C2H5

\

C(SO2C2H5)2

/

C2H5

Tetronal.

Sulphonal is prepared by the oxidation of a substance obtained by

the combination of acetone and ethylmercaptan. _Veronal_ is an ethyl

compound of barbituric acid, obtained by the condensation of urea and

diethyl malonyl chloride:

NH.CO

/ \

CO C(C2H5)2

\ /

NH.CO

Veronal.

Attempts have been made to connect the physiological working of local

anæsthetics with particular constitutional groupings, as, for example,

in cocaïne; and these have led to the introduction of such substances

as the _orthoforms_, _nirvanine_, _stovaïne_, _alyhine_, _novocaïne_,

and _adrenaline_ into medicine. Adrenaline, used in conjunction with

cocaïne, has proved itself a most valuable agent in producing what is

called _lumbal anæsthesia_, whereby large sections of the lower half

of the body may be rendered completely insensitive to pain.

The study of the putrefactive changes of albuminous substances of

animal origin, induced by the activity of micro-organisms, has revealed

the existence of a number of basic nitrogenous compounds, some of

which are highly poisonous. These were classed by Selmi under the

generic name of _ptomaines_ (πτῶμα, a corpse). Brieger found that the

typhoid bacillus yielded a poisonous substance—_typhotoxine_, and that

the bacillus of tetanus forms a highly toxic basic body, _tetanine_.

All the ptomaines, however, are not poisonous. Some of them, like

_choline_ (χυλὴ, bile)—originally discovered by Strecker in bile, in

the brain, in yolk of egg, and now found to be among the products of

the putrefaction of meat and fish—have been known for some time past.

Choline was first synthetically prepared by Wurtz. _Neurine_ (νεὺρον,

nerve), a derivative of brain substance, is related to choline, and

is readily transformed into it, but differs from it in being very

poisonous. It has been synthesised by Hofmann and by Baeyer. Another

of the so-called corpse-alkaloids—_cadaverine_—has been synthetically

formed by Ladenburg. Schmiedeberg and Kopp isolated the poisonous

principle of the fungus _agaricus muscarius_, which they named

_muscarine_. It occurs with choline, from which it can be readily

obtained, among the products of the putrefaction of flesh, as well as

in many fungi.

The synthesis of the alkaloids _conine_, _atropine_, _cocaïne_,

_piperine_, and _nicotine_ has been already referred to[5] as also that

of _vanillin_, the aromatic principle of the dried fermented pods of

certain orchids; _coumarin_, the odoriferous principle of woodruff and

of the tonka bean; of _salicylic acid_, _oil of wintergreen_, _oil of

mustard_, _bitter-almond oil_, and _camphor_. _Acetic_, _succinic_,

_tartaric_, and _citric acids_ have also been artificially obtained,

and may, indeed, be built up from their elements.

[5] P. 133.

No synthesis of recent years created more widespread interest than that

of _alizarin_, first effected by Graebe and Liebermann in 1868. Its

successful commercial manufacture by Sir William Perkin in this country

and by Caro in Germany created nothing less than a revolution in one

of our leading industries, and completely destroyed a staple trade of

France, Holland, Italy, and Turkey. To procure alizarin, anthraquinone

is treated with sulphuric acid, and the product is fused with alkali

and potassium chlorate.

The remarkable industrial results attending the synthetical formation

of this madder-product naturally led to attempts to procure other

important vegetable dye-stuffs artificially, notably _indigo_.

The synthetical production of indigo has been accomplished by

the joint labours of many chemists, notably Baeyer, Heumann, and

Heymann, and the substance is now prepared on an industrial scale.

The starting-point is _naphthalene_, obtained from coal-tar. This

is converted into _phthalic acid_, which is then transformed into

_phthalimide_. The last-named substance is converted into _anthranilic

acid_, which, on treatment with monochloracetic acid, is changed into

_phenylglycin_-ortho-_carbonic acid_. On melting this with caustic

potash it yields _indoxyl acid_, which is transformed into _indoxyl_,

and thence into _indigo_.

Another method is to treat the sodium salt of phenylglycin with

sodamide, whereby _indoxyl_ is at once obtained, and this by

condensation yields _indigo blue_:

C6H5.NH.CH2.COONa + Na.NH2

Sodium salt of Sodamide.

phenylglycin.

CO

/ \

→C6H4 CH2

\ /

NH

Indoxyl.

CO CO

/ \ / \

→C6H4 C:C C6H4

\ / \ /

NH NH

Indigo blue.

Phenylglycin is obtained by the action of monochloracetic acid

on aniline, which in its turn is obtained through nitrobenzene

from benzene. Since benzene can be synthetically prepared by the

condensation of acetylene, which can be obtained by the direct union of

carbon and hydrogen at a high temperature, it is theoretically possible

to build up indigo blue from inorganic materials.

