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 (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.] (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 () 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 ; (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 O i-x o irNNO NO NO tx lx txOO CO 00 On On On O N w rooo nonoO ONNONorONo 00 no rovO NO HNO H O MOO ro-rf-ONHNOOO r. EO O EO O EO O lO o EO O EO C EO o O On on00 00 NO eo eo nOnDnOnOnOnOnOnOnOnO O eo O EO O EO o eo O CO eo ro C 00 io co O 00 eo ro O OO eo Th ro co cm cm t-i >—( o O On on On On go oo oo OO' vo OOVOOOVOVOOVO EOEOEOEOEOLOEOEOEOEOEOEOEOEO O 0 o o 0 o o o o o 0 o o o o d o d o o o d d o o o d d d d d o o d d o' d d" d d 6 d Extinc- I Z E h OfcZ P !i! W co roco ro N N !>. CM 00 rO N M O 0 M M CM o o o o o 00 OO NO cm O N N\£HOW N O OnONH UN M OnNhv£) O NT) O OnunO W ND O unco O ro nt>00 O M n/goO rOfC't + 't>'UOUN vtnnO no nD no OOOOOOOOOOOOO On eo ro CM ro eo On eo CM m « ThOO Q eo m eo CM On NO row CNN O ro eo00 O rONO 00 *- On cm ion O N- 00 00 CO CON ON ON on o O O m OOOOOOOOOOOO'h-wm M rt eo ro CO NO t—( HH hM VH On NO M O ON CM w CM i- EO K On GO rj- O CM CM CO U o o o 0 o o O o o o 0 o o o o o d d d o o d o d d d o o d o o d d d o o d d o' d d cT 'S o o o o ONOO On O' CTn On o o >-n xf- ON ON o CO On O O O mO mO "lO ci m o On Onoo 00 ix Ixno o mini- fO ro N N m — o O ON ON OnOO oooooooooooooooooooooooooooooooooooooo EO O EO O On ONOO GO n- EO o EO O N- t'-'.NO NO NT) O no o no no tJ- rh NNNN 6 o o o 0 o o o o o 0 o o d d o o o o o d o o d o o o o o o o o d o o o o d d d o o' J' Extino TION- COEFFI- CIENT. J' Extino TION- COEFFI- CIENT. J' Extino TI ON- COEFFI- CIENT. Extino TION- COEFFI- CIENT. 0,381 0,41908 °>333 o,47756 0,285 0,54516 0,237 0,62526 0,380 0,42022 0,332 0,47887 0,284 0,54669 0,236 0,62709 0,379 0,42137 o,33i 0,48018 0,283 0,54822 0,235 0,62894 0,37^ 0,42251 o,330 0,48149 0,282 0,54976 0,234 0,63079 o,377 0,42366 0,3291 0,48281 0,281 0,55130 0,233 0,63265 0,376 0,42482 0,328 0,48413 0,280 0,55285 0,232 0,63452 o,375 0,42597 0,327 0,48546 0,279 0,55440 0,231 0,63639 0,374 0,42713 0,326 0,48679 0,278 o,55596 0,230 0,63828 0-373 0,42830 0,325 0,48812 0,277 o,55753 0,229 0,64017 0,372 0,42946 o,324 0,48946 0,276 o,559io 0,228 0,64207 0,371 0,43063 0,323 0,49080 0,275 0,56067 0,227 0,64398 o,37o 0,43180 0,322 0,49215 0,274 0,56225 0,226 0,64590 0,369 0,43298 0,321 0,4935° 0,273 0,56384 0,225 0.64782 0,368 0,43416 0,320 0,49485 0,272 0,56544 0,224 0.64976 0,367 o,43534 °;3I9 0,49621 0 271 0,56704 0,223 0,65170 0,366 0,43652 0,318 0,49758 0,270 0,56864 0 222 0,65365 0,365 0,4377! 