 200 = 1.3329 (at 150 = 1-3333)
Alcohol “ = 1.3623 (sp. gr. 20°/4° = 0.8000)
Acetone “ = X.3591 ( “ “ = 0.7920)
Ethylidene chloride “ = 1.4165 ( “ “ X.1743)
Anilin “ 1.5863 ( “ “ = 1.0216)
Acetic acid “ = 1.3718 ( “ “ = 1.0495)
Benzene “ = 1.5863 ( “ “ = 0.8799)
Toluene “ = 1-4955 ( “ “ = 0.8656)
For other refractive indices see, among others, Tabellen von
Landolt-Bornstein, pp. 205-220, 1883, and Conrady, Zeit. phys.
Chem. 3, p. 216, 1889 ; Die Brechungsindices des Wassers, Briihl,
Ber. d. d. chem. Ges. 24, p. 644, 1891.
2. THE REFRACTOMETER OF PULFRICH.
Apparatus and Method in General.—A right-angled prism
is placed in the upper part of a three-cornered support, fastened to
the foot of the apparatus (Fig. 72). The horizontal and vertical
surfaces of the prism form the above angle. The third inner
prism stands inclined and is perfectly smooth.
The outer portion of the horizontal prism surface is slightly con-
cave ; it forms the base of a glass cylinder, which is fastened to the
prism by means of cement. This cylinder is filled with the liquid
to be investigated, and is provided with a small thermometer.
If the rays of light are brought together at the lower edge of the
glass prism filled with liquid, by means of a lens fastened to the
foot of the apparatus (not represented in the figure), then the
light will pass from the liquid into the upper surface of the prism,
and leave the prism through the vertical surface, provided the angle
formed with the normal to the surface is less than the limiting
angle of total reflection.
The telescope, provided with cross-wires and situated opposite
the vertical prism surface (as shown in the figure), is fastened to
a graduated circle with which it rotates. The beginning of the
total reflection may be observed by adjusting the telescope so that,
the field of view appears dark in one portion and light in another. REFRACTOMETER OF PULFRICH.
173
The position of the telescope is determined, for which one-half
of the field of view is light and the other half dark. The refrac-
tive index of the liquid can be calculated by a simple formula
(p. 176) from the angle through which the divided circle rotates
in passing from the zero of the
scale to the required position.
Apparatus and Method
in Detail.—The hollow, three-
cornered support, in the upper
part of which the prism is fast-
ened, slides down over a three-
cornered solid support, which
is fastened to the foot of the
apparatus.
Inasmuch as the relative posi-
tions of the prism surfaces and
the divided circle or telescope
must always be the same, the
inner and outer supports must
be so constructed that the prism
will remain constantly in its
position.
The pressure-screw on the
support should be tightened be-
fore each experiment; and care
should be taken that, on remov-
ing the hollow support from the
apparatus, no dirt or dust col-
lects in the space between the
outer and inner supports. The
removal of the hollow support
is, therefore, avoided as much
as possible, and the glass cylin-
der which contains the liquid is usually cleaned by means of a
pipet.
Fig. 72.
This cylinder is blackened on the side turned from the source of
light, and is provided with a metallic cover, in the opening of
which is placed a thermometer. REFRACTIVE INDEX.
The cement on the cylinder (resin cement, gum arabic) must be
frequently renewed. This must be done with the utmost care and
cleanliness, as the rays of light enter the prism just' above the
cement.* If the liquid should ooze through the cement during
the experiment, it should be removed by means of filter paper; the
vertical surface of the prism should also be kept clean.
The telescope and divided circle are firmly fastened together.
The telescope is adjusted for parallel rays of light, and is provided
with cross-wires. The observer has only to focus the eye-piece
sharply on the cross-wires, avoiding at the same time any rotation
of the wires.
The zero point of the telescope is the horizontal position,
which is fixed by the zero points of the divided circle and the
vernier.
After the telescope has been approximately adjusted, the screw
below the divided circle is firmly clamped, and the final adjustment
made by means of the more delicate side-screw.
The circle is graduated to 0.50. By means of the vernier,
it is possible to read the scale to one minute.
Sodium light (sodium chloride, sodium bromide) is usually em-
ployed as the source of light. Thallium light and lithium light
may also be used. The light should be as intense as possible, and
should last for as long a period as possible. For contrivance see
pages 185 and 207.
The prism which accompanies the instrument will answer for the
investigation of most liquids. A prism of higher refractive index
is necessary only for liquids whose refractive indices are greater
than 1.6. Upon request, this extra prism will be furnished with
the instrument.
Method of Operation.—The determination is carried out in
an entirely or partially darkened room. The glass cylinder is
filled with the liquid to be investigated and the screw on the
support firmly tightened.
* The glass cylinder in the more modern form of apparatus is provided around
the interior of the lower end with a right-angled shoulder, which fits down over
a corresponding shoulder on the prism-support. The cement is placed only
between the vertical portions of these shoulders, thus leaving the base of the
cylinder where the light enters perfectly clear. REFRACTOMETER OF PULFRICH.
175
The source of light is placed at a distance of about y2 of a meter
from the apparatus, so that the rays of light are brought together
at the lower edge of the glass cylinder by means of the lens.
When the adjustment is correct, a sharp, inverted image of the
flame, in a darkened room, will be visible on a piece of white
paper held in front of the cylinder. This image should be some-
what above the upper surface of the prism, toward the middle of
the cylinder, as this is most suitable for the entrance of light into
the prism.
When the observer is satisfied that the cemented portion is suffi-
ciently tight and the glass surfaces clean, the telescope is so adjusted
that the field of view is divided exactly in the middle, the upper
portion being dark and the lower portion light. The angle through
which the telescope has been turned from the zero point (horizon-
tal position) is then read off on the divided circle (to one minute).
The index of refraction is calculated, according to page 176,
from this angle /, which the last "ray that enters the prism forms
with the vertical surface of the prism on passing out.
The dividing line between the light and dark portions of the
field of view should be as sharp as possible. If this is not the
case, the intensity of the light is too low, or the position of the
flame with reference to the apparatus is not properly adjusted, or
the prism surfaces are not clean, or, lastly, the cementing has not
been neatly done.
Enough liquid to cover the bottom of the cylinder is sufficient
for the determination ; the cylinder, however, must be carefully
cleaned, either with the help of a pipette or by removing the sup-
port B (p. 173)-
The temperature must be noted for each determination. In
order to determine approximately the connection between the
refractive index and the temperature, the liquid should be warmed
before pouring into the cylinder; then, by repeated simultaneous
observations of the temperature and refraction, the relation between
the two can be established. See also page 178.
The time required for an observation amounts to only a few
minutes. The different readings on the divided circle should not
vary more than than 0.5 to one minute; this in general will give
the refractive index accurate to within one unit in the fourth deci- REFRACTIVE INDEX.
mal place, an accuracy which is sufficient for most chemical pur-
poses.
To ascertain whether the instrument has undergone any change
after long use, experiments are made with liquids of known refrac-
tive indices. See table, page 172.
It is better to carry out an experiment with water before each
series of determinations.
Calculation of the Refractive Index n.—lf i is the
observed angle on the divided circle, and iV'the refractive index of
the glass compared with air, then the index of refraction of the
liquid compared with air is:
n '\liV2 sin 2 i*
If the refractive index is to be reduced to the vacuum standard,
n must be multiplied by the refractive index of air (at o° and 760
mm.) = 1.00027. This reduction, however, is frequently omitted.
The values of N and n depend upon the wave-length of the
light used in the experiment.
The values of N for the sodium, thallium, and lithium flames are :
N
Na = 1.61511
T1 = 1.62043
Li = 1.60949.
Sodium light is usually employed. As a matter of convenience,
the refractive indices n, which correspond to the different values of
i for sodium light, have been arranged in the form of a table (Sec.
xxi). The results are given for angles which differ 10' in magni-
tude ; the intermediate values can easily be calculated by means of
the differences d.
Sometimes it is necessary to calculate the refractive index of a
substance for light of a definite wave-length to light of a different
wave-length.
This calculation can usually be made very closely by means of
the Cauchy formula f :
"* = A + f,.’
* For the development, see Ostwald, Lehrb. allgem. Chem., 2. Aufl., Bd.
p. 406, 1891.
f Briihl, Zeit. phys. Chem. I, p. 308, 1887. REFRACTOMETER OF PULFRICH.
177
nis the refractive index for light of wave-length X; A and B are
two constants, the values of which can be determined if the refrac-
tive indices and n2 for the wave-lengths Xt and X 2 are known.
The formulas are:
HX2 « 2
A . A 1 7l(l a 2
2 2
A 1 A 2
and
B [nx A) V.
If the values thus obtained for A and B are substituted in the
equation
D
n\ ■=. A 2
the refractive index nK can be calculated for any light of known
wave-length.
The wave-lengths X (in millionths of a millimeter) for the differ-
ent kinds of light usually employed are ;
Potassium (red line) =r 768.0
Sodium (yellow line) = 589.3
Lithium (red line) = 670.8
Thallium (green line) = 534-9
Hydrogen (red line) Ha = 656.3
Hydrogen (green line) H(3 = 486.1
Hydrogen (violet line) Hv = 434.0.
Choice of Method for Determining the Refractive Index.
—The apparatus of Abbe or Pulfrich is usually employed for chem-
ical purposes. These methods are both accurate to from one to two
units in the fourth decimal place. Both methods are extremely
simple ; especially the method of Abbe, owing to the small quan-
tity of liquid required.
The uncertainty of the temperature is an objection to the method
of Abbe. The method of Pulfrich has the disadvantage that tthe
cylinder must be frequently cemented to the prism.
If the refractive index is to be determined accurately to the fifth
decimal place, a good spectrometer, with horizontal divided-circle,
must be employed. Wiedemann and Ebert, Physik. Prakt., p. 255,
1890) Kohlrausch, Prakt. Phys. vn, p. 146, 1892; Glazebrook
and Shaw, Physik. Prakt., Leipzig, p. 287, 1891.
Determination of refractive indices at higher temperatures, Bruhl,
Ber. d. d. chem. Ges. 24, p. 286, 1891. 178
REFRACTIVE INDEX.
Specific Refraction, Atomic and Molecular Refraction.
—The determination of the refractive index and its relation to
temperature is not of itself sufficient for chemical problems.
There are definite relations between the refractive index n and the
density d determined at the same temperature. These relations are
independent of the temperature. Such relations which are of im-
portance in the development of chemical laws are shown by the
expressions :
n X n2 —II
,— and
d n2 ~f- 2 d
These expressions are known as the “specific refraction,” or
simply the “refraction constant.” The second Lorentz-Lorenz
id formula, for practical and theoretical reasons,* is used almost
exclusively.
The refraction constant is further multiplied by the atomic or
molecular weight, for the development of stochiometric laws.
The expression
112 I a
n2 -f- 2 d
is called the atomic refraction, and the expression
«2 1 m
n2 2 d
the molecular refraction.
For the calculations, see Table of Atomic Weights, page 229, and
also the table on page 235, which gives
«2 I
'°gW+-2
for the different values of n. The molecular refraction is calculated
to the second decimal place.
* Briihl, Ber. d. d. chem. Ges. 19, p. 2746, 18S6; Liebig’s Ann. 235, p. 1, 1886;
and Zeit. phys. Chem. I, p. 310, 1887 ; 7, p. 1, 1891 ; Weegmann, Zeit. phys.
Chem. 2, pp. 219 and 258, 1888; Schiitt, ibid. 5, p. 348, 1890. APPLICATION OF REFRACTIVE INDICES.
179
APPLICATION OF REFRACTIVE INDICES TO
. CHEMICAL PROBLEMS.
1. The refractive index may be used to determine the degree of
parity of a substance; it is also frequently used in technical work
for the identification of substances.
For tables of refractive indices see, among others, Landolt-Born-
stein, Phys. chem.. Tab., pp. 204-220, 1883; Kanonnikoff, Jour,
pr. Chem. [2] 32, p. 497, 1885 ; Briihl, Zeit. phys. Chem. x. p.
312, 1887 ; 7, pp. 25 and 159, 1891; Jahn, Wied. Ann. 43,
p. 280, 1891 ; Conrady, Zeit. phys. Chem. 3, pp. 216 and 223,
1889.
2. The refractive index can often be advantageously employed to
determine the concentration of a solution or mixture.
If 100 parts of a mixture of a solution contain p parts of the one,
and therefore 100 p parts of the other constituent, and n and d
represent the refractive index and density of the mixture (solu-
tion), nv n.2, and dv d 2 the corresponding values for the two con-
stituents of the mixture, we have the following equations :
n i «, x , «„ I
s~.100 = -t—p +
and
«2 I 100 I p «22 I 100 p
«2 -f- 2 d «J2 -f- 2d} «22 -j- 2 d 2
If, therefore, the refractive indices for a number of concentra-
tions are known, or if the refraction constants of a solution and
those of its constituents are known, then the concentration can be
approximately determined from one of these two formulas. On
the other hand, the refraction constant of a liquid or solid can be
approximately calculated from the refraction values of their solu-
tions or mixtures of known concentrations. As to the degree of
accuracy, see the work of Schiitt, Zeit. phys. Chem. 5, p. 349,
1890, and 9, p. 349, 1892, and the bibliography in the same
Zeitschr. 5, p. 349.
3. The refraction constants (atomic and molecular refractions)
are of considerable value in the determination of the constitution of
organic compounds. REFRACTIVE INDEX.
The molecular refraction of a compound is equal to the sum of
its atomic refractions. *
If m is the molecular weight of a substance, the molecule of
which consists of p, q, r . . ~ atoms of the elements whose atomic
weights are av a 2, a3 . . ~ and n and d are the refractive index
and density of the substance, and nv n2, n3 . . . and dv dv dz . . .
the corresponding values for the elementary atoms contained in the
body, then
n2 I m n-.2 X a, n„2 I a,, «,2 I a* ,
= i- 4- n -L jl. r -2 4-
n2 -j- 2 d r nx2 2dx J «22 -f- 2d2 nz2 2d3
The atomic refractions of most elements are known. The
molecular refraction of a compound, then, can be (1) determined
directly; (2) calculated from the sum of the atomic refractions.