Synthetical indigo blue was placed on the market in 1897 with an

almost immediate effect on the production and price of the natural

variety, and to-day the output of Bengal indigo has fallen by more

than fifty per cent. In 1902 the amount of the natural product was

probably not greater than three million kilos, whereas in the same

year the production of synthetic indigo was upwards of five million

kilos. Before the introduction of the artificial variety the price of

pure indigo blue ranged from sixteen to twenty shillings per kilo; by

the end of 1905 it had fallen to seven or eight shillings. Mention

should be made also of _thio-indigo red_ and the _thionaphthene_

derivatives, some of which promise to be important colouring matters.

In recent years the so-called _sulphur colouring matters_ have acquired

considerable importance. Space will not permit of any fuller treatment

of the development of the manufacture of the artificial organic

colouring matters. This industry had its beginnings in England, but it

is now mainly carried on in Germany. Its importance may be gleaned

from the fact that the value of the production at the present time

amounts to not less than £12,500,000 per annum, two thirds of the

output being exported. It demands the services of battalions of skilled

chemists, and gives employment to many thousands of artisans.

Some of the most notable achievements of modern synthetical chemistry

are to be found in the work of Emil Fischer on the _sugars_ and the

_proteins_. Although the sugars have from the earliest times been

reckoned among the most characteristic products of plant life, and have

long been used as food and as sources of alcohol, comparatively little

was known until lately of their real nature and mutual relations,

in spite of numerous attempts to elucidate their constitution. Much

of the mystery surrounding their chemical history has now been

dispelled. Not only has the molecular structure of the more important

naturally occurring sugars been unravelled, but a large number of

hitherto unknown members of the various groups of the great family

to which they belong have been prepared. The first insight into the

constitution of these bodies may be said to date from the researches

of Kiliani, made about a quarter of a century ago. In 1887 Fischer

effected the synthesis of a form of fructose (fruit sugar), and

immediately afterwards of ordinary dextro-glucose (grape sugar) and

its enantiomorph lævo-glucose, and the two optically active forms

of natural fruit sugar. Since that time such sugars as arabinose,

xylose, fucose, mannose, sorbose, cane-sugar, maltose, lactose, etc.,

and the sugars existing as glucosides, have been examined, their

stereo-chemical relations defined, and synthetic methods of production

devised. Incidentally, their behaviour towards enzymes has been

studied, and the remarkable selective action of these ferments on the

various groups, due apparently to differences of configuration, has

been established, with the result that much light has been thrown

on the mechanism of enzyme action and on the general theory of

fermentation.

[Illustration: EMIL FISCHER.]

The study of the proteins by Fischer constitutes a new chapter in

bio-chemistry. Although long recognised as among the most important

of vital products, from the circumstance that they enter into the

composition of animal tissues and secretions and are essential

constituents of protoplasm, the proteins are among the worst defined

substances known to the chemist. They are difficult to separate, as

they closely resemble one another, and afford no certain indications of

individuality. Very few of them have been obtained in a form in which

their identity could be established. _Oxyhæmoglobin_ was isolated some

years ago, but the proteins of serum albumin and of egg albumin have

only recently been obtained in definite crystalline shape. All the

proteins—even the simplest of them—are of great complexity, and possess

apparently very high molecular weights. _Hæmoglobin_, for example,

appears to have approximately the formula C158H123N195O218FeS3, with

a minimum molecular weight of 16,600. Indeed, there is experimental

evidence to show that it is even considerably higher than this.

The main clues to the nature of these substances have been gained by

the systematic study of their hydrolysis, induced by reagents, or

by the action of enzymes, whereby they are found to break down into

proteoses, peptones, and a great variety of amino acids, some of which

have been synthesised. Among the proteins of simplest constitution are

the _protamines_, found in the spermatozoa of fish. They are basic

substances, especially rich in nitrogen, forming salts with platinum

chloride and certain metallic oxides. The best investigated member of

the group is _salmine_, obtained from the testicle of the salmon. The

products of its hydrolysis have been fairly well ascertained, and their

quantitative relation is such that the substance must have at least a

molecular weight of 2045, corresponding to the formula C81H155N45O18.

Many of the albumins and globulins—coagulable proteins contained in the

animal tissues—have been isolated in a more or less definite form, and

some of them have been found to yield substances akin to carbohydrates.

_Thyreoglobulin_, the globulin of the thyroid gland, has been found to

contain iodine, apparently as a normal constituent of a body which can

be isolated as a definite proximate principle. The presence of this

element is possibly connected with the curative value of the globulin

in crétinism. A considerable amount of work on the vegetable albumins

has also been done of late years; and some of them, as _edestin_ from

hemp seed and _zein_ from maize, have been obtained in definite form.

The limits of this work preclude a more detailed account of one of

the most interesting but at the same time one of the most obscure

departments of chemistry. The field has hitherto been tilled in a

somewhat intermittent and partial manner. Now that it has been entered

by chemists of experience and resourcefulness, armed with modern

methods of cultivation, it will doubtless soon yield a rich harvest of

facts, valuable alike to the physiologist and the physician.