0,317 0,49895 0,269 0,57025 0,221 0,65561 0,364 0,43890 0,316 0,50032 0,268 0,57187 0,220 0,65758 0,363 0,44010 0,315 0,50169 0,267 o,57349 0,219 0,65956 0,362 0,44130 0,314 0,50308 0,266 o,575i2 0,218 0,66155 0,361 0,44250 o>3T3 0,50446 0,265 0,57676 0,217 0,66355 0,360 0,4437° 0,312 0,50585 0,264 0,57840 0,216 0,66555 o,359 0,44491 0,311 0,50724 0,263 0,58005 0,215 0,66757 o,358 0,44612 0,310 0,50864 0,262 0,58170 0,214 0,66959 0,357 0,44734 0,309 0,5x005 0,261 0,58336 0,213 0.67163 0,356 0,44855 0,308 o,5H45 0,260 0,58503 0,2X2 0,67367 0,355 0,44978 0,307 0,51287 0,259 0,58671 0,211 0,67572 o,354 0,45100 0,306 0,51428 0,258 0,58839 0,210 0,67779 0,353 0,45223 0,305 o,5i57i 0,257 0,59007 0,209 0,67986 0,352 0,45346 0,304 0,51713 0,256 0,59176 0,208 0,68194 o,35i o,4547o 0,303 0,51856 0,255 0,59346 0,207 0,68403 o,35o 0,45594 0,302 0,52000 0,254 o,595i7 0,206 0,68614 o,349 o,457i8 0,301 0,52144 0,253 0,59688 0,205 0,68825 0,348 0,45843 0,300 0,52288 0,252 0,59860 0,204 0,69037 o,347 0,45968 0,299 o,52433 0,251 0,60033 0,203 0,69251 0,346 0,46093 0,298 o,52579 0,250 0,60206 0,202 0,69465 o,345 0,46219 0,297 0,52726 0,249 0,60381 0,201 0,69681 o,344 0,46345 0,296 0,52871 0,248 0,60555 0,200 0,69897 o,343 0,46471 0,295 0,530x8 0,247 0,60731 0,199 0.70115 0,342 0,46598 0,294 0,53166 0,246 0,60907 0,198 0.70334 o,34i 0,46725 0,293 0,53314 0,245 0,61084 0,197 0,70554 0,340 0,46853 0,292 0,53462 0,244 0,61262 0,196 0,70775 o,339 0,46981 0,291 o,536h 0,243 0,61440 0,195 0.70995 0,338 0,47109 0,290 o,5376i 0,242 0,61619 0,194 0,71220 o,337 0,47238 0,289 °,539I9 0,241 0,61799 O.I93 0.71445 0,336 0,47367 0,288 0,54061 0,240 0,61979 0,192 0,71670 o,335 0,47496 0,287 0,54212 0,239 0,62161 0,191 0,71897 o,334 0,47626 0,286 0,54364 0,238 0,62343 0,190 0.72125 234 TABLES TABLES 235 J' % Extinc- TION- COEFFI- CIENT. J' Extinc- TION- COEFFI- CIENT. J' Extino TION- COEFFI- CIENT. J' Extinc- TION- COEFFI- CIENT. 0,189 0,72354 0,145 0,83864 0,102 0,99140 0059 1,22915 0.188 0.72585 0,144 0,84164 0,101 0,99568 0,058 1,23658 0.187 0 728x6 0,143 0,84467 0,100 1,00000 0,057 1,24413 0,186 0,73049 0,142 0,84772 0,099 1,00437 0,056 1,25182 0.185 0,73283 0.141 0,85079 0,098 1,00878 0,055 1,25964 0,184 0.73519 0,140 0,85388 0,097 1,01323 0,054 1,26761 0 183 o,73755 o,i39 0,85699 0,096 1,01773 i ,02228 0,053 1,27573 1,28400 0 182 o,73993 0,138 0,86013 0,095 0,052 0,181 0.74233 0,137 0,86328 0,094 1,02688 0,051 1,29243 0,180 o,74473 0,136 0,86647 0,093 1,03152 0,050 1,30103 0,179 o,747'5 0.135 0,86967 0,092 1,03622 0,049 1,30981 0,178 0,74958 o,i34 0,87290 0,091 1,04096 0,048 1,31876 0,177 0,75203 o,i33 0,87615 0,090 1,04546 0,047 1,32719 0,176 o,75449 0,132 0,87943 0,089 1,05061 0,046 1,33725 0,175 0,75697 0,131 0,88273 0,088 1,05552 0,045 1,34679 0 174 0.75946 0,130 0,88606 0,087 1,06094 0,044 1,35655 0,173 0,76196 0,129 0,88942 0,086 i,o65<;i 0,043 1,36654 0.172 0.76448 0,128 0,89279 0,085 1,07059 0,042 1,37676 0,171 0.76701 0,127 0,89620 0,084 ',07573 0,041 1,38722 0.170 0,76956 0,126 0,89963 0,083 1,08093 0,040 i,39794 0,169 0 77212 0,125 0,90309 0,082 1,08619 0,039 1,40894 0,168 o,7747o 0,124 0,90658 0,081 1,09152 0038 