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PROCEEDINGS 


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AMSTERDAM, 
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June 1903. 


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KONINKLIJKE AKADEMIE VAN WETENSCHAPPEN 
TE AMSTERDAM. 


PROCEEDINGS OF THE MEETING 


of Saturday December 27, 1902. 


DEC —- 
(Translated from: Verslag van de gewone vergadering der Wis- en Natuurkundige 


Afdeeling van Zaterdag 27 December 1902, DL XI). 


CA a sar IN TS, 


H. W. Bakuvis Roozenoom: “Tin amalgams’’, p. 373. 

J. Porrer yan Loon: “Benzidine transformation’. (Communicated by Prof. C. A. Lorry per 
Bruyn), p. 377. ; 

Kk. F. Wexcxenacu: “On the duration of the compensatory pause after stimulation of the 
auricle of the mammalian heart”. (Communicated by Prof. C. A. PeKELMARING), p. 878. 

J. Carprssar: “On the geometrical representation of the motion of variable systems”, p. 386. 

J. K. A. Warri SALOMONSON: “A new law concerning the relation between stimulus 
and effect”, (4th Communieatien). (Communicated by Prof. C. Wixkren), p. 392. 

M. W. Brewermcx and A. van DerpeEN: “On a colourless bacterium, whose carbon food 
comes from the atmosphere”, p. 398. 


- CO : : 5 = - 
L. IL. Srerrseva: “The caleulation from the magnetic rotation of the plane of polari- 
m 


sation, for substances without an absorptionband in the visible spectrum”. (Communicated by 
Prof. H. Kamerrinait ONNES), p. 418, 


The following papers were read: 


Chemistry. — “Tin amalgams”. By Prof. H. W. BaKnurs RooznBoom. 


(Communicated in the meeting of November 29, 1902). 


As the number of properly studied amalgams is still very small 
I directed Dr. van Hereren to conduct an investigation on tin 
amalgams in connection with the research on cadmiun amalgams 
by Dr. Bur. The more important results are Communicated here. 

In the liquid condition tin and mercury are miscible in all pro- 
portions. From the different mixtures a solid phase is deposited at 
different temperatures. The points at which solidification begins are 
indicated in the accompanying figure by two lines AC and CL 

25 


Proceedings Royal Acad. Amsterdam, Vol. V. 


(3745 


which meet each other at C (0.3 at. °/, Sn and 
angle. 


54.5) in a sharp 


As the line CB ends in the melting point of tin, the solid phase 
Which deposits on cooling must be either tin or mixed crystals in 
Which ordinary tin occurs as a component. On analysis, the solid 
phase which has separated from the liquid amalgam at 25° was 
found to be composed of 94 atom °/, Sn. 

On account of the difficulty of obtaining trustworthy results in 


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98.96 | 99 .0 


this manner, measurements of the fj, M/S were also made at 25° 
of amalgams. of 0.001—100 atom °/, Sn against an amalgam of 16 
atom °/,. 

These measurements led to the results that the unsaturated amalgams 
have a 4. M. F. rising with the amount of tin until at 1.2 atom "/, 
saturation sets in. From this concentration up to 99 atom °/, the 
potential remains unchanged, consequently two phases of unchange- 
able concentration must exist between these limits; one of these is 
the liquid one of 1.2 °/,, the other the solid one containing 99 
atom °/,. 

At 25° the crystals deposited therefore consist of nearly pure tin 
which is the case in a still greater degree at higher temperatures. 
By a comparison of the values of the /. J/. /. for amalgams of which 
the whole mass was liquid at 25° and 50° the heat of amalgamation 
could be calculated. The introduction of 1 gram-atom of Sn into 
a liquid amalgam with O0.01—1.00 atom °/, Sn, therefore nearly 
pure Hg, absorbs about 3000 calories. 

The line CB may also be considered as the line of the solutions 
saturated with Sn. It takes a very peculiar course. The part from 
120° up to the melting point of tin is nearly straight, the centre 
part shows a very rapid increase of the solubility with the tempe- 
rature, the lower part, however, an exceedingly small increase and 
also an exceedingly small solubility. so that the line approaches 
very closely the Hg-axis. In the lower part of the figure (p. 374) 
this part with its course towards the melting point of He has been 
drawn on a larger scale. 

5 


The extraordinarily great curvature of the central part of the line 
would lead to the supposition that the liquid mixtures of Sn + He 
in the absence of a solid phase would on further cooling separate 
into two layers. 

On cooling below —34.5° a change takes place in all amalgams 
from 0.3 to 85°/,, accompanied by a decided evolution of heat and 
decrease of volume. With increasing concentrations of Sn it first 
increases but then decreases in intensity. The maximum lies near 
50°/,. This change occurs in the figure on the line CD which 
therefore runs to at least 85 "/,. 