There can be no reasonable doubt that the chemical processes of organic

life are essentially similar to those of the laboratory. The doctrine

that a special “vital force” is concerned in the production of vital

products receives no support from the teaching of modern science,

and is, indeed, contradicted by it. At the same time, it must be

admitted that we know very little as yet of the real agencies at work

in the elaboration and mutations of chemical products in the living

organism. Because we have effected the putting together of such a

product by purely laboratory processes—it may be, indeed, by a variety

of different and dissimilar processes—it by no means follows that

any one of them is identical with that actually occurring in nature.

The building up of materials in the plant by the agency of light,

for example, has not yet been imitated in the laboratory. Many plant

products are produced by the action of unorganised ferments—so-called

enzymes—none of which the chemist has succeeded in creating.

Processes akin to condensation undoubtedly occur in the living

organism; but the means by which they are effected are, in all

probability, very different from anything known to the chemist at

present. Many laboratory condensations are only accomplished at

relatively high temperatures or under considerable pressure—or, in

other words, under totally different conditions from those which obtain

in the organism.

CHAPTER XI

ON THE DEVELOPMENT OF PHYSICAL CHEMISTRY SINCE 1850

Chemistry and physics are each complementary to the other: that region

of inquiry in which they mutually overlap is known as _physical

chemistry_. Its beginnings are practically contemporaneous with those

of chemistry itself. Its main development has occurred, however, during

the last twenty-five years. Certain of its leading features have

been referred to already in connection with the establishment of the

fundamental principles of chemistry, the explanation of the so-called

gaseous laws, the constitution of gases, the relations of their volumes

to heat and pressure, and the conditions affecting their transition to

the liquid state.

As regards the molecular volumes of gases it has been shown that

simple relations are obtained when quantities represented by their

respective molecular weights are compared under identical conditions of

temperature and pressure—that is, under circumstances in which equal

numbers of molecules form the basis of comparison. The investigation

of the molecular volumes of liquids is complicated by the uncertainty

as to what constitutes in their case a valid condition of comparison.

Kopp’s assumption that a comparable condition was the temperature

at which the vapour pressures of the liquids are equal to the mean

atmospheric pressure was justified by the fact that the boiling-points

of liquids are approximately two thirds of their respective critical

temperatures. His conclusions have been confirmed and extended by

Lossen, Thorpe, and Schiff. It has been shown that the molecular

volume of a liquid—that is, the product of its relative density at the

boiling-point into its molecular weight—is in the main an additive

function modified by constitutive influences. Definite values have

thus been obtained for a number of the elements from a comparison of

homologous or similarly constituted compounds; and in certain cases

these are found to be practically identical with the values of the

elements in the uncombined state.

Considerable light has been gained during the last two decades

concerning the nature of _solution_. In its most comprehensive sense

solution means the homogeneous mixture of two or more substances: thus

the gases which exert no chemical action on each other are mutually

soluble; gases, liquids, and solids may be soluble in liquids; and,

lastly, solids maybe soluble in solids, forming what are known as

_solid solutions_. The mutual solubility of gases was studied by Dalton

who enunciated the _law of partial pressures_, which states that the

total pressure of a mixture of gases is the sum of the pressures

exerted by the individual components. This, like all the so-called

gaseous laws, is necessarily not strictly accurate under ordinary

conditions, but approximates to truth in proportion as the gases are

rarefied. Van ’t Hoff pointed out that the true partial pressures of

the components of a gaseous mixture might be experimentally ascertained

by the use of a membrane capable of effecting their separation, and on

this principle Ramsay measured the partial pressures of a mixture of

hydrogen and nitrogen contained in a palladium vessel connected with

a manometer. The palladium, at a sufficiently high temperature, is

permeable to hydrogen to the exclusion of the nitrogen. The conditions

affecting the solubility of gases in liquids were experimentally

studied by Dalton and Henry, and what is known as Henry’s law implies

that the volume of a gas dissolved by a definite volume of a liquid

is independent of the pressure; or, in other words, the density

(concentration) of the gas in solution is proportional to that in

the space above the liquid. Gases are dissolved by liquids in very

different amounts, but nothing definite is known as yet concerning the

relation between the nature of the gas and its solubility, although

certain broad generalisations are possible. Thus neutral gases—_e.g._,

hydrogen and nitrogen—are sparingly soluble, whereas gases which

show acidic or basic properties, such as the hydrogen halides, etc.,

ammonia, etc., are freely soluble. Easily liquefiable gases are also

comparatively soluble as noted by Graham.

Comparatively little is known definitely concerning the conditions

of solubility of liquids in liquids. Some liquids are wholly, others

partially miscible; and temperature and pressure appear to affect the

proportions in which the components form a homogeneous mixture. As

regards the solubility of solids in liquids, our knowledge is more

extensive, and a considerable body of literature exists on the subject,

chiefly concerning solubility of solids in water. The solubility of

a solid depends on the temperature of the solvent, and, as a rule,

increases with the temperature until a certain amount of the solid

has been dissolved, when the solution is said to be _saturated_. If

the clear saturated solution be slowly cooled, say, to a particular

temperature, it is frequently observed that more of the solid remains

in solution than is normal to that temperature; such a solution is

said to be _supersaturated_. On adding some of the solid to the

supersaturated solution the excess of the _solute_ is precipitated.