The observed and calculated values should agree. This is usually,
but not always, the case. Frequently the influence of the consti-
tution of the compound must be taken into account.
* The Landolt-Briihl theory may be formulated as follows:
I. Position isomerides have equal specific and molecular refractions ; saturation
isomerides have different refraction constants.
2. Polymers never show equal specific refractions nor multiple molecular re-
fractions corresponding to the molecular weights.
3. A change of complex atomic groups to simpler groups is always accom-
panied by a decrease in the refraction.
4. The optical effect of building up a more complex substance is the same,
whether an open-chain compound (amylene, diamylene) or a closed-ring com-
pound (paraldehyde, cymhydrene, menthol, etc.) or compounds with several
rings (pinene, cyneol) result.
5. The molecular refraction of truly saturated bodies is approximately equal
to the sum of the atomic refraction calculated from the empirical formula. All
those compounds which exhibit' only single-linking of atoms may be considered
saturated; these represent the true paraffins or derivatives of the general formula
(C„H2n+2)-xH2.
6. All unsaturated compounds show a refractive increment which is approxi-
mately proportional to the number of ethylene, acetylene, or carbonyl groupings.
The less the dispersive power of the substance, the more nearly this proportion-
ality holds true.
See Briihl, Zeit. phys. Chem. I, p. 340, 1887, and ibid. 7, p. 189, 1891, and
Weegmann, ibid. 2, pp. 222 and 369, 1888. On the influence of dispersion, see
Briihl, Liebig’s Ann. 235, 1, and Ber. d. d. chem. Ges. 19, p. 2746, 1886. APPLICATION OF REFRACTIVE INDICES.
181
If a compound containing C, H, O is investigated, then the
influence of the single, double, and triple linking of carbon atoms
on the refraction must be taken into account. The sum of the
*
atomic refractions must be increased by a “ refraction increment ”
= 1.7 units (for sodium light) for each double bond between two
carbon atoms. The atomic refraction of carbon, when singly
linked to oxygen, is also different from that when it is doubly
linked, and these values are less than for carbon atoms bound
together with one or two bonds. (See table below.)
If, therefore, the molecular refraction calculated on the assump-
tion of single linkings is less than the observed value, it indicates,
when the manner in which the oxygen is linked does not come
into consideration, the presence of double bonds between carbon
atoms. The number of double bonds may be found by dividing
the difference between the observed and calculated values by x.7.
The following table contains some of the most important atomic
refractions, calculated from the rf formula of Conrady,* Bruhl,-j-
-and Landolt for sodium light and the C-line of hydrogen.
|= represents the double linking; |= the triple of carbon;
C' represents a carbon atom in the middle of a chain of carbon
atoms; C° a single carbon atom; O' hydroxyl-oxygen; O" car-
bonyl-oxygen ; O2 ether-oxygen; and N' a nitrogen atom singly
linked to carbon.
Atomic
Weight.
Atomic
Refrac-
tion for
Sodium
Light.
Approximate
Atomic
Weight.
Atomic Re-
fraction for
Sodium Light.
Conrady.
Atomic Refraction
FOR THE C-LINE.
Landolt.
Bruhl.
1.707
I.707
1.78
1.836
1=
2.22
C'
II.97
2.494
12
2.501
2.48
2-365
c°
II.97
2.586
12
2.592
2.48
H
I
I.051
X
I.OSI
1.04
1.103
O'
15.96
I-5I7
l6
1.521
1.58
I. 506
O"
15.96
2.281
l6
2.287
2.34
2.328
O2
15.96
1.679
l6
1.683
1.58
1-655
N'
14
2.76
Cl
35-37
5-976
35-5
5-998
6.02
6.014
Br
79.76
8.900
80
8.927
8.95
8.863
I
126.54
14.12
126.5
14.12
13-99
13.808
* Conrady, Zeitschr. phys. Chem. 3, p. 226,1889. Bruhl, ibid. 7, p. 19X, 1891. SPECTRUM ANALYSIS.
The difference between certain of these values is rather small.
C' and C° differ very slightly, the difference between O' and O2
being somewhat larger.
On the relations for nitrogen, see Lowenherz, Zeit. phys. Chem. 6, p 552,
1890; Briihl, Zeit. phys. Chem. 7, p. 176, 1891, and Ber d. d. chem. Ges. 26,
p. 806, 1893; Trapesonzjanz, Ber. d. d. chem. Ges. 26, p. 1428, 1893; for sul-
phur: E. Wiedemann, Wied. Ann. 17, p. 577, 1882; Nasini, Gazz. Chim. Ital.
13, p. 296, 1883, and Rend. Lincei 2, p. 623, 1886; 6, pp. 259 and 284, 1890 ;
Nasini and Costa, Verdfifentl. chem. Instit. Rom, Ref. Zeit. phys. Chem. 9, p.
639, 1892.
On the relation of refraction to the constitution of compounds, influence of the
double bond, etc., see Briihl, Ber. d. d. chem. Ges. 12, p. 2135, 1879, and 19, p.
3103, 1886; Liebig’s Ann. 200, p. 139, 1880; Zeit. phys. Chem. I, p. 311,
1887 ; Wallach, Liebig’s Ann. 245, p. 19X, 1888.
Kanonnikoff, Jour. pr. Chem. (2) 32, p. 497, 1885 ; Weegmann, Zeit. phys.
Chem. 2, p. 229, 1888; Landolt and Jahn, molecular refraction and dielectric
constant, Zeit. phys. Chem. 10, p. 289, 1892; refraction of gases, Briihl, Zeit.
phys. Chem. 7, p. 1, 1891.
Determination of dispersion: Briihl, Zeit. phys. Chem. X, p. 357, 1887, and 7,
p. 140, 1891, ibid, literature; Nasini, Roma. Accad. d. Lincei Rendiconti feb-
brajo, 1887 ; Weegmann, Zeit. phys. Chem. 2, p. 235, 1888; Barbier and Roux,
Compt. rend. IX2, p. 582, 1891 ; Gladstone, Jour. Chem. Soc. 59, pp. 290 and
589, 1891.
XVIII. SPECTRUM ANALYSIS.*
1. THE DIRECT-VISION SPECTROSCOPE.
Many elements and compounds which give characteristic emis-
sion or absorption spectra may be recognized by means of the
small apparatus represented in figure 73.
Two brass tubes, movable one in the other, contain a combina-
tion of crown and flint-glass prisms which cause the dispersion of
* For the theoretical consideration of spectrum phenomena see, among others,
Kayser, Lehrbuch der Spectralanalyse, and H. W. Vogel, Praktische Spec-
tralanalyse. SPECTROSCOPE OF BUNSEN.
the light that passes through. The rays of light enter through the
slit i-, and pass through the lens c and the prism combination into
the eye-piece 0.
Fig. 73.
The instrument is adjusted by means of the sun spectrum. The
inner tube is moved to such a position in the outer tube that the
Fraunhofer lines of the sun spectrum appear sharp.
2. THE SPECTROSCOPE OF BUNSEN.
Apparatus (Fig. 74).—This consists, in its essential parts, of a
collimator A, through which the light enters, the observing-tube
B, the scale-tube C, and the prism P.
Fig. 74.
The collimator is so adjusted that the rays of light which enter the
slit in the plate f fall parallel on the prism F, by means of which they
are dispersed ; the image of the spectrum is formed in the telescope B. 184
SPECTRUM ANALYSIS.
The image of the micrometer scale in the tube C is also visible
just above the image of the spectrum. By means of this the rela-
tive positions of the different portions of the spectrum can be
determined.
Adjustment of the Apparatus.—lt is, above all, necessary
that the rays of light leave the collimator in a parallel direction, and
that the image of the slit appears distinct in the telescope. To
accomplish this the eye-piece of the telescope is adjusted so that
the cross-wires appear sharp. The telescope is then removed from
its support and focused sharply on some distant object (church
steeple, tree, etc.). By means of a mark this adjustment of the
telescope for parallel rays is fixed once for all.
The prism is then removed and the telescope placed directly
opposite the collimator A. The slit is illuminated and its position
adjusted so that the slit and cross-wires appear sharp at the same
time, and so that no parallax is produced on moving the eye. By
raising or lowering the telescope the middle of the slit can be
made to coincide with the middle of the cross-wires.
If the prism has not already been adjusted to the position of
minimum deviation, it may be so adjusted in the following
manner :
The slit is illuminated with sodium light, the prism is given a
chance position, the direction of the outgoing rays determined by
means of the naked eye, and the telescope turned so that the
sodium line coincides with the cross-wire. The prism is then turned
in the direction of the refracting edge, the telescope being moved
at the same time. This rotation is continued until the image of the
slit begins to move in the opposite direction. This position of the
prism, for which the change in direction begins, is the position of
minimum deviation. The prism should be fixed in this position.
Finally, it is necessary that the image of the scale should be dis-
tinct in the telescope.
The scale-tube is illuminated by means of a small flame, which
should not be placed too near the tube, and given such a position
that the image of the scale is visible above the spectrum. The
scale-tube is then drawn out until the scale divisions appear sharp
in the telescope, and so that the image of the scale produces no
parallax with the image of the slit on moving the eye. The hori- SPECTROSCOPE OF BUNSEN.
zontal position of the scale is brought about by rotating the scale-
tube.
Reduction of Scale Values to Wave-lengths.—lt is es-
pecially desirable, for scientific purposes,* that the positions of the
different portions of the observed spectrum be expressed not in
terms of an arbitrary scale, but in wave-lengths of the light
employed.
The scale-tube is given such a position that the division 100 coin-
cides with the middle of the sodium lines. This coincidence is
preserved in all the movements of the telescope. The reduction of
the scale values to wave-lengths is accomplished then by means of
elementary spectra or the sun spectrum.
In the first case a series of salts, which show characteristic lines
of known wave-lengths throughout the whole range of the spectrum,
Fig. 75.
are vaporized in the Bunsen burner which illuminates the slit. The
following lines, whose positions in the spectrum are shown in figure
75, are especially adapted to this purpose ;
Wave-lengths in Millionths
of a Millimeter (A .io 6).
Potassium red line Ka 768
“ blue “ Kj3 404.6
Lithium red “ Lia 670.8
Sodium yellow “ Na 589.0-589.6
Thallium green “ T1 534-9
Strontium blue “ Srs 460.8
768
As a matter of convenience for introducing the substances into
the flame, the molten chlorides of the metals may be fastened, in
* For technical purposes, identification of colors, determination of concentra-
tions, etc., this calculation to wave-lengths is unnecessary. 186
SPECTRUM ANALYSIS.
the form of beads, on platinum wires and a number of such wires
arranged in a horizontal position, movable around a vertical axis;
or, still better, a spoon of platinum gauze (p. 205) may be em-
ployed. See also the arrangements of Pringsheim, Wied. Ann. 45,
p. 426, 1892, and Kayser, Lehrb. d. Spektralanalyse, p. 77, 1883.
If an exhausted Geissler tube be partially filled with hydrogen and
the electric spark (small induction coil with three chromic-acid
elements) passed through the tube, the four hydrogen lines Ha,
Up, Hy, and ZTS (A= 656.3, 486.1, 434.0, and 410.2), corre-
sponding to the Fraunhofer lines C, F, G, h (Fig. 75), are visible
and may be used for reducing the scale divisions to wave-lengths.
The accuracy of this reduction to wave-lengths depends upon the
number of lines observed * and their distribution in the different
portions of the spectrum.
When the scale divisions corresponding to a number of lines have
been once determined, the relation of the same to the wave-lengths
is represented graphically.
The scale divisions are laid off as abscissas, and the wave-lengths
as ordinates, on millimeter paper. It is possible, then, by means of
the curve which is determined by these points, to represent the
position of any line in wave-lengths.
A greater accuracy may be obtained by means of the sun spec-
trum.
The slit is illuminated by direct sunlight or bright clouds, and
then, according to the accuracy desired, the positions of 10, 20, or
50 characteristic Fraunhofer lines are determined. A number of
the most important of these lines are shown in figure 75. The
wave-lengths of the lines, which are not given in the previous page,
are as follows:
A-lO 6 A-10—6
Line A 760.4 Line C 517.3
“ a 718.6 “ //j 396.6
“ 687.0 “ H2 393.4
“ E 527.0
When a larger number of Fraunhofer lines are observed, refer-
ence may be made to Angstrom’s Tables; or to Kayser’s Lehrbuch
* Landolt-Bornstein, Tables of Spectrum Lines, pp. 200-203, 1883. 187
SPECTROSCOPE OF BUNSEN.
iiber Spektralanalyse ; likewise to that of G. and H. Kriiss, Kalo-
rimetrie und quantitative Spektralanalyse.
Special Rules for Spectrum Observations. Emission
and Absorption Spectra.—The chlorides are usually employed
to obtain metallic spectra. These are volatilized on a platinum
wire in the outer portion of the Bunsen flame ; difficultly volatile
oxides should be moistened with hydrochloric acid.
The observer must not be deceived by the sodium lines which
are always visible, or the faint green and blue lines which are due
to the lower part of the Bunsen flame.
For observations of very faint lines, the flame which illuminates
the scale should be removed until the cross-wire has been adjusted
to the desired line; the scale is then illuminated and the position
of the cross-wire determined.
It is also necessary that all foreign light be excluded during the
observations. The prism and the objectives of the three tubes are
therefore covered with a black cloth ; a screen of black paper is
also placed around the eye-piece of the telescope, to protect the
eye from the illuminating flame.
The spectroscope is usually provided with a comparison prism, by
means of which the lower half of the slit can be covered. By this
arrangement it is possible to determine the identity of substances
without accurate measurements.
Direct light is allowed to enter the upper half of the slit, while
light from a flame placed to one side (Fig. 74), through total
reflection, enters the lower half of the slit. The substance to be
investigated is introduced into one flame, and the comparison
substance into the other. The two spectra will appear one above
the other, and in case of identity of the two substances the lines
of the one spectrum must be the prolongations of the lines of the
other.