The change causes a new phase to appear which also belongs to 
the second solidifving-line CA. The maximum in the intensity of 
the change on CD at about 50°/, would lead us to suppose that 
mixed crystals having about this composition are formed. The modi- 
fication of tin therein contained must differ from ordinary tin. 

Between —934°.5 and - 
deposited from the mother-liquor (which moves along the line CA), 


38°.5 these mixed crystals continue to be 


this is accompanied by expansion. This change in volume diminishes 
as the amount of tin present increases and dies out near 75 °/,. 
The solidification point of pure mercury and also the final solidifi- 
eation point of all amalgams containing up to about 60°/, Sn, lies 
at —38°.6 (line AH). As the line (A of the saturated solutions 
also ends here it would seem that at the solidifying point of Hg, 
the solubility of tin has decreased to 0, so that instead of a eutectic 
mixture only the remaining mercury solidifies. 

Still, the point A bears quite the characteristic of a eutectic point 
as not only the line AF is horizontal, but all mixtures up to 60 °/, 
Sn also remain a shorter or longer time at this temperature which 
proves that a residual liquid is solidifying completely. 

A ereat uncertainty still exists as to the nature of the tin-modifi- 


cation which occurs in mixed crystals below —34°.5 chietly because 
it has so far not been possible to discover the part played in the 
amalgams by the grey modification of tin which may occur below 
20° C. 

But from the change in volume which takes place in the different 
transformations at and below —34°.5 we may argue that the specific 
volume of the tin must be smaller than that of the grey modification 
and larger than that of liquid and, therefore, also of ordinary tin. 


(514 


Chemistry. — “Benzidine transformation.” By Dr. J. Porrur van 
Loon (Groningen). (Communicated by Prof. C. A. LoBry Dr 


BRUYN). 
(Communicated in the meeting of November 29, 1902). 


It is known that hydrazobenzene when treated with a dilute mineral 

acid is converted into benzidine and diphenylene, benzidine being, 
however, the main product. 1 endeavoured to ascertain the proportion 
in Which the isomers are formed and in how far this depends on the 
temperature and the concentration of the acid and L further attempted 
fo measure the velocity with which the transformation takes place 
under definite circumstances, 
_ Benzidine was obtained pure by recrystallisation from water and 
distillation in vacuo; the melting point of this substance was 128° 
which is in agreement with the statements of Merz and STRASSER. 
Gourn= tf. Pract: Cho N; B 60: 186). 

For the preparation of hydrazobenzene, azobenzene was used as 
the starting point: this was purified by distillation and then reduced 
with zine dust in an alcoholic alkaline solution. The hydrazobenzene so 
obtained was dissolved by warming in alcohol and the still yellow 
liquid decolorised by means of ammonia and zine dust: the filtrate 
deposited pure white crystals of hydrazobenzene which could be 
separated unaltered from the liquid. A determination of the melting 
point gave as result 122°. 

For the study of the transformation it was necessary to have a 
method for the quantitative determination of benzidine. lt was found 
possible to do this gravimetrically by adding potassium sulphate to 
a solution containing not too much free acid and so precipitating the 
base as sulphate which was then collected on a weighed filter. According 
to my experiments, the slight solubility of benzidine sulphate amounts 
to 5—6 milligrams per 100 ce. of water at the ordinary temperature 
and consequently a correction should be applied. To ascertain in 
What proportion the two bases are formed during the transformation 
of hydrazobenzene, weighed quantities of this substance were put 
into bottles of about 120 ee. capacity and then shaken with a definite 
solution of an acid until all had dissolved. The benzidine present 
in the solution was then estimated, as directed, and the proportion 
calculated from the two data. 

At the ordinary temperature, N/10 hydrochloric acid used in this 
manner causes 84 per cent of the hydrazobenzene to be converted 
into benzidine. Normal hydrochloric, hydrobromic acids convert 90 


(3 


per cent of the same into benzidine. At a higher temperature ihe 
proportion is another, for in four experiments with one-tenth normal 
hydrochloric acid, nitric acid, sulphuric acid and hydrobromie acid 
the proportions at a 1007 were respectively 66.4, 67.5, 63.1 and 
65.8 per cent, therefore, much lower. 

To get some data respecting the velocity of reaction a beaker with 
50 per cent alcohol which contained hydrochloric acid in tenth- 
normal concentration was put into a thermostat and while stirring 
violently and passing a current of carbon dioxide over the surface 
a few grams of hydrazobenzene were introduced into the liquid in 
which that substance is but little soluble. 

At 25°, the velocity appeared to be dependent on the concentration 
of the acid and it increased more rapidly than the concentration. 
The experiments are being continued in the two directions indicated 
above. 


(Chem. Lab. Univers. Gronimgen). 