In certain cases of solubility of substances in water, increase of

temperature appears to diminish the amount dissolved. In nearly all

such cases the difference in solubility is due to differences in the

hydration of the solute. The phenomena of solid solutions have been

less perfectly investigated, but the facts appear to show that such

solutions in general tend to obey the laws regulating the solution of

liquids in liquids. Alloys may be looked upon as solid solutions; and

Roberts-Austen has shown that metals are capable of intradiffusion,

like liquids and gases respectively.

The general question of solution was greatly developed in 1885 by

Van ’t Hoff, by specially considering the case of dilute solutions. The

gaseous laws are capable of their simplest expression when the gases

are rarefied to such an extent that their molecules exert no sensible

mutual influence. The case of dilute solutions is analogous. If the

solute is present only in very small amount, the mutual influence of

its molecules is practically negligible. Under such conditions it obeys

the laws hitherto supposed to be applicable only to matter in the

gaseous state.

It may be desirable to explain how this fundamental fact was

recognised. It has long been known to the physiologist that certain

membranes are _semi-permeable_—that is, they allow of the passage of

certain liquids, and of substances in solution, to the exclusion of

others. This phenomenon is termed _osmosis_, and is of great biological

significance. It was first studied by plant-physiologists, notably by

Traube and Pfeffer. Many such semi-permeable membranes can be formed

artificially, but the most generally convenient is found to be one

consisting of copper ferrocyanide deposited on the walls of a porous

vessel.

If a vessel so prepared be filled with a solution of sugar, and be

then placed in water, the water is found to pass through the membrane,

but the membrane is impermeable to the sugar. In consequence pressure,

termed _osmotic pressure_, is found to occur within the pot, and may

be measured by suitable means. These osmotic pressures may at times be

very large: thus a 1 per cent. solution of sugar may exert a pressure

of half an atmosphere, and in the case of a solution of potassium

nitrate of the same concentration it may amount to a couple of

atmospheres.

Pfeffer determined the relation of the osmotic pressures to the

concentration of solutions of these substances, measuring the pressures

in centimetres of mercury by a manometer attached to the closed porous

vessel. His results in the case of sugar were as follows:

_Percentage _Pressure in cm.

strength (C)._ of mercury (P)._ _P/C._

1 53.5 53.5

2 101.6 50.8

4 208.2 52.1

6 307.5 51.3

It will be seen from these numbers that the ratio P/C is practically

constant—that is, _the osmotic pressure varies directly as the

concentration_. It was further found that the osmotic pressure exerted

by a solution of uniform strength increases with the temperature.

The importance, of these observations in relation to the general theory

of solution was first recognised by Van ’t Hoff. Osmotic pressure was

regarded by him as analogous to gaseous pressure. Since P/C is constant

for any one substance, and since for a definite weight of the solute

the concentration is inversely as the volume of the solution, we obtain

an equation analogous to the statement of Boyle’s law, PV = constant.

Van ’t Hoff also found that the _osmotic pressure is proportional

to the absolute temperature_, like the gaseous pressure. From these

results, in conjunction with Avogadro’s hypothesis, it follows that

_the osmotic pressure exerted by any substance in solution is the

same as it would exert if present as gas in the same volume as that

occupied by the solution, provided that the solution is so dilute that

the volume occupied by the solute is negligible in comparison with

that occupied by the solvent_. Another important consequence is that

_solutes, when present in the ratio of their molecular weights in equal

volumes of the same solvent, exert the same osmotic pressure_. Such

solutions are said to be _isomotic_ or _isotonic_. It can be proved by

thermodynamical reasoning that depression of the vapour pressure and

freezing-point of a solution is proportional to its osmotic pressure.

The significance of this relation in connection with the determination

of the molecular weight of a soluble substance has already been

referred to.[6]

[6] See pp. 70–73.

Determinations of molecular freezing-point depressions by Raoult

and others showed that certain substances exerted only about half

the osmotic pressure calculated from their known formulæ, whereas

others have abnormally high osmotic pressures. The explanation of

the discrepancies in the latter case was given in 1887 by Arrhenius,

who pointed out that _only those solutions which have abnormally

high osmotic pressures are electrically conductive_. This pregnant

observation proved to be very fruitful in suggestiveness; and the

connection between conductivity and Van ’t Hoff’s theory of solution

was developed by Arrhenius into the doctrine of _electrolytic

dissociation_ or _ionisation_—one of the most important consequences

of Faraday’s electrolytic laws, the work of Hittorf, and the kinetic

conceptions of Williamson and Clausius to which the last quarter

of a century has given rise. Arrhenius showed that not only were

free ions present in an electrically conductive solution before

electrolysis, as maintained by Clausius, but that the proportion of

molecules dissociated into ions could be calculated from measurements

of electrical conductivity, as well as from measurements of osmotic

pressure. Both methods give concordant results—a strong confirmation of

the validity of the theory. In a solution of common salt, containing a

gramme equivalent of that substance in a litre, Arrhenius calculated

that only about three tenths of the salt exists as NaCl, the remaining

seven tenths being resolved into independent ions of chlorine

(chloridion) and sodium (sodion): NaCl⇄[Na·] + Cl´, each moving freely

in all directions, like gaseous molecules. On passing the current,

electrodes placed in the solution exert a directive action on the free

ions, these alone being concerned in determining the conductivity, the

un-ionised molecules or the solvent itself exercising no influence.