For qualitative observations of the absorption spectra of colored
solutions, the solution to be investigated should be placed in a
glass prism with parallel sides (Fig. 80, p. 195), between the flame
(petroleum flame) and the slit-tube. Inasmuch as the absorption
spectra depend upon the concentration of the solution, the obser-
vations are extended to solutions of different concentrations,
dilute and concentrated. The temperature and the nature of the SPECTRUM ANALYSIS.
solvent also influence the absorption. The spectroscope should be
placed in a room of almost constant temperature (about iß°) ;
then the influence of temperature for
all observations within the temper-
ature-interval 15 to 210 can be
neglected.*
The positions of maximum dark-
ness, for an absorbing substance, are
the most important absorption bands.
The positions, in wave-lengths, of
the edges of the absorption bands are
determined for solutions of different
concentrations. The greater the dilu-
tion, the narrower the bands, and the
more nearly do they coincide for dif-
ferent solutions. If the darkness of
the observed bands increases sym-
metrically about the middle position,,
then the arithmetic mean of the band
edges for very dilute solutions repre-
sents approximately the position of
maximum darkness. This position,
then, from observations on extremely
dilute solutions, can be interpolated.f
The determination of the position of
maximum darkness is especially desir-
able for the identification of sub-
stances.
Spectrum investigations in general
depend not only upon the positions-
of the lines and bands, but also on
their distinctness and dimensions; a
sketch—or better, photograph—should
therefore be made of the observed
spectrum.
Potassium.
Carbon.
Fig. 76.
* Bremer, Zeit. anorg. Chem. I, p. 112, 1892.
t Kriiss, Zeit. phys. Chem. 2, p. 314, 1888. UNIVERSAL SPECTROSCOPE OF KRUSS.
189
The sketch may be prepared as shown in figure 76. The lines and
bands are represented by black lines and shadings of equal length.
The intensity bf the spectrum lines may be indicated by the inten-
sity of the lines in the sketch; or, better, by the curve in the same
line where abscissas correspond to scale divisions or wave-lengths
and the ordinates to intensities.
On the application of photography to spectrum analysis, see
Ostwald, Zeit. phys. Chem. 9, p. 582, 1892.
3. THE UNIVERSAL SPECTROSCOPE OF
This instrument is a modification of the Bunsen-Kirchhoff ap-
paratus, and consists, as does the ordinary apparatus, of the prism,
a collimator with comparison-prism, a scale-tube, and the observing
telescope {A, B, and C, Fig. 77).
KRUSS.*
Fig. 77.
The advantages in the construction of this apparatus are:
1. The different parts of the apparatus have been adjusted as far
as possible by the manufacturer.
2. The measuring contrivance is especially accurate.
3. The instrument is provided with an arrangement on the slit-
* Reference; A. Kriiss, in Hamburg. 190
SPECTRUM ANALYSIS.
tube for quantitative measurements according to the method of
Vierordt.
The collimator A can not be adjusted ; the manufacturer has
taken special care that the slit stands exactly in the focus of the
objective and parallel to the refracting edge of the prism. The
single slit is generally used, the dopble slit being attached only for
the method of Vierordt (p. 193).
The sides of the slit are made of platinum, and the width of the
opening can be regulated and determined by means of a micrometer
screw. The slit should be narrowed until the spectrum image is as
sharp as possible. If the platinum edges of the slit are not clean,
then the spectrum will contain horizontal streaks. In such cases
the edges should be cleaned by drawing a piece of glazed paper
through the almost closed slit.
The scale-tube B is also free from adjustment. The scale is
placed in the focus of the objective, and the tube fixed so that the
middle of the sodium line* coincides with the scale division 100.
For all measurements where extreme accuracy is not required, the
scale may be used and the contrivance on the observing telescope
neglected. The scale divisions are reduced to wave-lengths, as
described on page 185.
The observing telescope Cis provided with cross-wires. The
telescope and cross-wires are adjusted by means of the special con-
trivance represented in figure 78, which is used instead of the scale
for fine measurements, especially for carrying out the method of
Vierordt.
The telescope is turned about its vertical axis by means of the
screw and measuring contrivance i\lx i\, situated directly below the
eye-piece o. The micrometer screw is provided with a graduated
head rx (100 divisions) ; the number of whole rotations can be read
directly from the contrivance lx iv
After adjusting the cross-wires, then, to a definite place in the
spectrum, it is possible to represent the relative positions in the
spectrum to four places. The first two are expressed by the
divisions on the index lx iv and the others by the screw-head ry
* The sodium line D, as is known, consists of two lines, visible when the slit is
very narrow. UNIVERSAL SPECTROSCOPE OF KRIJSS.
Inasmuch as the cross-wires can be moved by means of the
micrometer screw l 2 r2, it is necessary, before using the contrivance
lx rv to place I] r2 on the zero.
This second micrometer screw, with the contrivance /2 r2 for
moving the cross-wires, is used for fine measurements in the spec-
trum.
From the known relation between the value of these two microm-
eter screws, the results obtained by either contrivance can be
calculated into terms of the other, likewise into scale divisions, so
Fig. 78.
that it is possible to make control-measurements by three inde
pendent methods.
The contrivance r212 has still a special use. The cross-wires
move in the slide h through an opening in the eye-piece ; this slide
lies in the focal plane of the eye-piece, and is provided with the
slit k, which, for observing faint lines and for carrying out the
method of Vierordt, is used to screen the portions of the spectrum
not in use.
In case the positions in the spectrum are determined by moving
Irv then l 2rv as already mentioned, must be adjusted to o. The
cross-wires for this adjustment are in the middle of the field of SPECTRUM ANALYSIS.
view, provided the contrivance has first been shoved from right to
left as far as possible into the eye-piece. For this adjustment of
the instrument, l 2 r2 on o and the cross-wires in the middle of the
field of view, the slit kis closed. If the slide is then shoved from
left to right in the eye-piece, until the movement is again stopped
by means of a special contrivance on the instrument, the field of
view will be dark, owing to the spectrum being covered by the
closed slit, and the line of contact of the two sides of the slit will
coincide with the middle of the cross-wire. If the slit is unsym-
raetric, as in the older form of apparatus, then, on opening to a
definite width by moving l 2 r2, the left side remains stationary and
the width of the slit or the spectrum region can be read off directly
from the measuring contrivance r2 lr
In the more recent form of apparatus the slit opens symmetri-
cally on the two sides, and the light from the two edges of the
spectrum region has a mean wave-length, which was established in
the previous adjustment of the cross-wires by moving lx rv while
the width of spectrum field is determined by means of /2 r2.
The divisions on rx lx and r212 are reduced to wave-lengths accord-
ing to the method on page 185. The positions of 20 to 30
Fraunhofer lines should be determined for this purpose. The
spectrum region is then represented in wave-lengths (e.g.,
A 612.7 604.3).
The universal spectroscope is provided with two prisms: x. A
single flint-glass prism, with a refracting angle of 6o° and a mean
dispersion of A— H2 =40 30'; 2. a Rutherford prism, with a
dispersion of A H2 = 8-n°.
On account of the greater intensity of the spectrum, the first
prism should always be used for ordinary qualitative investigations
and where the determinations are to be made as quickly as possible.
The Rutherford prism is placed in the instrument only when it is
necessary to widen the range of the spectrum and attain the
greatest accuracy possible in the measurements.
The prisms are placed in a closed, light-proof cap D (Fig. 77),
and are held in the position of minimum deviation by the pressure
of a spring fastened to the lower side of the knob K. By means
of a simple contrivance the prisms can be automatically adjusted to
the position of minimum deviation for any movement of the ob-
serving telescope. SPECTROPHOTOMETER.
4. THE UNIVERSAL SPECTROSCOPE AS
SPECTROPHOTOMETER.
Method of Yierordt.*
Principle and Calculation.—The object of the photometric
measurements is to determine the amount of absorption for a
definite range of the spectrum when the light is passed through an
absorbing medium. These measurements are especially valuable in
the investigation of liquids (solutions).
The method of Yierordt depends upon the use of a double slit,
which can be fastened on the collimator of a spectroscope instead
of the single slit.
The intensity of a definite kind of light is proportional to the
width of the slit. If, therefore, the spectroscope is provided with
two slits, one directly above the other, either of which can be ad-
justed independently of the other, then two spectra in contact will
be formed, the intensities of which will be different, provided the
slits are of equal width and illuminated by lights of different inten-
sities. If, however, the widths of the slits are so adjusted that the
two spectra for any definite range are of equal intensities, then the
intensities of the two lights are proportional to the widths of the
slits. If the intensity of one light be placed =l, the intensity of
the other is obtained from the relative widths of the two slits, which
can easily be determined.
The absorption of light by a layer of liquid depends upon the
thickness of the layer. The results are referred, therefore, to
a layer of liquid 1 cm. in thickness.
The operation is usually carried out so that the light which
enters one slit has passed through a layer of the given liquid 1 ram.
in thickness, while the light from the same source, which enters the
other slit has passed through a layer of the same liquid 11 mm. in
thickness. If the slits be then adjusted so that the two resulting
spectra are of the same intensity, and the intensity of the original
light be placed = 1, then the ratio of the widths of the two slits
* Yierordt, Use of the Spectroscope for Photometry in Absorption Spectra,
Tubingen, 1873. SPECTRUM ANALYSIS.
gives directly the intensity J' of the light after passing through a
layer of the liquid i cm. in thickness.
The extinction-coefficient e is calculated from the value of J',
and may be defined as the reciprocal value of the thickness which a
substance must have in order to decrease the intensity of the light
which passes through it to jL of the original intensity, e and
J' bear to each other the simple relation that e— log. J'. For
the development of this relation, see Kruss, Kolorimetrie und Spek-
tralanalyse, p. 78, 1892, and Methoden der Analyse, p. 84, 1892.
The abbreviated table of Yierordt for the calculation of e from J’ is
given on page 233.
In the case of solutions the extinction-coefficient depends upon
the concentration c, where c represents the number of grams of
dissolved substance in 1 c.c. of solution. So nearly is this co-
efficient proportional to the concentration that the quotient
e
—A) i. e., the absorption ratio for each dissolved substance may
be regarded as constant.
In general, the intensity f , the extinction-coefficient e, and the
absorption-ratio A should be determined in different portions of
the spectrum for each concentration of solution.
Apparatus and Method of Operation,—The universal
spectroscope may be used advantageously.
The single slit is replaced by a double slit (Fig. 79) ; i. e., one
slit divided into two halves by means of a horizontal contrivance, so
that each half can be adjusted independently of the other by means
of the two fine measuring screws tx and t„. To obtain good results it
is necessary that the slits should open symmetrically on both sides.*
The width of the slit is read off in terms of the scale divisions
on the head of the measuring screw. Each rotation of the screw
corresponds to xoo divisions. The width of one slit is placed =l,
corresponding to xoo scale divisions. To produce the same inten-
sity of light for a definite color, the other slit must be 30 scale
divisions in width; then 0.3 represents the intensity J', from
which the extinction-coefficient e may be obtained directly from
the table (p. 229).
* Kruss, Kolorimetrie und-Spektralanalyse 1, p. 86, 1892. SPECTROPHOTOMETER.
195
The liquid to be investigated is placed in a vessel of the form
represented in figure 80,—a glass vessel with parallel sides, and
11 mm. ih thickness. The vessel is provided with the Schulz
Fig. 79.
glass body a, a rectangular glass prism 10 mm. in thickness. The
light, therefore, must pass through a layer of liquid i or n mm. in
thickness. In the observation the intensity of the light which
passes through a layer of the liquid i cm. in thickness is compared
with the intensity of the same light when passed
through the prism a into the lower slit. If the
upper slit is adjusted to 100 divisions in
width, and the lower slit adjusted so that the
lights are of equal intensities, then the value
of J' can be read off directly from the lower
screw-head.
The liquid in the glass vessel must be free from
air-bubbles; these can be removed by means of
a platinum wire. In case a very volatile solvent
is used, a vessel which can be closed must be
used to contain the liquid.
The vessel containing the liquid is placed on a suitable stand
directly in front of the slit (Fig. 79). The apparatus is illumi-
nated by means of an electric light, the Auer light, or a petroleum
lamp B, as shown in the figure.
Fig. 80. 196
SPECTRUM ANALYSIS.
The lamp is placed directly in line with the collimator R, about
10 cm. from the vessel containing the liquid ; the broad surface of
the flame should be parallel to the direction of the collimator.
The two halves of the slit must be equally illuminated by the
flame. The middle of the flame, therefore, must be of the same
height as the dividing line between the two halves of the slit. To
determine when this condition is fulfilled the one slit is opened 30
divisions and the other adjusted so that the intensities of the cor-
responding spectrum regions are the same.* If the lamp is prop-
erly adjusted, then the second slit must be of the same width
(= 30 divisions) as the first.
It is further necessary, when the opening of the slit is closed
slowly, that the graduated screw-head should stand at o the instant
at which all the light is extinguished. If this is not the case, the
screw-head and vernier must be adjusted to this condition.
The vessel containing the liquid must be placed directly in front
of the slit, so that the upper surface of the glass prism is horizontal
and in the same plane with the line dividing the two halves of the
slit. If this condition is not fulfilled, a broad, shadowy band
appears in the spectrum, the width of which must be reduced to a
rather heavy line by adjusting the foot-screws of the stand so that
the upper surface of the prism is horizontal. This line is finally
brought into coincidence with the dividing line of the two slits,
which is made visible by opening the slits to different widths.
This adjustment is made by regulating the height of the horizontal
surface of the prism by means of the broad screw contrivance on
the stand. See page 198 on the use of the Hiifner-Albrecht rhomb.
The scale attached to the observing telescope (p. 191) is used to
determine the exact wave-lengths of the spectrum region investi-
gated ; and the limits of a definite spectrum region are determined
by means of the eye-piece slide described on page 191.
To obtain accurate results, the method should be carried out in
that portion of the absorption spectrum where there is no sudden
change of intensity, but where the intensity increases or decreases
gradually. There is less liability to error when the slit in the eye-
* The adjustment of the two slits to equal illuminations should be made sev-
eral times. This can be more easily accomplished in the green portion of the
spectrum. SPECTROPHOTOMETER.
piece is as narrow as possible; the minimum width, however,
should not be less than 50 divisions on the micrometer screw.