1,42022 0,167 o,77729 0,123 0,91010 0,080 1,09692 0,037 1,43180 0 166 0,77990 0,122 0,91365 0,079 1,10238 0,036 i,4437o 0,165 0.78252 0,121 0,91722 0,078 1,10791 0,035 1,45594 0,164 0,78516 0,120 0,92082 o,o77 1*35r 0,034 1,46853 0 163 0,78782 o,i 19 0,92446 0,076 .1,11919 0.033 1,48149 0,162 0.79049 O.IlS 0,92812 0,075 1,12494 0,032 1,49485 0,161 0 79318 0,117 0,93182 0,074 1,13077 0.031 1,50864 0.160 0,79588 0,116 o,93555 0,073 1,13668 0030 1,52288 0,159 0,79861 0,115 o,9393i 0,072 1,14267 0,029 i,5376i 0 158 0,80135 0,114 0,94310 0,071 1,14875 0,028 1,55285 0.157 0,80411 0,113 0,94963 0,070 1,15491 1,16116 0,027 1, c; 6864 0,156 0,80688 0,112 0,95079 0,069 0,026 1,58503 0.' 55 0,80967 0,1 II 0,95468 0,068 1,16750 0,025 1,60206 0,154 0 81248 0,110 0,95861 0,067 i,i7393 0,024 1,61979 o,i53 0,81531 0,109 0,96258 0,066 1,18046 0023 1,63828 0,152 0,8x816 O.IoS 0,96658 0,065 1,18709 0,022 1,65758 0.151 0,82103 0,107 0,97062 0,064 1,19382 1,20066 0,021 1,67779 0,150 0,82391 0,106 o,9747o 0,063 0,020 1,69897 0,149 0,82682 0.105 0,97882 0,062 1,20761 0,015 1,82391 0,148 0,82974 0,104 0,98297 0,061 1,21468 0,010 2,00000 0.147 0.146 0,83269 0,83565 0,103 0,98719 0,060 1,22185 0 005 2,30103 236 TABLES. CORRECTION TABLE FOR THE PROJECTING THREAD OF MERCURY IN A STANDARD THERMOMETER OF JENA GLASS ACCORDING TO RIMBACH. o—ioo° graduated in 0. Length of degree, about 4 mm. ; t observed temperature ; t° temperature of the surrounding air ; n number of degrees through which the thread projects. = 30 Oo Ln 40 45 So i 55 60 65 70 75 80 85 n = 10 0,04 0,04 0,05 0,0 n 0,05 i 0,06 0,06 0,07 0,08 0,09 0,10 0,10 20 0,12 0,12 0,13 0,14 0,15 0,16 0,17 0,18 0,19 0,20 0,22 0,23 30 0,21 0,22 0,23 0,24 0,25 0,25 0,27 0,29 0,31 o,33 o,35 0 37 40 0,28 0,29 Q.31 o.33 o,35 1 0,37 o,39 0,41 o,43 o,45 0,48 0,51 50 0,36 0,38 0,40 0,42 0,44 | 0,46 0,48 0,50 o,53 o,57 0,61 0,6s 60 0,45 0,48 0,51 o,53 o,55 0,57 0,60 0,63 0,66 o,6q o,73 0,78 70 — — — — — 0,66 0,69 °,71 o,75 0,81 0,87 0,92 80 — — — — 0.76 0,81 0,87 o,93 1,00 1,06 90 — — — — — 0,92 0.99 1,06 i,'13 1,20 100 — — — — 1 — — — 0,10 x,i8 1,26 i,34 Tables for thermometers of Jena glass from o 360°, see Rimbach, Ber. d. d. chem. Ges. 22, p. 3074, 1889. INDEX. ABBE, refractometer, x6B Absorption, coefficient of, 57 heat of, 138 spectra, 187, 193 Andrews, spec, heat determination, 120 Araometer, 27 Atomic weights, table of, 226 Axial angle of crystals, 166 Crystals, measurement of, 166 Crystal-float method, 17 DENSITY, 13 of gases, 32 of liquids, 19 of solids, 14 Depression of the freezing point, 8l Dielectric constant, 75, 182 Diffusion, 57 Dilation, 31 Dilution, heat of, 139 Direct-vision spectroscope, 183 Dispersion, 171, 183 Double refraction in crystals, 164 Drop method, 49 Dumas, vapor den. determination, 32 BALANCE, chemical, 9 Barometer, 224 Beckmann, depression of freezing point, 81 97. 