Methods of determining the migration velocity of the ions have been

worked out by Hittorf, Kohlrausch, Lodge, and others.

[Illustration: SVANTE AUGUST ARRHENIUS.]

The theory of ionisation affords a satisfactory explanation of many

chemical phenomena. It accounts for the characteristic properties of

acids, and explains why different acids have varying “strengths” and

why a “weak” acid has the same “strength” as the “strong” acid at

high equivalent dilutions: in each case the acid is nearly completely

ionised—in other words, the “strength” of an acid depends on the

concentration of its hydrogen ions. So, too, the “strength” of a base

is related to the number of its hydroxyl ions. Aqueous ammonia is

relatively a “weak” base—its solution contains few hydroxyl ions. On

the other hand, caustic potash is a “strong” base—its solution, on

moderate dilution, is almost completely ionised: KOH = K· + OH´, the

positive ion being represented by one or more dots, and the negative

ion by one or more dashes. The theory accounts, too, for many phenomena

in analytical chemistry—such as why magnesia is precipitated by ammonia

only in the absence of ammonium chloride, and why sulphuretted hydrogen

throws down zinc sulphide in the absence of hydrochloric acid. It

also serves to explain many thermo-chemical facts observed by Hess,

Thomsen, and others, such as the fact that the heat of neutralisation

of the “strong” acids and bases is independent of their nature, and has

the uniform value of 13,700 calories, in agreement with the value, as

calculated by Van ’t Hoff, for the reaction H· + OH´ = H2O, deduced

from Kohlrausch’s measurements of the conductivity of water at varying

temperatures.

Certain phenomena relative to the effect of concentration (mass action)

in determining chemical change—many of which have been studied by

Ostwald and his pupils, as, for example, why two dilute solutions can

be mixed together without thermal disturbance; numerous hydrolytic

actions; the alkalinity and acidity of salts on solution; the behaviour

of the “indicators” in analysis; such phenomena as the precipitability

of common salt in aqueous solution by hydrogen chloride; the influence

of an excess of a precipitant; the varying behaviour of reagents; the

varying colour of salt solutions; the reason why water is formed in so

many reactions; why a potential difference occurs at the surface of

two electrolytic solutions, etc.—phenomena for the most part otherwise

unintelligible, are all capable of explanation by means of it.

Although, in the above statement, we have been mainly concerned with

aqueous solutions, it should be said that the theory of ionisation

is applicable to other solvents, organic and inorganic. Moreover,

it should be added, the theory has not been universally accepted as

accounting for all the phenomena of solution. Many substances form

definite hydrates which can be isolated, and it is a moot point

whether such hydrates are capable of existing in aqueous solution, as

contended by Mendeléeff, Pickering, Kahlenberg, Armstrong, and others.

Such hydrates are, however, unstable compounds, affected by temperature

changes, and dissociable on dilution in accordance with the law of

concentration (mass action). Further, there is evidence, largely based

on the work of Kohlrausch, H. C. Jones, and Lowry, to show that the

ions in aqueous solutions of electrolytes are themselves hydrated.

Limitations of space preclude further attempts to deal with the

development of physical chemistry during the last half-century, and

many important matters must remain practically unnoticed.

The subject of thermo-chemistry is mainly the creation of the last

half-century, elaborated by the labours of Hess, Andrews, Thomsen,

Favre and Silbermann, and Berthelot. The work of Wenzel and Berthollet

on the influence of molecular concentration on chemical change has

been greatly extended by Berthelot, Guldberg and Waage, Julius

Thomsen, Van ’t Hoff, Harcourt and Esson, and Le Chatelier; and the

theory of mass action and the nature of reversible processes are now

capable of definite expression, and can be proved independently by

thermo-dynamical and kinetic reasoning. The phenomena of catalysis

and the action of enzymes and of fermentation in general have

received attention from many investigators. The phenomena of gaseous

transpiration have been studied by Graham, Maxwell, and O. E. Meyer.

Thermal dissociation has been experimentally observed by Deville,

Troost, and others, and mathematically investigated by Willard Gibbs

and Van der Waals; and its analogy to electrolytic dissociation

has been established. The nature of gaseous explosions has been

investigated by Berthelot, Le Chatelier, Abel, and Dixon. Important

work has been done by Gladstone, Lorentz, Landolt, Nasini, Brühl,

and others, on the connection between the nature and constitution of

substances and their optical characters. Similar work has been done by

Sir William Perkin as regards their magnetic rotation, and by Thorpe

and Rodger with reference to their viscosity. The theory of phases,

originating with Gibbs and developed by Van der Waals and Roozeboom,

has been greatly extended. Sir J. J. Thomson and Sir J. Larmor have

elaborated an electrical theory of the atom. Barlow and Pope have

traced the relation between valency and volume, and the accurate

measurements of Groth and of Tutton have extended our knowledge of the

crystallographic relations of correlated substances.