Other conditions must also be observed in observations on solu-
tions : •
1. The solution must be approximately at the temperature of the
room ; in regard to the influence of temperature on the constant of
the apparatus, see page 188. A temperature difference of 4to 50
may be neglected. Care must be taken that the heat from the
source of light does not produce a greater variation than 50 (Bre-
mer, Zeit. anorg. Chem. 1, p. 112, 1892).
2. The influence of the solvent on the value of J', owing to the
absorption and reflection of light, must not be neglected.
If the glass vessel is filled with water, the upper slit must be
adjusted to a width of 90.5 divisions on the micrometer, while the
lower slit is 100 divisions in width, in order that the two intensi-
ties shall be equal. In the investigation of all aqueous solutions,
then, the upper micrometer must be placed on 90.5, and the lower
on 100, for the starting point of the measurement.
According to Kriiss, if the lower micrometer is adjusted to 100,
the upper one, for various solvents, should be adjusted as follows :
For alcohol (90 per cent.) = 95.0
For alcohol absolute = 110.0
For ether aqueous = 98.0
For ether anhydrpus = 91.5
For chloroform anhydrous = 112.0
For benzene anhydrous = X 02.5
For glacial acetic acid anhydrous = 88.0
The measurements were made within the spectrum region :
A 5x3.1 A 523.0. It is desirable, however, that the amount of
absorption be determined for each solvent, for the values may vary
from those given above.
3. It is also necessary to determine the most suitable concentra-
tion.
The best results are obtained when the concentration is so chosen
that the lower half of the slit, for adjustment to equal intensity,
must be narrowed from the division 100 to from 30 to 10 on the
micrometer; the value of J' then becomes 0.3 to o. 1. If the solu-
tion is so slightly colored that J' amounts to more than 0.3 (about SPECTRUM ANALYSIS.
0.5 or 0.6), then the accuracy may be increased by adjusting the
micrometers on 50 instead of 100, corresponding to a half turn
of the screw. The value thus obtained for J' must be multiplied
by 2.
The widths of the slits should not exceed 100 divisions; in case
the solution is too concentrated, it should be diluted, or better, a
stronger light, the Auer or electric light, should be employed.
Inasmuch as the absorption ratio A undergoes a slight
e
change in many cases, and apparently depends upon the degree of
ionization * for electrolytes (electrolytic dissociation), the value
of A must be determined for different concentrations when an
accurate study of the absorption ratio is undertaken.
Uses of the Hiifner-Albrecht Rhomb in the Method of
Vierordt.—This recently}- proposed improvement of the Vier-
ordt spectrophotometer may be appropriately considered here.
The double slit D (Fig. 81), provided with the regular microm-
eter screws ml and m 2, is fastened on the collimator S. Ais the
liquid vessel with the Schultz glass prism g, which rests on a
micrometer stand. The glass rhomb R is placed between the
liquid vessel and the double slit. The object of interposing this
body is to separate the two spectra by a sharp, fine line, and thus
avoid the disturbing influence of the rather heavy dividing line
which occurred in the preceding method (p. 196).
The rhomb must be adjusted and fastened by means of the screws
sx and s2, so that its horizontal edge next to the slit is of the same
height and in immediate contact with the dividing line between the
two slits, and so that the horizontal section of the rhomb lies in
the prolongation of the optic axis of the collimator.
The upper rays of the light 11', which pass through the layer of
liquid 11 mm. in thickness, fall upon the lower half, and the lower
rays tx t', which pass through the Schultz glass prism, fall upon the
upper half of the slit, the rays t and tx coming in contact at the
horizontal edge of the rhomb next to the slit. The rays t' and //,
which illuminate the lowest and uppermost portions of the slit,
* J. Traube, Ber. d. d. chem. Ges. 25, p. 2989, 1892.
f Kriiss, Zeit. anorg. Chem. 1, p. 122, 1892. SPECTROPHOTOMETER.
leave, on their passage through the liquid vessel, a free space sev-
eral millimeters broad, into which the upper surface of the prism g
may be shoved without producing the troublesome conditions
previously.mentioned. See Hiifner, Zeit. phys. Chem. 3, p. 563,
1889, in regard to the use of the rhomb.
Inasmuch as the upper half of the slit is illuminated by the lower
light in this method, the lower measuring screw m 2 should be placed
Fig. 81.
on 100, and the upper half of the slit (provided with the larger
screw-head is adjusted so that the intensities of the illumina-
tions are equal (pp. 196, 198, and 199).
Before the experiment is begun, the source of light must be
placed (p. 196) so that the upper and lower spectra are of equal
intensities when the slits are of equal widths. The rhomb R
should be protected from foreign light by covering it with a
cap. 200
SPECTRUM ANALYSIS.
The following results, obtained by G. Kriiss for the spectrum of
potassium permanganate, may be noted:
i c.c. of solution contains
Spectrum region 0.00025 gm. 0.000125 Sm. 0.0000625 gm. Absorption
J' e J' e J' e A
A 494.7 A 486.5 0.043 1.36654 0.230 0.63828 0.477 0-32149 0.0001909
A 486.5 A 480.9 0.076 1.17393 0.287 0.54212 0.539 0.26842 0.0002251
A 480.9 A 474.8 0.154 0.81248 0.440 0.35655 ——- 0.0003277.
The mean of all the extinction-coefficients in one spectrum
region for the different concentrations is used in the calculation of
the absorption ratio.
The polarization-spectrophotometer of Gian, and especially of
Hiifner, is used as frequently, perhaps, as the spectrophotometric
method of Vierordt. Gian, Wied. Ann. 1, p. 351, 1877 ; Hiifner,
Jour, prakt. Chem. (2) 16, p. 290, 1877 ; and Zeit. phys. Chem.
3, p. 562, 1889. On the comparison of the two methods, see G.
and H. Kriiss, Kolorimetrie und quantitative Spektralanalyse, and
Kriiss, Zeit. anorg. Chem. 1, p. 104, 1892. The disadvantage of
the polarization-spectrophotometer, owing to the greater loss of
light, may be overcome somewhat by the use of the Auer gas-light.
Application of Absorption Spectra.—The qualitative and
quantitative investigations of absorption spectra may be applied in
the following directions:
1. It is frequently possible to accurately determine the concen-
tration of colored solutions from the extinction-coefficient e and
the absorption ratio
A =L.
e
When A is known (if necessary, for several concentrations), the
concentration may be calculated from the extinction-coefficient e
by means of the formula c— Ae. See G. and H, Kriiss, Kolo-
rimetrie und Spektralanalyse, 1892.
2. Absorption-spectra are of great analytical value for identify-
ing elementary and complex substances.
On elementary spectra, see, among others, Kriiss and Nilson, Ber.
d. d. chem. Ges. 20, p. 2134, 1887 ; on the significance of the
maximum darkness for the identification of color substances, see
page 187. ROTATION OF THE PLANE OF POLARIZATION.
201
3. Absorption spectra are closely related to the constitution of
the compounds. See Kock, Wied. Ann. 32, p. 167, 1887 ; G.
Kriiss, Zeit. phys. Chem. 2, p. 312, 1888 ; ibid, earlier litera-
ture; C. Liebermann, Ber. d. d. chem. Ges. 21, p. 2527, 1888;
Hartley, Jour. Chem. Soc., p. 641, 1888; Althausse and Kriiss,
Ber. d. d. chem. Ges. 22, p. 2065, 1889; Schiitze, Zeit. phys.
Chem. 9, p. 109, 1892; Grebe, ibid. 10, p. 673, 1892; Weigle,
ibid. 11, p. 22, 1893.
4. Absorption phenomena are of special interest in the theory of
solutions. Walther, Wied. Ann. 36, p. 518, 1889; Rigollot,
Compt. rend. 112, p. 38, 1891; Knoblauch, Wied. Ann. 43.
p. 738, 1891 ; Ostwald, Zeit. phys. Chem. 9, p. 579, 1892 ;
Lellmann, Lieb. Ann. 270, p. 204, 1892.
XIX. ROTATION OF THE PLANE OF
POLARIZATION.
General.—The particles of ether in a ray of ordinary light
vibrate in different directions perpendicular to the line of propa-
gation, while in plane polarized light the particles vibrate in a
single plane. This plane is called the plane of polarization.*
Light may be polarized in various ways: very simply by allow-
ing a ray of ordinary light to pass through a Nicol prism. This
consists of a definite combination of two sections of Iceland spar
(Landolt, Optisches Drehungsvermogen, p. 3, 1879), so that
the entering ray of light is divided into two polarized rays, and
so that only the one (extraordinary) ray passes through the prism,
while the other (ordinary) ray is removed by total reflection.
If two such Nicol prisms are placed in similar positions in a
tube, the polarized ray of light which leaves the first prism will
* According to Fresnel, the particles of ether vibrate perpendicular to the plane
of polarization; the above assumption of Neumann, owing to its greater sim-
plicity, will be taken here. 202
ROTATION OF THE PLANE OF POLARIZATION.
also pass unobstructed through the second prism ; if the second
prism is rotated through an angle of xBo°, the ray will still pass
through, for the planes of polarization of the two prisms are par-
allel for this position. If, however, the second prism is rotated
through 90 or 270°, the planes of polarization of the two prisms
will be perpendicular to each other, and the light which passes
through the first prism will be completely extinguished by the
second. If the eye is placed behind the second prism, and one of
the prisms is rotated through 360°, four positions 90° apart will be
seen to be positions of maximum light and maximum darkness,
while the intermediate positions will exhibit varying degrees of
illumination.
The first .prism is called the polarizer; the second, situated next
to the eye, the analyzer.
If the polarizer and analyzer are illuminated with homogeneous
light and adjusted to the positions of maximum darkness, and a
transparent substance—a liquid in a tube—is introduced between
them, the dark field of view in many cases becomes illuminated,
and one of the prisms must be rotated through a definite angle to
again restore the maximum darkness (principle of the simple
polarimeter).
One speaks of the rotation of the plane of polarization of a
substance and of the angle of rotation, distinguishes optically
active and inactive substances, and calls the substance dextro- or
levorotatory, according to the sense of the rotation—i. e.,
according as the analyzer must be rotated to the right or left to
restore the maximum darkness (p. 208).
Specific Rotatory Power.—The rotatory power of liquids
and dissolved substances only will be considered here.
The amount of rotation of the plane of polarization depends:
1. On the nature of the substance.
2. On the number of optically active molecules, which influence
the ray of light; for homogeneous liquids, therefore, on the length of
the column and density of the liquid through which the light passes ;
for solutions, on the length of the column and the concentration.
3. On the wave-length of the light used in the observations.
4. On the temperature at which the observation is made.
5. On the nature of the solvent, in the case of solutions. ROTATION OF THE PLANE OF POLARIZATION.
203
Let a represent the angle of rotation—i. e., the angle through
which the analyzer must be rotated to the left or right to restore
the original condition, after interposing a tube filled with an opti-
cally active liquid ; let d be the density of the liquid, and I the
length of the column of liquid ; then
r -i a
W = id
is called the specific rotatory power, or the specific rotation of a
homogeneous liquid.
The specific rotatory power may be defined as that rotation of
the plane of polarization produced when the light passes through
an optically active substance 1 dm. in length, which contains
1 gm. of substance per c.c. of volume.
The molecular rotatory power represents the rotation produced by
one gram-molecule of the substance under the conditions mentioned
for the specific rotatory power.
We have then :
r ma m [«]
[m\ = ——
100 I a 100
The values are divided by 100 to avoid large numbers.
If c is the number of grams of substance contained in 100 c.c. of
a solution, the specific rotatory power for the given concentration
is calculated by the formula ;
r n 100 a
M
likewise
m a
[»] =
If p grams of substance are contained in 100 gm. of solution, and
the density of the solution is d, then the specific rotatory-
power is
_ _ zoo a
M = 1
and the molecular power is
m a
M = -[JT-
The calculations for solutions are made according to
the above formulas; however, the temperature, the concentration,
and the solvent should be considered. 204
ROTATION OF THE PLANE OF POLARIZATION.
In general, the specific rotation of a substance is in no way pro-
portional to the concentration of the solution. The value of [«],
therefore, should be calculated for different concentrations, and the
relation of the specific rotation to concentration expressed by
formulas of the form [«] = A -f- B q and [a] A -(- B q -(- C q1;
where q is the number of grams of the solvent in 100 gm. of solu-
tion, and A, B, and C are constants, the values of which can be
easily determined from three or more determinations of [a] for
different values of q. A is the true specific rotatory power of the
pure substance, for in this case q = o.
In order to determine whether the two- or three-constant formula
is to be used, [a] should be determined for widely varying con-
centrations, and the relation of [a] to q represented graphically by
placing the corresponding values in a system of coordinates
(p. 186). If the curve is a straight line, the formula [a] = A B q
should be employed ; otherwise the formula
[a] A -j- B q Cq2
is used; e.g., for tartaric acid the first formula is used ; for sodium
light it becomes [«] = 1.950 -f- 0.1303 q.
If the true specific rotatory power of the dissolved substance is
to be determined as accurately as possible, the substance should be
dissolved in an inactive solvent which permits of very high concen-
trations. The observations should be made with several solvents.
The more concentrated the solution is, the smaller are the devia-
tions in the values of [a] calculated for the given concentration
and for the pure substance. The true specific rotatory power can
not be calculated for sparingly soluble substances. It is sufficient
in such cases to establish the above interpolation-formulas which
show the dependence of the specific rotatory power on the concen-
tration.
Sodium light is usually employed in these observations; the less
intense lithium light or the too volatile thallium light are seldom
used. When lithium light is used, a red glass is placed between the
flame 'and the apparatus to hold back the yellow rays. The kind of
light used is indicated by a sub-index, thus [«] D (specific rotation
for sodium light) ; [«]u for lithium light, etc.
If the observations are to be made with light in other portions of ROTATION OF THE PLANE OF POLARIZATION.
205
the spectrum, a combination of polariscope and spectroscope is
used (Landolt, Drehungsvermogen, p. Ix 9, 1879).