103 thermometer, 218 Berthelot, heat of combustion, 14X Boiling point, 90 elevation of boiling point, elevation of, 97 Bomb, calorimetric, 141 Bunsen spectroscope, 183 ice-calorimeter, 121 ELECTRIC conductivity, 58 Electro magnetic rotation, 214 Electromotive force, 72 Elevation of the boiling point, 97 Emission spectra, 187 Expansion, coefficient of, 76 Extinction-coefficient, 194 CALIBRATION of a wire, 73 of a capillary tube, 46 of a thermometer, FORMATION, heat of, 152 Freezing point, depression of, 81 Fusion, heat of, 126 Calorie, 109, 132 Calorimeters, 112, 119, 121, 134 Capillarimeter, 46 Capillarity, 45 Capillary electrometer, 71 Cathetometer, 216 GLAN, polarization spectrophotome ter, 200 Chemical equilibrium, 57 Combustion, heat of, 141 Conductivity, electric, 58 molecular, 69 Contraction, 31 Goniometer, 153 HEAT of combustion, 141 of dilution, 139 of formation, 152 of fusion, 126 Convergent light, 165 Critical pressure, 97 temperature, 97 of hydration, 140 of neutralization, 133 INDEX Heat of precipitation, 138 of solution, 137 of vaporization, X 29 Hofmann, vapor density, 34 Hiifner polarization spectrophotome- Reaction velocity, 57 Refraction, index of, 168 atomic, 178 molecular, 178 specific, 178 Refractometer, 168, 172 Regnault-Pfaundler, specific heat, 115 Rotation of the plane of polarization, ter, 200 Hydration, heat of, 140 Hydrostatic balance, 19, 25 ICE-CALORIMETER, 121 electro-magnetic, 214 Rotatory power, molecular, 203 specific, 202 lons, velocity of, 71 Isomorphism, 167 JONES-SCHLEIERM ACHER, boiling-point determination, 93 SCHIFF, specific heat, 117 Siwoloboff, boiling point, 93 Solidifying point, 79 Solubility, 56 Solution, heat of, 137 Specific gravity, 13 Specific heat, 109 of liquids, 117 of solids, ill Spectrophotometer, 193, 200 Spectroscope, 182, 183, 189 Spectrum analysis, 182 Stalagmometer, 49 Stauroscope, 167 Strouhal and Barns, calibration of a KOHLRAUSCH, electric conduc- tivity, 58 Kopp, specific heat, Ix 7 Kriiss, spectroscope, 189 LAURENT, half-shadow apparatus, 211 Lippich, half-shadow apparatus, 214 Lunge and Neuberg, vapor density, 41 MELTING point, 79 Meyer, V., vapor density, 38 Micropolaris'cope, 160 Mitscherlich, polarimeter, 207 Mohr-Westphal, balance, 24 Molecular refraction, 178 volume, 28 wire, 73 THERMOCHEMICAL constants, _ 134 Thermometer, 218 Thermostat, 65 Transport numbers, 71 OSMOTIC pressure, 57 PASTILLE press, 149 Poiseuille-Oslwald, viscosity determina- VAPOR density, 32 pressure, 90 Vaporization, heat of, 129 Vernier, 215 Vibration, directions of. in crystals, 164 Vierordt, spectrophotometer, 193 Viscosity, constant of, 53 tion, 53 Polarimeter, 207, 211, 214 Polaristrobometer, 209 Pressure regulator, 95 Pulfrich, refractometer, 172 Pyknometer, 14, 19 WATER-EQUIVALENT, no, RAABE turbine, 66 Radiation, 115 113 Wild polaristrobometer, 209 Wollaston, goniometer, 153 Raoult, depression of freezing point, 79