Lastly, the whole subject of photo-chemistry, although originating with

the observations of Ingenhousz, Scheele, and Senebier, may be said

to have been studied only within our own time, notably by Bunsen and

Roscoe, Pringsheim, Pfeffer, Vogel, and Abney.

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Leipzig.

Meyer, O. E. _The Kinetic Theory of Gases._ Translated by R. E. Baynes.

Longmans, 1899.

Muir, M. M. Pattison. _History of Chemical Theories and Laws._ John

Wiley and Sons, New York, 1907.

Nernst, Walter. _Theoretical Chemistry._ Translated by C. S. Palmer.

Macmillan, 1895.

Ostwald’s _Klassiker der Exakten Wissenschaften_.

Pictet, Amé. _Vegetable Alkaloids._ Translated by H. C. Biddle. John

Wiley and Sons, New York, 1904.

Richter’s _Lexikon der Kohlenstoff Verbindungen_. Leopold Voss, Hamburg

and Leipzig.

Roscoe and Schorlemmer, _Treatise on Chemistry_. Macmillan.

Rutherford, E. _Radio-Activity._ Cambridge University Press, 1904.

Schorlemmer, Carl. _Rise and Development of Organic Chemistry._ Edited

by Arthur Smithells. Macmillan.

Schryver, S. B. _Chemistry of the Albumens._ Murray, 1906.

Soddy, F. _Radio-Activity._ The Electrician Printing and Publishing

Co., London, 1904.

Stas. _Recherches sur les Rapports réciproques des Poids Atomique,

1860–1865._

Stewart, A. W. _Recent Advances in Organic Chemistry._ Longmans, 1908.

Stewart, A. W. _Stereo Chemistry._ Longmans, 1907.

Thorpe, T. E. _Dictionary of Applied Chemistry._ Three vols. Longmans.

Thorpe, T. E. _Essays in Historical Chemistry._ Macmillan, 1902.

Travers, Morris W. _Study of Gases._ Macmillan, 1901.

Van ’t Hoff, J. H. _Arrangement of Atoms in Space._ Translated by A.

Eiloart. Longmans, 1898.

Walker, J. _Introduction to Physical Chemistry._ Macmillan.

Wurtz, Ad. _The Atomic Theory._ Translated by E. Cleminshaw. Kegan

Paul.