The light used should be as constant as possible and of as great
an intensity as possible.
A lamp similar to that represented in figure 82 may be used
to produce homogeneous sodium
light, ais a Bunsen burner, b a
chimney with an opening in one
side, and d a movable rod, to
which is fastened a platinum wire
and a platinum-gauze spoon. Com-
mon salt is melted in this spoon and
volatilized in the hottest portion
of the flame.
The following simple contriv-
ance is also to be recommended
for producing a strong and lasting
sodium light :
A strong platinum wire is cov-
ered with platinum gauze. The
necessary sodium chloride, or,
better, sodium bromide, on ac-
count of the greater intensity of
light, is fused, finely powdered,
and placed in a platinum boat.
The platinum gauze is then heated
to redness and rolled in the sodium
salt. A Miinke burner is used as
the source of light (p. 186).
Influence of Temperature,
Liquid-tube, and Liquid.—An
elevation of i° in temperature for a
column of liquid 2 dm. in length
diminishes the angle of rotation
several tenths of a degree. The
observation temperature, therefore, must be noted for all accurate
measurements. It is advantageous to make the observations at
a constant temperature of about 20°. This can be easily done
Fig. 82. ROTATION OF THE PLANE OF POLARIZATION.
if the liquid-tube is surrounded by a metallic mantle (Fig. 83),
which is filled with water during the experiment, and which is pro-
vided with a thermometer opening at d.
If the apparatus is not provided with this contrivance, tubes of
the ordinary form (Fig. 84) are used. These are glass tubes A,
usually 1 to 2 dm. long ; they are ground off at the ends exactly
perpendicular to their axes, and are closed by means of parallel
Fig. 83.
glass plates (g} g2), which can be fastened on by means of the screw
arrangements mx nv m 2 n.,.
The glass plate must not be pressed down too strongly, for glass
under pressure becomes doubly refracting; this would influence the
rotation of the plane of polarization, and hence introduce an error.
It is better, therefore, to place a rubber ring on the inner glass
Fig. 84.
surface. In all cases, however, the influence of these plates for new
instruments should be tested.
The exact length of the tube should be given by the manufacturer;
otherwise see the measuring contrivance of Landolt, Drehungsver-
mogen, p. 125, 1879.
The tube and glass plates must be carefully cleaned. The pres-
ence of air-bubbles must be avoided in filling the tube. The liquid POLARIMETER OF MITSCHERLICH.
207
should be clear. In case of filtration, care must be taken to
prevent any change in the concentration of the solution.
the weights should be given in percentages. For accu-
rate determinations, the weighings should be reduced to the vacuum
standard (p. 12). The specific gravity is determined by means
of the pyknometer (p. 19). The results should be accurate to
the fourth decimal place.
Special attention should be called to the bi-rotation and similar
phenomena, according to which the rotatory power of many solu-
tions undergoes a change with time, and frequently becomes con-
stant after the lapse of considerable time (Ostwrald, Allgem. Chem.,
2. Aufl., Bd. 1, p. 496, 1891, and Sonnenthal, Zeit. phys. Chem. 9,
p. 656,1892).
The apparatus (Figs. 85 and 86) consists in its simplest form
of a polarizing Nicol a, by means of which the light on entering the
tube is polarized. The rays of light are made parallel by means
of a lens; and, after passing through the empty or filled tube f,
they enter the second analyzing prism b, which is usually fastened
to a graduated circular disc (with vernier, p. 215), by means of
which the prism can be rotated. Sometimes, as in the figure, the
disc is fixed in position ; in such cases the vernier is fastened to
the prism and may be rotated by means of the handle c.
1. THE POLARIMETER OF MITSCHERLICH.
The observations are carried out in a (at least, partially) dark-
ened room ; foreign light may be excluded by a black screen placed
behind the sodium light.
The empty tube is first placed in the apparatus, the analyzer
rotated through 360°, and the two positions, 180° apart, are
determined for which the Nicols are crossed (positions of maxi-
mum darkness). The field of view then appears somewhat like
figure 87 ; black streaks occur in the middle of the field. The
zero of the scale can be adjusted to this position by rotating the
polarizer with the help of the screw e; this adjustment, however,
is usually made by the manufacturer.
After determining the zero point, the tube is filled with liquid,
and the angle measured through which the analyzer must be ROTATION OF THE PLANE OF POLARIZATION.
rotated to the right or left to restore the condition of maximum
darkness.
If the angle, calculated from the zero point, is smaller when
the analyzer is turned to the right than when turned to the left,
a dextrorotatory substance is usually present, while in the opposite
case a levo body is present. If, for example, the analyzer must
be rotated 40° to the right or 140° to the left to restore the maxi-
mum darkness, the substance
is dextrorotatory.
To determine this with
certainty, in doubtful cases,
where considerable rotation
is produced, a tube of half
the length or a solution of
half concentration is used.
The rotation then will be
only half as great as in the
first case. In the above ex-
Fig. 86.
Fig. 85.
Fig. 87.
ample therefore, the analyzer must be rotated 20° or 200° to the
right, or adjusted from the left to the numbers no° or 290°, then ;
„ , . 140°
290° = 360° —.
For accurate measurements a large number of observations should
be made, and the adjustment made for the two positions of maxi-
mum darkness, ißo° apart; the results obtained frequently show
slight variations. The differences between the separate observa-
tions usually amount to several tenths of a degree.
The Mitscherlich apparatus has been modified in recent times POLARISTROBOMETER OF WILD.
209
somewhat on the principle of the half-shadow instrument. A
small telescope is placed in front of the analyzer and a quartz
plate of definite thickness is introduced behind the polarizer. On
rotating the analyzer, the two halves of the field of view become
evenly and unevenly shaded, as in the case of the Laurent and
Lippich apparatus described farther on. This new construction of
the Mitscherlich apparatus is more sensitive than the older form.
2. THE POLARISTROBOMETER OF WILD.
This apparatus (Figs. 88 and 89) is capable of sharper adjust-
ment than that of Mitscherlich.
A Savart plate * s, formed of two quartz or calcite plates, is
placed between the polarizing and analyzing Nicols. A number of
dark interference bands (Fig. 90) are produced by this plate,
which vanish for definite positions of the prisms. In the measure-
Fig. 88.
ments, the instrument is adjusted to these positions of maximum
illumination.
The polarizer, which is illuminated by sodium light, is fastened
to the graduated disc E provided with a vernier; this disc can be
rotated by means of the knob P fastened to the toothed rod Q.
The readings are made by means of the telescope T, in which is
placed at Van inclined mirror, which reflects the light from a small
gas-flame onto the vernier. It is to be noticed, inasmuch as the
polarizer is rotated, that a rotation of the disc E to the left, and
therefore of the knob P to the right, corresponds to a dextro-
rotatory substance.
The zero point is adjusted by determining, during the rotation
of Q, the four positions 90° apart, for which the interference bands
* Wiillner, Physik, 3. Aufl., Bd. 11, p. 604, 1875. 2 10
ROTATION OF THE PLANE OF POLARIZATION.
(Fig. 90) vanish. By means of the screw M these positions can be
made to correspond with the scale divisions o°, 90°, 180°, and
270°, provided this adjustment has not already been made.
Fig. 89.
The instrument can be adjusted very sharply to the maximum
illumination. The apparatus is provided with a small cross-wire
telescope (Fig. 88, c, d, e), the eye-piece of which is focused
sharply on the cross-wires. In adjusting to
maximum illumination the cross-wires should
be placed symmetrically with reference to the
darkened edges of the field of view.
The direction in which the substance rotates
the plane of polarization is determined as on
page 208, greater care being necessary, how-
ever, owing to there being four zero points.
Let the zero points be o°, 90°, xBo°, and
270°, and, after introducing the filled tube, suppose the positions
of maximum illumination to be 40°, 130°, 220°, and 310° ; a ro-
tation of 40° to the right or 50° to the left is to be considered.
Fig. 90. HALF-SHADOW APPARATUS OF LAURENT.
A tube of half length or solution of half concentration is then ex-
amined, and if the substance is dextrorotatory, the positions of
maximum illumination will be 20°, uo°, 200°, and 290°, or if
levo-, 65°, 1550, 2450, and 3350.
In the case of strongly rotating substances the angle of rotation
sometimes amounts to more than 90°. By examining tubes of
different lengths, however, it is an easy matter to determine
whether the angle is aor 900 + a.
For extremely accurate work the measurements should be made
from each of the four zero points; usually, however, it is sufficient
to measure from two points xBo° apart. After a little practice, the
separate observations should not vary more than a few hundredths
of a degree.
The measurements are carried out in a somewhat darkened room.
The liquids should be clear; any coloration should, if possible, be
avoided.
3. THE HALF-SHADOW APPARATUS OF
LAURENT.
The sodium light enters this polarimeter (Figs. 91 and 92)
through a diaphragm, which is provided with a plate of potassium
bichromate crystal, in order to remove the foreign light which
accompanies the yellow light.
On leaving the lens e, the rays pass parallel into the Nicol d, and
then enter a second diaphragm f half of which is covered with a
quartz or mica plate of definite thickness cut parallel to the axis.
From here the rays pass through the liquid-tube p into the analyzer
g, thence through the lenses i and h (Fig. 92) of the telescope K,
through which the observations are made.
The characteristic part of the apparatus is the quartz or mica
plate, the thickness of which is chosen so that the rays of sodium
light which pass through suffer a change of phase of half a wave-
length.
If the polarizer is adjusted so that the plane of polarization of
the light is parallel to the axis of the quartz, then for each position
of the analyzer the two halves of the field of view will be equally
illuminated. If, however, the polarizer is placed at an angle a with 2 12
ROTATION OF THE PLANE OF POLARIZATION.
this axis, the plane of polarization of the rays of light which pass
through the quartz plate will suffer a like displacement, but in the
opposite direction (Landolt, Drehungsvermogen, p. 115, 1879).
For this second adjustment the circular field of view appears
divided into two halves (Fig. 93), which for most positions of the
Fig. 91.
Fig. 92.
Nicol are unequally illuminated (Fig. 93, 1 and 2), but which for
two positions 180° apart are uniformly illuminated.
The instrument can be adjusted sharply to this mean, uniform
illumination ; this is the zero position from which the measure-
ments are made. HALF-SHADOW APPARATUS OF LAURENT.
213
The apparatus (Fig. gi) is constructed so that the analyzer,
fastened to the telescope and vernier, can be moved by means of
an arm on the fixed circle c. The vernier is read by means of the
microscopd L.
As already mentioned, the plane of the polarizer must form an
angle with the axis of the quartz plate, thereby producing unequal
illuminations of the two halves of the field. This is accomplished
by means of the contrivance JK, by means of which the polarizer
can be rotated.
The apparatus is firsf adjusted to the parallel position, so that for
any position of the analyzer the two halves of the field of view are
equally illuminated. The polarizer is then rotated through the
angle aby means of JK. The smaller the angle is, the more
sensitive is the instrument; the more brilliant the light and the
clearer the liquid, the smaller can a be. The proper adjustment of
Fig. 93.
the polarizer is that position corresponding to the greatest change of
shade in the field of view for a slight movement of the analyzer.
At the beginning of the observation the telescope is focused
sharply on the diaphragm, so that the dividing line at the edge of
the quartz plate appears sharp.
In determining the zero point the tube should be filled with
water, in order that the intensity of the light may be the same as
that when the active liquid is observed. In case the field of view
is too dark, on account of the liquid being colored or not being
clear, the illumination may be increased by a slight rotation of the
polarizer; this, however, renders the instrument less sensitive.
If a dextrorotatory substance is observed, the angle on the circu-
lar disc will be smaller when turned to the right than when turned
to the left; for strongly rotating substances, the method on page
208 is used. 214
ROTATION OF THE PLANE OF POLARIZATION.
The mean of a large number of results, measured from the two
zero points xBo° apart, should be taken as the true value.
The apparatus can be used only for sodium light, for the thick-
ness of the crystal plate has already been adjusted for L
4. THE HALF-SHADOW APPARATUS OF
LIPPICH.
The essential features in the method of operation for the Laurent
apparatus apply also to this much-used apparatus.
The main difference in the construction consists in that the
quartz plate is replaced in this apparatus by a third Nicol prism,
which covers half of the field of view.
On rotating the polarizer by means of an arm, its plane of polar-
ization forms an angle with that of the smaller middle prism. This
angle should be as small as possible (p. 213).
This apparatus has the advantage over that of Laurent in that
homogeneous light of any wave-length can be used. With the
finer construction of this apparatus the angles may be read to
0.001 or 0.002°. On observations with this apparatus, see, among
others, Sonnenthal, Zeit. phys. Chem. 9, p. 660, ibid. Rimbach,
p. 700, 1892.
On the technically important apparatus of Soleil-Ventzke for investigations of
sugar, see Landolt, Drehungsvermogen, p. 149, 1879.
Tables of the Rotatory Power, Landolt-Bornstein, Phys. chem. Tab., p. 224,
xBBj.
The significance of the rotatory power in stereochemistry, see Meyerhoffer,
Stereochemie, Leipzig, 1892, and Hantzsch, Grundriss der Stereochemie, Breslau,
1893.* The other uses for scientific and technical purposes, especially for deter-
mining the concentrations of solutions, see Landolt, Optisches Drehungsvermogen,
1879, anh ®er- d* h- diem. Ges. 21, p. 191, 1888. For further recent literature
see Hartmann, Ber. d. d. chem. Ges. 21, p. 221, 1888 ; Pribram, Sitzungsber.
Wien. Akad. (97) II b, June, 1888, and Ber. d. d. chem. Ges. 22, p. 6, 1889 ; Long,
Sill. Ann. Jour. 36, p. 351» 1888, and 38, p. 264, 1889; Sorokin, Jour. russ.
Ges. p. 417, 1888; Ref. Zeit. phys. Chem. 4, p. 482, 1889; Kanonnikow, Jour,
russ. Ges. pp. 571 and 686, ISBB, and p. 369, 1890 ; Ref. Zeit. phys. Chem. 4,
p. 482, 1889, and 6, p. 88, 1890; Sonnenthal, Zeit. phys. Chem. 9, p. 660;
Rimbach, ibid. 9, p. 700, 1882.
On magnetic rotation, see Perkin, Ber. d. d. chem. Ges. 15, p. 1363, 1882 ;
Jour. Chem. Soc. 45, p. 422, 1884; 52, p. 362; 1887; 53, p. 561, 1888; 55, GENERAL CONTRIVANCES FOR MEASUREMENTS.
215
p. 680, 1889. Jour, prakt. Chemie N. F. 32, p. 523, 1885 ; Chem. News 59,
p. 247, and 60, p. 253, 1889; 62, p. 255, 1890; 64, p. 269, 1891 ; Jahn, Sitz-
ungsber. Berl. Akad. p. 237, 1891, and Wied. Ann. 43, p. 280, 1891; Wachs-
muth, Wied. Ann. 44, p. 377, 1891, and Schonrock, Zeit. phys. Chem. 11,
P- 753, i 893-
XX. GENERAL CONTRIVANCES FOR
MEASUREMENTS.
1. THE VERNIER (CIRCULAR VERNIER).
The arc A (Fig. 94) is fixed in position, while the arc 8,. the
vernier, is movable about the central point of the two arcs. Ais
graduated in degrees and half degrees, B is divided so that 30 of
Fig. 94.
its divisions correspond to 29 half-degree divisions on the main
circle; therefore each division on the vernier is one minute of arc
smaller than one division on A. GENERAL CONTRIVANCES FOR MEASUREMENTS.
The vernier is adjusted so that its zero point coincides with the
zero point of the circle ; the first division then is removed i', the
second 2', the third 3', etc., from the corresponding divisions on
the circular scale.
If the vernier is rotated through a definite angle, the magnitude
of which is to be determined, the number of whole and half degrees
through which the index o of the vernier has moved, is read off
directly from the main circle.
This reading is sufficient only in case the zero of the vernier
coincides with a division on the circle ; usually, therefore, a definite
number of minutes must be added to the first reading. The
number of the division on the vernier which coincides with a
division on the main scale, represents the number of minutes to be
added.
The vernier is usually read by means of a microscope, which
must be placed so that the division to be observed falls in the
middle of the field of view. The field of view is illuminated,
when necessary, by means light reflected from a small mirror;
a small white paper-screen may also be used for this purpose.
The apparatus with vernier attachment is frequently constructed
so that the vernier is fixed and the circle movable.
2. THE CATHETOMETER.
The cathetometer is used to measure the vertical distance between
two points.
The column M (Fig. 95) resting on the foot D, which is sup-
ported by the screws mx m 2 mt, is movable about its axis.
On this column are two sliding contrivances F and F', with
which the telescope B is fastened, and which are connected to the
counter-weight Q by means of a cord passing over the pulley T.
The slide F' can be clamped at any desired height by means of
the screw K, after which the slide F can be raised or lowered by
means of the micrometer screw J. The telescope B provided with
the spirit-level L is fastened to Fby means of the forks G and G'.
The telescope can be leveled by means of the screw o.
In the middle of the column Mis an inlaid silver strip, which is
graduated in small divisions. By means of a vernier in the opening THE CATHETOMETER.
Fig. 95. 21 8
GENERAL CONTRIVANCES . FOR MEASUREMENTS.
at F it is possible to determine the vertical distance between two
positions of the telescope with great accuracy.
In carrying out the measurements it is necessary (i) that the axis
of the column is exactly vertical; and (2) that the axis of the tele-
scope is exactly horizontal.
To adjust the axis of rotation to a vertical position, the column
is turned so that the axis of the telescope is parallel to the line
joining mx and mr After adjusting the spirit-level by means of
these screws, the column is turned through an angle of xBo°, and
the level again adjusted by means of the screw 0 and the foot-screws
m 1 and w2; the adjustment must be such that the level remains
unchanged for these two positions 180° apart. When this is accom-
plished, the column is rotated so that the axis of the telescope is
perpendicular to the line joining m 1 and m 2; the level is then
adjusted by means of the screw mr The final adjustment must be
such that the level remains unchanged during a complete rotation.
To determine whether or not the axis of the telescope is hori-
zontal, the cross-wires of the telescope are adjusted sharply on a
definite mark ; the telescope is then removed from its position,
turned end for end, and replaced in its position. The column is
then rotated through 180°, when the cross-wires must again coincide
with the mark, provided the axis of the telescope is horizontal. If
the cross-wires do not fall exactly on the mark, half of the distance
must be corrected by means of the screw 0.
3. THE THERMOMETER.
The Beckmann Thermometer.—Besides the ordinary mer-
cury thermometer, the Beckmann thermometer is especially valuable
in physico-chemical measurements. This thermometer can not be
used for determining definite temperatures, but only for determining
definite temperature differences (depression of the freezing point,
elevation of the boiling point, thermochemical measurements, etc.).
The thermometer, provided with an arbitrary scale divided into
0.01 or 0.020, is represented in figure 36, page 82. The char-
acteristic part, the mercury reservoir at the upper end, is shown in
figure 96.
By means of this reservoir at the upper end of the thermometer- THE THERMOMETER.
219
tube, the quantity of mercury in the lower bulb of the thermometer
can be increased or decreased.
If a definite temperature change is to be measured, the ther-
mometer js heated to approximately the desired temperature; if,
then, the mercury thread is too long, the thermometer is heated to
i or 20 above the temperature, until the thread extends to the
mercury in the upper reservoir. By gently tapping the lower
end of the thermometer with the hand, the mercury thread is
broken off from the excess of mercury in the reservoir. If the
quantity of mercury in the lower reservoir should be too small, the
adjustment is made in a manner similar to that
just described : the thermometer is heated until
the thread extends to the mercury in the reser-
voir, and, after cooling to approximately the
desired temperature, gently tapped with the
hand, as before.
These and other thermometers, constructed
in recent times by F. O. R. Gotze, in Leipzig,
have been adjusted so that the same thermo-
meter can be used for freezing-point and boil-
ing-point determinations.
It must also be noticed that for such ther-
mometers, owing to the separation of the mer-
cury at higher temperatures, the degree becomes
somewhat smaller ; the elevation of the boiling
point is thereby diminished. Inasmuch as this
error may amount to more than i per cent., it
is necessary for accurate measurements that the thermometer be
calibrated, in case the corrections for different temperatures are not
known.
Fig. 96.
Mercury thermometers for measuring temperatures up to 550°, see Reckling-
hausen, Ber. d. d. chem. Ges. 26, p. 1514, 1893 ; see, further. The Measurement
of High Temperatures, by C. Earns, Leipzig, 1892.
A simple air thermometer: Lothar Meyer, Ber. d. d. chem. Ges. 26, p. XO5O,
1593.
Thermometer Testing and Temperature Corrections.—
The testing and correcting of thermometers may be divided as
follows: (a) Determination and correction of the zero point;
the boiling point; (V) correction for the value of the degree ; 220
GENERAL CONTRIVANCES FOR MEASUREMENTS.
(d) correction for the projecting thread of mercury ; () correc-
tion of the caliber error.
Determination of the Zero Point.—The thermometer is
kept for a considerable time at a temperature not much above o°,
packed in melting snow or immersed in pulverized ice moistened
with distilled water. The water formed must be carefully removed.
The determination should also be made by lowering the tempera-
ture of the room.
The thermometer is left in the ice for an hour or so, after
which the temperature is read. This temperature, equal to that of
the ice, is represented by E .
If the thermometer is heated to a higher temperature, the capac-
ity of the mercury reservoir increases, owing to the expansion of
glass. On subsequent cooling, this change, in many cases, is not
completely corrected until weeks or even months have elapsed.
This causes a lowering of the position of the mercury, a depression
of the zero point, the amount of which depends on the kind of
glass, the temperature to which it has been heated, and the length
of time heated. After heating for some time at ioo°, the depres-
sion for ordinary glass amounts to i°, for Jena normal glass a mean
of 0.056° (Bottcher, Zeit. f. Instrumentenkunde, p. 409, 1888).
Owing to this depression of the zero point, it is better that
thermometers which are to be used for temperatures approximately
equal to zero should be kept in a room of as low a temperature as
possible, and should be surrounded by snow for a considerable
time before use. If the thermometer is to be used for higher tem-
peratures, then the zero point ElOO should be determined; i.e., the
zero point which a thermometer shows after remaining for some
time in ice, when the same thermometer, about half an hour before,
had been heated to ioo°. This zero point is also used as the basis
for graduating thermometers. For use at higher temperatures, the
zero point is determined for the corresponding temperature; e.g.,
Em, Em, etc. In such cases the change of the zero point may be
considerable. If E0 and Ewo are known, and /is a temperature
between o and ioo°, then we have approximately :
E =£loo+ E° Iof10° (100 /)*
* Landolt, Zeit. phys. Chem. 4, p. 351, ISB9. THE THERMOMETER.
22 1
For thermometers of Jena normal glass the equation is approx-
imately :
Et = ElOO -(-0.00056(100—/).
This zero correction must always be subtracted from the observed
temperature
Determination of the Boiling Point.—The apparatus rep-
resented in figure 97 may be used for this purpose. The ther-
mometer B is fastened in the top
of the double-walled vessel A C,
so that the mercury thread, when
adjusted to the boiling point,
stands at the top of the stopper,
and so that the mercury reservoir
is at least 2 cm. above the surface
of the boiling liquid. The vapor
escapes at r; a small water man-
ometer is placed at r' to measure
the excess of pressure p in the
vapor chamber. The pressure in
the apparatus is slightly greater
than the atmospheric pressure,
owing to the narrowness of the
outlet-tube r. After heating for
a suitable length of time, the tem-
perature is read off. The baro-
metric pressure is simultaneously
read, reduced to o° (p. 224), and
then added to the slight excess of
pressure p, which must first be
reduced to mercury units. If bis the corrected barometric pres-
sure in millimeters, then the boiling point t of water (between 715
and 770 mm.) is given to o.oi° by the equation :
Fig. 97.
See also Tabellen von Landolt-Bornstein, p. 40, 1883.
Correction for the Degree Value.—lf A is the boiling point
t = xoo° 0.0375° (b 760).
* Kohlrausch, Prakt. Phys. vn, p. 82, 1892. 222
GENERAL CONTRIVANCES FOR MEASUREMENTS.
reduced to 760 mm., and Em the freezing point, with a ther-
mometer previously heated to ioo°, then the degree value of the
thermometer is:
100
C J? 9
° 0
and the degree-value correction which is to be added to the ob-
served temperature t is :
Correction for the Projecting Mercury Thread.—This
correction is given by the formula of Landolt,* as follows;
g = {G-i)t.
/= 0.000131 (« io) t,
where n is the length of the projecting thread and t is the observed
temperature. The correction /isto be added in all temperature
measurements.
The corrections for the projecting mercury thread are given in
the table (p. 236) calculated by Rimbach for thermometers of
Jena glass (graduated to o.i° for o— ioo°) and for (o—360°).
This correction, however, should be avoided whenever possible.
See Guillaume, Compt. rend. 112, p. 87, 1891, and Mahlke,
Zeit. f. Instrumentenkunde 13, p. 58, 1893.
Calibration of the Thermometer.—The errors arising from
the unequal diameters of the tube are, especially for high tempera-
tures, of considerable magnitude. For accurate measurements,
therefore, the calibration of the thermometer must not be neglected.
For this purpose the mercury thread is broken off from the
main quantity of mercury, of such a length a, measured in
degrees, that n = is approximately a whole number. For
thermometers which are used for high temperatures a=so ; in
general, a= 20 or io°.
The mercury thread may be broken off by tapping the thermo-
meter after it has been turned upside down. If the thread is too
long or too short, the process is repeated, and, inasmuch as the
thread usually breaks at the top of the mercury bulb,f its length
* Landolt, Zeit. phys. Chem. 4, p. 353, 18S9.
f To obtain a thread of any desired length, see Kohlrausch, Prakt. Phys. vix,
p. 84, 1892. THE THERMOMETER.
223
can be first adjusted by means of ice-water to the desired value
and the thermometer then gently tapped.
If a definite interval—e.g., from o to 100—is to be calibrated,
then the number of scale divisions which correspond to the length
of the thread in the different intervals o to a, ato 2 a . . . (n —1) a
to 100 must be determined. The thread must be moved in this proc-
ess from one interval to another, and the readings should be unin-
fluenced by parallax. The parallax can be avoided by placing the
thermometer on a plane mirror and making the reading with the
eye in the same straight line with the scale division and its image.
The use of a cross-wire microscope provided with a micrometer
screw and slide contrivance is still better.
Let E be the zero point and 100 -f- the boiling point of the
thermometer, and suppose the length of the thread in scale divi-
sions for the different intervals to be as follows:
Intervals.
O a
a— 2 a
(n —l) a 100
Scale Divisions.
a + dj
a -j- d 2
a 6n, etc. ;
then, if we write
£ s“f ~f“ ”f" •• •
n
the correction table* of the thermometer (without regard to
the correction of the zero point) is as follows :
Scale Division.
a
2 a
m a
Correction.
A-cl,
2 A (cl, -|- d 2)
mA (d, + d 2 • • • dm).
These corrections are to be added to or subtracted from the cor-
responding scale divisions according as their values are positive or
negative. The results are then represented graphically, and the
correction for each degree obtained from the curve, f
General.—When all of these corrections for a temperature
*See Kohlrausch, Prakt. Phys. vn, p. 86, 1892.
I See also the calibrations of Neumann-Thiesen, Carl’s Repert. Exp. Phys.
15, ,P. 285. 224
GENERAL CONTRIVANCES FOR MEASUREMENTS.
determination have been obtained, it is unnecessary to make a com-
parison with an air thermometer, and the accuracy of the tempera-
ture is increased more than tenfold.
If a good, standard thermometer is at hand, a correction table
for any thermometer can be obtained by comparison with the
standard. A calibration is then unnecessary.
The two thermometers are fastened together, with their mercury
bulbs side by side, and heated to different temperatures in a ther-
mostat. A better method, however, is the simultaneous heating of
the two thermometers in the vapors of boiling liquids, whereby
the change from one temperature to another can be easily accom-
plished by means of a good pressure regulator (p. 95).