INDEX

Abel, 184

Abney, 185

Absolute zero, 97

Acetanilide, 159

Aceto-acetic ester, 148

Actinium, 59

Adrenaline, 160

Agurin, 158

Alizarin, 162

Alkaloids, 132

Allyl alcohol, 4

Alyhine, 160

Ammonium chloride, dissociation of, 66

Ampère, 62

Anderson, 133

Andrews, 70, 95, 183

Aniline blue, 4

Aniline purple, 4

Antimony, origin of name, 28

Antipyrin, 159

Argon, 43, 45, 46

Argyrodite, 37

Armstrong, E. F., 151

Armstrong, H. E., 183

Aromatic compounds, 121, 123

Arrhenius, 179, 180

Arsine-dimethyl, 20

Artiads, 116

Asymmetry, 141

Atmolysis, 84

Atomic value, 114

Atomic weight, determination of, 75

Atomicity, 114

Atropine, 135, 162

its synthesis 135

Australene, 130

Autoracemisation, 144

Avogadro, 62

his hypothesis, 63

Baeyer, 125, 129, 161, 163

Balard, 139

Baly, 129, 151

Bamberger, 147

Barbier, 154

Barlow, 184

Basarow, 157

Basicity, 16

Becquerel, Henri, 52

Behrend, 157

Benzene, 123

its constitution, 123 _et seq._, 128

Benzidam, 3

Berberine, 136

Bernoulli, Daniel, 82

Berthelot, Daniel, 82, 183, 184

Berthollet, 183

Berzelius, 63

Biot, 138

Bitter almond oil, 7

Blagden, Sir Charles, 72

Boisbaudran, Lecoq de, 36, 38, 39

Boltzmann, 83

Bone oil, 133

Boron, specific heat of, 71

Boyle’s law, 84–87

Brauner, 33

Bredt, 129, 130

Brieger, 161

Brühl, 149, 151

Bunsen, Robert W., 18, 34, 43, 185

Bunsen burner, 22

Cacodyl, 20

Cadaverine, 161

Cæsium, 21, 34

Caffeine, 157

Cahours, 4, 132

Cailletet, 96

Camphene, 131

Camphor, 130, 131, 162

Cannizzaro, Stanislao, 64, 79

Carbon, atomic weight of, 75

specific heat of, 71

tetravalency of, 115

Carbon carbonyl, 155

Carbon suboxide, 155

Carnelley, 108

Carnolite, 58

Cavendish, 43, 45

Cayley, 120

de Chancourtois, 102

Chloral hydrate, 159

Choline, 161

Cinchonine, 137

Clausius, 83, 179

Cleve, 38, 47

Cleveite, 47

Cocaïne, 136, 162

Codeine, 137

Coindet, 8

Collie, 49, 128

Condensation, 152

Conine, 162

Conservation of mass, law of, 78

Coumarin, 132, 162

Critical point, 94

Critical pressure, 95

Crookes, Sir William, 35, 40, 75

Curie, Marie, 55

Cyanic acid, 7

Cyanuric acid, 7

Debierne, 59

Decipium, 40

Delafontaine, 49

Demarçay, 30

Desch, 151

Deville, 184

Dewar, 71, 96, 127

Dexter, 157

Didymium, 40

Digitalis, 10

Disintegration theory, 54

Dixon, 184

Dobbie, 151

Doebner, 134

Dumas, Jean B. A., 8, 9, 30, 31, 63, 75, 102, 130

Duppa, 148

Dysprosium, 38

Edestin, 169

Electrolysis, 179

Elements, nomenclature of, 27

Emanation from Radium, 58

Emanium, 60

Enantiomorphism, 140

Enzymes, 144

Ether, discovery of its constitution, 12, 17

Etherin theory, 10

Europium, 39

Favre, 183

Fenton’s reagent, 154

Findlay, 151

Fischer, Emil, 158, 165, _et seq._

Fittig, 153

Fluorine, 33, 34

Formulæ, chemical, significance of, 68

Frankland, 114, 116, 148

Fuchsine, 4

Fumaric acid, 146

Gadolinium, 39

Gallium, 36, 107

Gases, kinetic theory of, 83

law of diffusion of, 84, 89

liquefaction of, 94

molecular theory of, 79

Gas-mantles, 40

Gay Lussac, 63, 80

Geometrical isomerism, 146, 147

Gerhardt, 79, 113

Germanium, 37, 107

Geuther, 148

Gibbs, Willard, 184

Giesel, 60

Gladstone, 30, 102, 184

Gmelin, 7, 63, 102

Gore, 33

Graebe, 162

Graham, Thomas, 2, 14, 23, 29, 83

Grignard’s reagent, 154

Groth, 184

Guldberg, 183

Guye, 81

Haarmann, 132

Hæmoglobin, 168

Hantzsch, 147

Hartley, 151

Haüy, 139

Heliotropin, 132

Helium, 43, 47, 49

Helmholtz, 117

Henry’s law, 173

Hermann, 26

Herschel, 140

Hess, 181, 183

Heumann, 163

Heymann, 163

Hillebrand, 47

Hittorf, 179

Hofmann, August W., 3, 67, 133, 161

Holmium, 38

Hoogewerff, 133

Horbaczewski, 157

Hübner, 127

Hydrogenium, 16

Hyoscyamine, 135

Ilmenium, 26

Indigo, 162, 164

Indigo blue, 163

Indium, 36

Ingenhousz, 185

Ionisation, 178

Ionium, 58

Ionone, 132

Irone, 132

Isoborneol, 131

Isoconine, 134

Isoquinoline, 133

Isotonic solutions, 178

Jones, H. C., 183

Jones, H. O., 147

Kahlenberg, 183

Kammerlingh Onnes, 49, 97

Kekulé, Friedrich August, 23, 113, 114, 121, 123, 125, 153

Kiliani, 165

Kipping, 147

Kirchhoff, 21

Knorr, 128, 151, 159

Koenigs, 133

Kohlrausch, 182, 183

Komppa, 129

Kopp, 172

Körner, 127

Krüss, 40

Krypton, 43, 50

Krystallin, 3

Kundt, 46

Laar, 149

Lactic acid, spatial representation of, 141

Ladenburg, 127, 134, 147, 161

Lamy, 35

Landolt, 78, 184

Langlet, 49

Larmor, Sir J., 184

Lauder, 151