A microscope, provided with cross-wires, or an eye-piece micro-
meter, and movable in a vertical direction, should be used for
reading the thermometer scale in all accurate determinations. The
thermometer should always be shaken or gently tapped before the
reading is made. It is also to be observed that the position of the
top of the mercury thread, for a definite temperature, deviates
slightly, according as the mercury rises or falls to the position in
question.
4. THE BAROMETER
A good barometer (mercury barometer) should be free from air
and aqueous vapor.
The top of the mercury is read with the naked eye avoiding
parallax, or with a cathetometer.
The most important correction is the reduction of the barometric
pressure to o°. If bis the observed barometric pressure, t the
temperature, and 0.000181 the coefficient of cubical expansion
of mercury, then the barometric pressure reduced to o° is
b0 =b— 0.000181 bt.
When the expansion of the measuring scale is to be taken into
account, the coefficient of expansion of brass can be taken as
0.000019 and that of glass as 0.000008; the barometric pressure
is then calculated to o° :
For a brass scale by the formula b0 b 0.000162 b t
“ “ glass “ “ “ “ b—0.000173 £ A
(Tables of Landolt-Bornstein, p. 26, 1883). THE BAROMETER.
225
If the diameter of the barometer-tube is less than about 20 mm.,
the capillary depression must be taken into account. The correc-
tions for tubes of different diameters are given in Landolt-Bornstein’s
Tables, p. 21, 1883. These corrections are to be added to the
height of the mercury column.
The reduction of the barometric pressure to 450 geographical
latitude is, in general, unnecessary for chemical purposes (Kohl-
rausch, Prakt. Phys. yii, p. 74, 1892). 226
TABLES.
XXL TABLES.
TABLE OF ATOMIC WEIGHTS.
According to Ostwald and
Clarke,*
on the Basis of o=i6.
Aluminium, . , . . 27 x 0 27.11
Ostw. Clk.
Molybdenum, , . . 95.90 95-99
Ostw. Clk.
Antimony, 120.30 120.43
Argon,
Neodymium, . . . 140.80 140.80
Nickel, 59-00 58-69
Arsenic, 75 00 75-01
Nitrogen, ..... 14.04 14.04
Barium, . . 137.00 137-43
Bismuth, 205.00 208.11
Osmium, 192.00 190.99
Oxygen, x 6.00 16.00
Boron, n.oi 10-95
Bromine, 79-96 79-95
Palladium, 106.00 106.36
Phosphorus, .... 31.03 31.02
Cadmium, 1X2.10 111.95
Calcium, 40.00 40.07
Platinum, 194.80 194.89
Potassium, .... 39.14 39-11
Carbon, 12.00 12.00
Cerium, 140.20 139-35
Praseodymium, . . . 143.60 143.60
Rhodium, 103.00 103.01
Caesium, 132.90 132.89
Rubidium, 85.40 85.43
Chlorine, 35.45 35-45
Chromium, .... 52.20 52.14
Ruthenium, .... 103.80 x0x.68
Samarium, .... 150.00 150.26
Cobalt, 59-00 58.99
Columbium, .... 94 20 93-73
Scandium, .... 44.10 44-12
Selenium, 79-10 79.02
Copper 63.30 63.60
Erbium, 166.00 166.32
Silicon, 28.40 28.40
Silver, 107.938 107.92
Fluorine, 19.00 19.06
Sodium, 23.06 23.05
Gadolinium, 156.76
Gallium, 69.90 69.91
Strontium, .... 87.50 87.6 X
Sulphur, 32.06 32.07
Germanium 72.30 72.48
Glucinum (Berylium), 9.10 9.08
Tantalum, .... 183.00 182.84
Tellurium, . ... 125.00 127.49
Gold, 197.20 197.23
Helium,
Terbium, 160.00
Thallium, 204.10 204.15
Hydrogen, .... 1.007 1.008
Indium, 113.70 113.85
Thorium, ..... 232.40 232.63
Thulium, 171.00 170.10
lodine, 126.86 126.85
Tin, 118.10 119.05
Iridium, 193-20 193.12
Iron, 56.00 56.02
Titanium, 48.10 48.15
Tungsten, 184.00 184.83.
Lanthanum, .... 138.50 138.64
Lead, 206.91 206.92
Uranium, 239.40 239.59
Vanadium 51.20 51.38
Lithium, 7.03 7.03
Magnesium, .... 24.38 24.28
Ytterbium, . . . .173.20 173.19
Yttrium, 89.10 89.02
Manganese, .... 55-00 54-99
Mercury, 200.40 200.00
Zinc, 65.50 65.41
Zirconium, 90.70 90.40
* [Clarke’s latest report, Jour. Amer,
Chem. Soc. 20, p. 171, 1898.—Tr.] TABLES.
227
TABLE OF OBACH, ABRIDGED ACCORDING TO OSTWALD.
f
for a
1000 a
(Electric Conductivity.)
to a 999.
o
1
2
3
4
5
6
7
8
9
oo
1.0000
010
020
030
040
050
060
071
081
091
OI
101
in
122
132
142
152
163
i73
183
194
02
204
215
225
235
246
256
267
278
288
299
03
309
320
33i
341
352
363
373
384
395
406
04
4i7
428
438
449
460
47i
482
493
5°4
5i5
05
526
537
549
560
571
582
593
605
616
627
06
638
650
661
672
684
695
707
718
73o
74i
07
753
764
776
788
799
811
823
834
846
858
08
870
881
893
905
917
929
941
953
965
977
09
989
*001
*013
*025
*038
*050
*062
*074
*087
*099
IO
O.IIII
124
136
148
161
173
186
198
211
223
II
236
249
261
274
287
299
312
325
338
35i
12
364
377
39°
403
416
429
442
455
468
481
13
494
508
521
534
547
561
574
588
601
614
H
628
641
655
669
682
696
710
723
737
75i
15
765
779
793
806
820
834
848
862
877
891
l6
905
919
933
947
962
976
990
*005
*019
*034
17
0.2048
063
077
092
107
121
136
iSi
166
180
l8
195
210
225
240
255
270
285
300
3!5
33i
19
346
361
376
392
407
422
438
453
469
484
20
500
516
53i
547
563
579
595
610
626
642
21
658
674
690
707
723
739
755
771
788
804
22
821
837
854
870
887
903
920
937
953
970
23
987
*004
*021
*038
*055
*072
*089
*106
*123
*141
24
0.3158
175
193
210
228
245
263
280
298
316
2.5
333
35i
369
387
405
423
441
459
477
495
26
514
532
5So
569
587
605
624
643
661
680
27
699
717
736
755
774
793
812
831
850
870
28
889
908
928
947
967
986
*006
*025
‘045
*065
29
0.40S5
104
124
144
164
184
205
225
245
265
3°
286
306
327
347
368
389
409
430
451
472
31
493
5U
535
556
577
599
620
641
663
684
S2
706
728
749
771
793
815
837
859
881
.903
33
925
948
970
993
*015
*038
*060
*083
*106
*129
34
0.5152
175
198
221
244
267
291
314
337
361
35
385
408
432
456
480
504
528
552
576
601
36
625
650
674
699
723
748
773
798
823
848
37
873
898
924
949
974
*000
*026
*051
*077
*103
3«
0.6129
155
181
208
234
260
287
313
340
367
39
393
420
447
475
502
529
556
584
611
639
40
667
695
722
750
779
807
835
863
892
921
41
949
978
’ 007
*036
*065
*094
*123
*153
'182
*212
42
0.7241
271
301
331
361
39i
422
452
483
513
43
544
575
60 6
637
668
699
73i
762
794
825
44
857
889
921
953
986
*018
*051
*083
*116
*149
45
0.8182
215
248
282
3i5
349
382
416
45°
484
46
5J9
553
587
622
657
692
727
762
797
832 228
TABLES
0
1
2
3
4
5
6
7
8
9
47
868
9°4
939
975
Oil*
048*
084*
121*
i57*
194*
48
0.9231
268
305
342
380
418
455
493
53i
57°
49
608
646
685
724
763
802
841
881
920
960
5o
1.000
004
008
0X2
016
020
024
028
033
°37
5i
041
045
°49
053
058
062
066
070
075
079
52
083
0S8
092
096
IOX
105
110
114
119
123
53
128
132
137
141
146
151
i55
160
165
169
54
174
179
183
l88
193
198
203
208
212
217
55
222
227
232
237
242
247
252
257
262
268
5«
2 73
278
283
288
294
299
304
3°9
3*5
320
57
326
33i
336
342
347
353
358
364
37o
375
58
381
387
392
398
404
410
4i5
421
427
433
59
439
445
45i
457
463
469
475
481
488
494
bo
5 00
506
513
519
525
532
538
545
55i
558
6i
564
57i
577
584
59i
597
604
611
618
625
62
632
639
646
653
660
667
674
681
688
695
63
703
710
717
725
732
740
747
755
762
770
64
778
786
793
801
809
8.7
825
833
841
849
65
857
865
874
882
890*
899
907
9i5
924
933
6b
941
95°
959
967
976
985
994
003*
012*
021*
67
2.030
040
049
058
067
077
086
096
106
i*5
68
125
135
145
155
165
175
185
195
205
2*5
69
226
236
247
257
268
279
289
300
311
322
70
333
344
356
367
378
390
401
4i3
425
436
7i
448
460
472
484
497
S09
521
534
546
559
72
571
584
597
610
623
636
650
663
676
690
73
704
717
73i
745
759
774
788
802
817
831
74
846
861
876
891
906
922
937
953
968
984
75
3.000
016
032
049
065
082
098
US
132
149
76
167
184
202
219
2 37
255
274
292
3x0
329
77
348
367
386
405
425
444
464
484
505
525
78
545
566
587
608
630
651
673
695
717
739
79
762
785
808
831
854
878
902
926
950
975
80
4.000
025
051
076
102
128
155
181
208
236
81
263
291
319
348
376
405
435
465
495
525
82
556
587
618
650
682
7*4
747
780
814
848
83
882
917
952
988
024*
061*
098*
135*
173*
211*
84
5.250
289
329
369
410
452
494
536
579
623
85
667
711
757
803
849
897
944
993
042*
092*
8b
6.143
194
246
299
353
407
463
5i9
576
634
87
692
752
813
874
937
000*
065 *
130*
197*
264*
88
7-333
403
475
547
621
696
772
850
929
009*
89
8.091
174
259
346
434
524
6iS
7°9
804
901
90
9.000
IOX
204
3°9
417
526
638
753
870
989
9i
IO.XI
IO-33
10.36
10.49
10.63
10.77
10.90
11.05
11 20
u-35
92
ii-5o
11.66
11.82
11.99
12.16
I2-33
12.51
12.70
12.S9
13.08
93
13.29
*3-49
13 7i
13-93
14-15
14-38
1463
14.87
i5 13
*5 39
94
15-67
15-95
16.24
16.54
16.86
17.18
17-52
17.87
18.23
18.61
95
19.00
19.41
19.83
20.28
20.74
21.22
21.73
22.26
22.81
23-39
9b
24.00
24.64
25-32
26.03
26.78
27-57
28.41
29 30
30.25
31.26
97
32-33
33-48
34-7i
36.04
37-46
39.00
40.67
42 48
44-45
46.62
98
49.00
51.6
54-6
57-8
61.5
65-7
70.4
75 9
82.3
89.9
99
99.0
no
124
142
166
199
240
33 2
499
999 TABLES.
229
TABLE FOR THE CALCULATION OF REFRACTIVE INDICES
FOR SODIUM LIGHT ACCORDING TO PULFRICH.
Deg.
Min. i
Refrac-
tive
Index.
d
Deg. Min.
Refrac-
tive
Index.
»
d
Deg.
Min.
Refrac-
tive
Index.
d
O
°
I,6l 511
0,1
8
0
1,60 910
2,5
16
0
1,59 HI
4,8
10
5ID
0,1
10
885
2,5
IO
093
4,9
20
S°9
0,1
20
860
2,6
20
044
4.9
3°
508
0,2
30
834
2,7
30
1,58 995
5,°
4°
506
0,2
40
So 7
2-7
40
945
5,i
5°
5°4
o,3
5°
780
2,8
5°
894
5,i
I
o
1,61 501
0,3
9
0
1,60 752
2,8
17
O
i.S8 843
5,2
IO
498
0,4
10
724
2,9
IO
791
5>2
20 1
494
0,5
20
695
2,9
20
739
5-2
3°
489
o,5
30
66b
3,°
3°
687
5-3
40 j
484
o,5
40
636
3,°
40
634
5-3
50
479
c,6
50
606
3,1
50
S81
5,4
2
o
1,61 473
0,6
10
O
1,60 575
3,2
x8
0
1,58 527
5,4
IO
467
0,7
10
543
3,2
10
4 73
5,4
20
460
0,8
20
5“
3,2
20
419
5,5
30
45 2
0,8
30
479
3,3
3°
364
5,5
40
444
0,9
40
446
3,3
40
3r9
5,6
50
435
0,9
50
413
3,4
50
253
5-7
3
O
i,6x 426
1,0
11
0
1,60 379
3,4
19
O
1,58 196
5,7
IO
416
1,°
10
345
3,4
10
139
5,7
20
406
1,1
20
311
3,5
20
082
5,8
30
395
i, 1
30
276
3,6
30
024
5,8
40
3*4
1,2
40
240
3,6
40
i,57 966
5,9
5°
372
1,2
50
204
3,7
5°
9°7
5,9
4
O
i,61 360
1,3
12
0
1,60 167
3,7
20
0
i,57 848
6,0
IO
347
1,4
10
130
3,7
10
788
6,0
20
333
1,4
20
093
3,8
20
728
6,0
3°
3i9
1,4
30
055
3,9
3°
668
6,1
40
305
1,5
40
016
3,9
40
607
6,1
50
290
1,5
50
i,59 977
4,o
50
546
6,1
5
0
1,61 275
1,5
13
0
i,59 937
4,o
21
0
i,57 485
6,2
10
260
1,6
10
897
4,1
10
323
6,2
20
244
1,7
20
856
4,1
20
361
6,3
30
227
1,8
30
815
4,2
30
298
6,4
40
209
1,8
40
773
4,2
40
234
6,4
SO
191
1,9
50
73i
4,2
50
170
6,4
6
0
1,61 172
1-9
14
0
1,39 689
4,3
22
0
i,57 i°6
6,4
10
153
1,9
10
646
4,3
10
042
6,5
20
134
2,0
20
603
4,4
20
1,56 977
6,5
30
114
2,I
30
559
4,5
30
912
6,6
40
093
2,1
40
5H
4,5
40
846
6,6
5°
072
2,2
50
469
4,6
50
780
6,7
7
O
1,61 050
2,2
15
0
1,59 423
4,6
23
0
1,56 713
6,7
IO
028
2,3
10
377
4,6
10
646
6,7
20
005
2,3
20
3 3i
4,7
20
579
6,8
3°
1,60 982
2,3
30
284
4,7
30
5“
6,8
40
959
2,4
40
237
4,8
40
443
6,8
50
935
2,5
50
189
4,8
50
375
6,9
8
O
1,60 910
16
0
i,59 141
24
0
11,56 3^6 TABLES.