Laurent, 79

Le Bel, 143, 147, 148

Leduc, 80, 81

Le Royer, 8

Leucol, 133

Liebermann, 162

Liebig, Justus von, 5

Linnemann, 127

Liquid diffusion, 16

Liquids, molecular volumes of, 172

Lossen, 172

Lowry, 151, 183

Low temperature research, 97, 39

Lutecium, 89

Magenta, 4

Magnus, 79

Maleic acid, 146

Mansfield, 3

Marignac, 39, 75

Mauve, 4

Maxwell, 83

Medlock, 3

Mellitic acid, 7

Membranes, semi-permeable, 176

Mendeléeff, 30, 102, 109, 183

Mercury forms a monatomic gas, 71, 92

Metaphosphoric acid, 14

Meyer Lothar, 103

Meyer, Victor, 67, 147

Mitscherlich, 63, 138

Moissan, 33

Molecule, integral, 62

Molecules, their number, 93

their size, 93

Monium, 40

Morley, 80

Morphine, 137

Mosander, 39

Multirotation, 145

Muscarine, 161

Muspratt, 4

Mutarotation, 145

Naphthalene, 163

Narceïne, 136

Narcotine, 136

Nasini, 184

Natanson, 157

Neodymium, 39

Neon, 43, 50

Neoytterbium, 38

Neurine, 161

Newlands, 102

Nicotine, 135, 162

Nilson, 37, 40, 107

Nirvanine, 160

Nitrogen compounds, stereo-isomerism of, 147

Novocaïne, 160

Odling, 30, 114

Oil of wintergreen, 162

Olszewki, 96

Opianic acid, 136

Organic synthesis, 152

Orthoforms, 160

Osmotic pressure, 176

Ostwald, 182

Oxyhæmoglobin, 167

Ozone, 70

its symbol, 70

Papaverine, 136

Partial pressure, law of, 173

Pasteur, 139

Peachey, 148

Pelopium, 26

Penny, 75

Periodic law, 101

Perissads, 116

Perkin, Sir William, 3, 129, 131, 132, 162

Pettenkofer, 30

Pfeffer, 176, 185

Phenacetin, 159

Phenylglycin, 163

Phosphorous oxide, molecular weight of, 73

Phosphorus pentachloride, 66

Phosphorus pentafluoride, 67

Phthalic acid, 163

Pickering, 183

Pictet, 96, 135

Pinene, 130, 131

Pinner, 135

Piperine, 134, 162

Plattner, 35

Playfair, 20

Pollucite, 35

Pope, 147, 184

Posselt, 135

Praseodymium, 38

Pringsheim, 185

Protamines, 168

Proteins, 165

Prout’s law, an illusion, 76

Ptomaines, 161

Pyridine, 133

Quinine, 137

Quinoline, 133

Racemic acid, 140

Racemism, 143

Radio-thorium, 60

Radium, atomic weight of, 58

discovery of, 55

disintegration of, 58

emanation, 58

extraction of, 55

Radium chloride, 57

Ramsay, Sir William, 44, 47, 173

Raoult, 72, 178

Rayleigh, Lord, 44, 81

Regnault, 43, 79, 88, 157

Reich, 36

Reimann, 135

Richards, Theodore, 77

Richter, 36

Rodger, 184

Roosen, 157

Roozeboom, 184

Rosaniline, 4

Roscoe, 21, 30, 117, 185

Rose, 26

Rotatory power, 144

Rubidium, 21, 34

Runge, 133

Rutherford, 59

Salicylic acid, 162

Salmine, 168

Samarium, 40

Sarcine, 157

Sarcolactic acid, 140

Saturated solutions, 174

Saussure, 43

Scandium, 37, 107

Scheele, 33, 140, 185

Schiff, 172

Schischkoff, 21

Schmidt, 83

Schmiedeberg, 161

Scott, 80

Selmi, 161

Senebier, 185

Sesquiterpenes, 129

Silbermann, 183

Silicon, specific heat of, 71

Skraup, 133

Solute, 175

influence of, on boiling-point, 71

on freezing-point, 71

on vapour pressure, 73

Sonstadt, 153

Soret, 70

Spectrum analysis, 21

Stas, 75

Steric hindrance, 151

Stovaïne, 160

Strecker, 102, 158, 161

Sugars, 165

Sulphonal, 159

Supersaturated solutions, 174

Tait, 70

Tautomerism, 149

Terebenthene, 130

Terpenes, 129

Tetanine, 161

Tetronal, 159

Thallium, 35

Thebaine, 137

Thénard, 43

Theobromine, 157

Thioacetic acid, 127

Thomsen, Julius, 51, 108, 183

Thomson, Sir J. J., 184

Thomson, Thomas, 3

Thorium, 60

Thorpe, 172, 184

Thulium, 38

Thyreoglobulin, 169

Tiemann, 129, 132

Traube, 176

Travers, 50

Trional, 159

Triphenylrosaniline, 4

Troost, 184

Turner, Edward, 2, 14, 75

Turpentine, oil of, 129

Tutton, 184

Type theory, 18

Typhotoxine, 161

Unverdorben, 3

Uranium, 54

Uranium │x│, 54

Urbain, 40

Urea, synthesis of, 157, 158

Uric acid, 158

Valency, 112

Vanadium, 30

Van der Waals, 95, 184

Van Dorp, 133

Vanillin, 132, 162

Van ’t Hoff, 117, 141, 145, 147, 173, 177

Veronal, 159

Verquin, 4

Victorium, 40

“Vital force” doctrine, 169

Vogel, 185

Von Miller, 134

Waage, 183

Wallach, 129

Warburg, 46

Waterston, 83

Weber, 71

Weisbach, 37

Welsbach, Auer von, 38

Werner, 147

Williamson, Alexander W., 14, 16, 113

Winkler, 107

Wintergreen, oil of, 132

Wislicenus, 140

Wöhler, Friedrich, 5, 7

Wollaston, 63

Wroblewski, 96

Wurtz, 153

Xanthine, 157

Xenon, 43, 51

Zein, 169

Zinin, 3

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History of Chemistry, Volume 2 (of 2) From 1850 to 1910 · 第 13 / 13 章