Deg. Min.
Refrac-
tive
Index.
d
Deg. Min.
Refrac-
tive
Index.
d
Deg. Min.
Refrac-
tive
Index.
d
24
0
1,56 306
7,o
32
0
I.S2 570
8,6
40
0
1,48 168
9,7
10
236
7,o
10
484
8,6
10
071
9,7
20
166
7,o
20
398
8,6
20
1,47 974
9,7
30
096
7,i
30
312
8,7
30
877
9,7
40
025
7,i
40
225
8,7
40
780
9,7
50
i,55 954
7,i
50
138
8,7
50
683
9,7
25
0
i,55 883
7i
33
0
1,52 051
8,8
41
0
i,47 586
9,8
10
812
7,2
10
i,5i 963
8,8
10
488
9,8
20
740
7,2
20
875
8,8
20
390
9,8
30
668
7,3
30
787
8,8
3°
292
9,8
40
595
7,3
40
699
8,8
40
194
9,8
5°
522
7-4
50
611
8,9
5o
096
9,8
26
0
i,55 448
7 4
34
0
i,5i 522
8,9
42
O
1,46 998
9,8
10
374
7,4
10
433
9,0
10
900
9,9
20
3°°
7,5
20
343
9,0
20
801
9,9
30
225
7,5
30
253
9,o
30
702
9,9
40
150
7,5
40
163
9,o
40
603
9,9
5o
075
7,6
5°
0 73
9,o
5o
504
9,9
27
0
i,54 999
7,6
35
0
i,5o 983
9,1
43
0
1,46 405
9,9
10
923
7,6
10
892
9,i
10
306
9,9
20
847
7,7
20
801
9,1
20
207
9,9
3°
77 0
7,7
3°
710
9,i
30
108
9,9
40
693
7,8
40
619
9,2
40
009
10,0
5o
615
7,8
50
527
9,2
50
i,45 909
10,0
28
0
i,54 537
7,8
36
0
1,50 435
9.2
44
0
i,45 809
10,0
10
459
7,9
10
343
9,2
10
709
10,0
20
380
7,9
20
251
9.2
20
609
10,0
30
301
7,9
30
159
9,3
3°
509
10,0
40
222
7,9
40
066
9,3
40
409
10,0
5o
I43
8,0
50
i,49 973
9,3
50
3°9
10,0
29
0
1,54063
8,0
37
0
1,49 880
9,3
45
O
i,45 2°9
10,0
xo
i,53 983
8,1
10
787
9,4
10
109
10,0
20
902
8,1
20
693
9,4
20
009
10,0
30
821
8,x
3°
599
9,4
3°
i,44 9°9
10,0
40
740
8,2
40
505
9,4
40
809
10,1
5o
658
8,2
50
411
9,4
5o
708
10,1
3°
0
i,53 576
8,2
38
0
i,49 317
9,5
46
O
1,44 607
10,1
10
494
8,2
10
222
9,5
10
506
10,0
20
412
8,3
20
127
9,5
20
406
10,1
30
329
8,3
30
032
9,5
30
305
10,1
40
246
8,3
40
1,48 937
9,5
40
204
10 0
5o
163
84
50
842
9,6
50
104
10,1
31
0
i,53 °79
8,4
39
0
1,48 746
9,6
47
0
1,44 003
10,0
10
1,52 995
8,4
10
650
9,6
10
1,43 903
10,1
20
911
8,5
20
554
9,6
20
802
10,1
30
826
8,5
3°
458
9,6
30
701
10,1
40
74i
8,5
40
362
9,7
40
600
10,1
5o
656
8,6
50
265
9,7
5o
499
10,1
32
0
1,52 570
40
0
1,48 168
48
0
1,43 398 TABLES.
Deg. Min.
Refrac-
tive
Index.
d
Deg. Min.
Refrac-
tive
Index.
d
Deg. Min.
Refrac-
tive
Index.
d
48
0
'1,43 398
10,1
56
0
1,38 610
9,8
64
0
i,34 191
8,5
10
297
10,1
10
513
9,7
10
106
8,5
20
196
10,0
20
416
9,7
20
021
8,5
30
096
10,X
3°
319
9,7
30
i,33 936
8,4
40
1,42 995
10,1
40
222
9,7
40
8521
8,4
5o
894
10,1
5o
125
9,6
50
768
8,4
49
0
1,42 793
10,0
57
0
1,38 O29
9,6
65
0
1,33 684
8,3
10
693
10,1
10
i,37 933
9,6
10
601
8,3
20
592
10,1
20
837
9,6
20
518
8,2
3°
491
10,1
3°
741
9,6
30
436
8,2
40
39°
10,1
40
645
9,5
40
354
8,2
5o
289
10,1
5o
550
9,5
50
272
8,1
50
0
1,42 188
XO, I
58
0
i,37 455
9,5
66
0
i,33 191
8,1
10
087
10,0
10
360
9,5
10
no
8,1
20
1,41 987
10,1
20
265
9,5
20
029
8,0
3°
886
10,0
30
170
9,5
30
1,32 949
8,0
40
786
10,1
40
075
9,4
40
869
7,9
5o
685
10,1
50
1,36 981
9,4
50
790
7,9
51
0
1,41 584
10,0
59
0
1,36 887
9,3
67
0
1,32 711
7,9
10
484
10,1
10
794
9,3
10
632
7,8
20
383
10,0
20
701
9,3
20
554
7,8
30
283
10,0
30
608
9,3
30
476
7,7
40
183
10,0
40
515
9,3
40
399
7,7
5o
083
10,0
5o
422
9,3
5o
322
7,7
52
0
1,40 983
10,1
60
0
i,36 329
9,2
68
0
1,32 245
7,6
10
882
10,0
10
2 37
9,2
10
169
7,6
20
782
10,0
20
145
9,2
20
093
7,5
30
682
10,0
30
053
9,2
30
013
7,5
40
582
10,0
40
i,35 961
9,i
40
i,3i 943
7,4
5°
482
9,9
5o
870
9,i
5o
869
7,4
53
0
1,40 383
10,0
61
0
i,35 779
9,i
69
0
i,3i 795
7,4
10
283
10,0
10
688
9,o
10
721
7,3
20
183
9,9
20
598
9,0
20
648
7,3
30
084
9,9
30
508
9,o
3°
575
7,2
40
1,39 985
9,9
40
418
8,9
40
S03
7,2
50
886
9,9
5o
329
8,9
5o
43i
7,2
54
0
i,39 787
9,8
62
0
i,35 240
8,9
7o
0
1,31 359
7,i
10
689
9,9
10
iSi
8,9
10
288
7,o
20
590
9,9
20
062
8,8
20
218
7,o
3°
49i
9,9
30
i,34 974
8,8
30
148
7,o
40
392
9,8
40
886
8,8
40
078
6,9
5°
294
9,8
5o
798
8,8
5o
009
6,8
55
O
i,39 196
9,8
63
0
i,34 7io
8,7
7i
0
1,30 941
6,8
10
098
9,8
10
623
8,7
10
873
6,8
20
000
9,8
20
536
8,7
20
805
6,7
30
1,38 902
9,8
30
449
8,6
30
798
6,7
40
804
9,7
40
363
8,6
40
671
6,6
5o
707
9,7
50
2 77
8,6
5o
605
6,6
56
0
1,38 610
64
O
1,34 191
72
0
1,30 539 232
TABLES.
n2 I
TABLE FOR CALCULATING log. FROM THE REFRAC-
® n2 2
TIVE INDEX n ACCORDING TO CONRADY.
n2 I
log. —-o—. = o, . . . I.
& ;?2 -f- 2
n =
o
1
2
3
4
5
6
7
8
9
Diff.
Ap-
prox.
i,3°
2
7182
7315
7447
7579
7710
7841
7972
S102
8231
8360
131
i
8488
8616
8744
8871
8998
9124
9250
9375
9500
9625
127
2
9749,
9873
9996
*0119
*0241
*0363
*0485
*0606
0726
*0846
123
3
3
0966
1085
1204
1323
1441
1559
1676
1793
1909
2025
ns
4
2141
2256
2371
2486
2600
2714
2828
2941
3054
3166
114
5
3278
3390
35oi
3612
3723
3S33
3943
4053
4162
4271
1X0
6
4379
4487
4595
4703
4810
49*7
5023
5129
5235
534i
107
7
5446
555i
5656
5760
5864
5968
6071
6174
6277
6379
104
8
6481
6583
6684
6785
6886
6986
7086
7186
7286
738 s
100
9
74S4
7583
7681
7779
7877
7974
8071
8168
8265
8361
97
1,40
8457
8553
8648
8743
8838
8933
9027
9121
9215
9309
95
i
9402
9495
9588
9681
9773
9865
9957
*0048
*0139
*0230
92
2
4
0321
0412
0502
0592
0682
0771
0860
0949
1038
1127
90
3
1215
1303
1391
1479
1566
1653
1740
1827
1914
2000
87
4
2086
2x72
2258
2343
2428
2513
2597
2681
2765
2849
85
5
2933
3017
3100
3183
3266
3348
343°
3513
3595
36771
82
6
3758
3839
392°
4001
4082
4162
4242
4322
4402
4482
80
7
456i
4640
4719
4798
4877
4955
5033
Sin
5189
5267
78
8
5344
5421
5498
5575
5652
5728
5804
5880
5956
6032
76
9
6107
6182
6257
6332
6407
6482
6656
6630
6704
6778
75
i,5°
6852
6926
6999
7072
7145
7218
7291
7363
7435
7507
73
i
7579
7651
7723
7794
7865
7936
8007
8078
8x48
8218
7i
2
8288
8358
8428
8498
8567
8636
8706
8775
8844
8913
69
3
8981
9049
9118
9186
9254
9322
9389
9457
9524
959i
68
4
9658
9725
9792
9858
9925
9991
*0057
*0123
*0189
*02,55
66
5
5
0320
0385
0451
0516
0581
0645
0710
0774
0839
0903
65
6
0967
1031
1095
1158
1222
1285
1348
1411
H74
1537
63
7
1600
1663
1725
1787
1849
1911
1973
2035
2096
2158
62
8
2219
2280
2341
2402
2463
2523
2584
2644
2704
2764
61
9
2824
2884
2944
3003
3062
3122
3681
3240
3299
3357
60 TABLES.
2 33
TABLE OF EXTINCTION-COEFFICIENTS CORRESPONDING
TO THE DIFFERENT VALUES OF ,P ACCORDING
TO VIERORDT, ARRANGED BY G. KRUSS
u
g
h
2 w
H
Z
w
xf On i-h On co xh O irifON CM Tfvo N vD VO conO eo
H NO EO EO W~) EO V-O ET)VO VO CO O O
ON *H COED 00 conO 00 — conO 00 — conO 00 h
ro t*- rt IT) 1-0 ED idvO MD VO N IN NCO 00
ro co ro co ro co ro to ro ro fC fO fO rc ro ro ro ro ro
CM
CM
00
ro
iJ-UNO t)- ro N
ro NO NO ON O M
On M tx OnO
GO On O' On ON O
ro tn to toto rI-
M
CM
M
O
oh
•- m m m CM ro 'xJ-NO
ro tJ- eonO On O
CM ro Tf eonO O
OOOOOOOm
'xhoh’rt-Tt-Tf'rfr^-Tt-
IN
CnM t|-Nw
CM rt* EO NO CO
CM CO rt- vONO
*5-
ON
rt-
u
u
O 0
o
o
o
o
0
o
0
0
o
0 0
o o o d
d
o
d
O
o
o
d
o d
d
d
d
o
d
d'd
o
d
d
d
o
d
o d
o
s
GO eo co O 00
EO ET) EO EO Tt-
Tj- rj*
EO CO O CO EO
rf- to CO
Tt*
ro O OO EO n O CO
CO ro Cl M M N H
nt* Tf Tf- Tt
eo ro
M M
Tj-
O 00
M O
Tj-
NO ro O
O d O
•& •rf
On CO
ON On
ro ro
eo rj- ro cm i-i
On On Qn Qn On On Cn
ro rO ro ro ro ro ro
O Onoo EO Tt- ro CM
On CO 00 00 00 CO 00 CO 00
rO ro ro ro ro ro co ro ro
o o
o
o
o
o
o
o
o
o
o
0 d
o d d d
o
o
o
O
o
o
o
6 6
o
o
o
o
o
o d
d
d
o
o
d
d
o o
d
U
g
h
X
TION-
OEFFI-
h
Z
5
ONNHOOTfMHH*-
EOCO ro CM nO CM vO CM NO
On *-* fO ED N h N
LT) EO EO LO EO’O VO 'O VO
M W M C) N N M M N M
,26922
EOCO 0 CO 0 On ro rf m tJ- COCO O NO m OnnO NO nO CO
'O N N COCO EO o NO moo Th H- N H 00 EOM O l>» eo
m ro in N ON h eo 00 on M 00 m M ion Onh OO O
N n N N KX O) X X 00 On On On On O O O O O w m m m cm
CM CM CM CM CM CM CM CM