Physiology. — ‘On the duration of the compensatory pause after 
stimulation of the auricle of the mammalian heart.’ By Prof. 
Kk. FE. WereKeBacH. (Communicated by Prof. PEKELHARING). 


(Communicated in the meeting of 29 November 1902). 


When an extrasystole is set up by artificial stimulation of the 
ventricle or auricle of the beating frog’s heart, this extra-systole is 
followed up by a pause longer than the pause succeeding a spon- 
taneous systole. This long interval was studied by Margy, Dastre 
and others, and called a compensatory pause, because the longer 
quiescence of the heart was regarded as a compensation for the extra 
activity of the heart muscle. And it was not without reason that 
the word “compensation” was used, because the pause after an extra- 
systole is of such length, that the following spontaneous contraction 
just commences in the moment when it would have set in if, instead 
of an extra, a spontaneous systole had preceded. _ENGELMANN (6) 
has given a simple and exhaustive explanation of the pause: the 
normal, physiological stimulus to contraction reaching the heart from 
the vena cava and causing it to contract finds, after an extra-systole 
auricle and ventricle in a refractory phase and so it cannot cause 
a contraction. It is only the following stimulus which finds the 
heart again in a condition in which it can react on that stimulus; 
the contraction (the “post compensatory’’) then commencing, presents 


Ne 


(379 ) 


itself precisely in the moment in which it would have commenced 
if the heart’s action had been disturbed; so the rhythm of the 
physiological stimulation is not disturbed. In fig. I) the case is 
represented schematically. An artificial stimulus f reaches 7. When 
the second stimulus arrives it finds the ventricle still refractory ; so 
one systole is missing, but the following third stimulus, causes just 
at the right time again a normal systole. So the pause following 
the extra systole is with regard to its duration just Compensatory ; 
the time taken up by a spontaneous systole + extra systole and pause 
is just equal io that of two normal systoles. 

If, however, we stimulate the froe’s heart at the vena cava where 
the contraction always sets in, the compensatory pause is entirely 
missing and the following spontaneous systole succeeds the extra 
systole after a period equal to the normal period of contraction. In 
Fig. 1 the second artificial stimulus Y reaches the vena cava; the 
following spontaneous contraction sets in after the usual interval 20, 
a compensatory pause is missing. Whilst the interval between the 
systole preceding the extra systole and the one following the extra- 
systole after stimulation of the ventricle (or of the auricle) was 
double the normal period = 40, the same interval is here only 


12 + 20 — 32. 


} Ho Fy r 


From this ensues that the stimulus is not rhythmically induced from 

1) In these schemes answering to those used formerly by ENGELMANN and by me 
the lime is indicated on the three abseissae, and this is done for the duration of the 
phase and the stimulation of vena cava (Ve), auricle (A) and ventricle (V). | = 
physiological stimulus, ¥= artificial stimulus. The perpendicular lines represent the 
contractions of the heart-cavities. The slanting lines connecting the base points of 
the systole-mark indicate the direction in which the stimulus is conducted. If 
these lines are dotted the conduction does not actually take place. The duration 
of the spontaneous period is put at 20 abscis units (= 1 mM.), the interval from 
the moment of the physiological stimulus to the ventricular contraction (Ve V's) =5 
units. 


( 380 3 


outside to the vena cava, but that it originates in that place in a 
definite period. It is certainly the most natural and the most suitable 
explanation of the phenomenon to assume that at the venae cavae 
(as is known to be the case in less degree in the other parts of the heart) 
continually stimulating matter is formed, till this obtains such a 
strength that a contraction is caused. When however, the muscle 
fibres contract the stimulating matter seems to have been used up 
or at least to have been destroyed, so that every time after a con- 
traction the same time is wanted to produce new stimulating matter 
to such a strength that again a contraction follows. This destroying 
of the stimulating matter (dissociation in tons, chemical changes 
or whatever this may be) always takes place when there is a 
contraction, whether the systole is caused by the stimulating matter 
itself or caused by a stimulus induced from elsewhere. For it 
is a well-known fact, that by artificial stimulation of the auricle 
or the ventricle, more frequent than the spontaneous rhythm, the 
latter can be entirely overpowered. 

Another explanation is that at the vena cava there is a continual 
stimulation constant in strength, expressing itself periodically in 
systoles, because with each systole irritability, contractility and con- 
ductive power of the heart muscle are neutralized; so if a systole 
has taken place if always again lasts a certain time before the heart 
has recovered itself in so far that another contraction is possible. 
ENGELMANN Objects to this, that the explosion brought about by the 
contraction in the molecular system of the muscle cell will destroy 
the stimulating matter in stock together with the other properties of 
this muscle cell, (irritability, contractility and conductive power); 
moreover did) ENGELMANN show that the period of the formation of 
the stimulus can be changed independent of the irritability in the 
wall of the vena by chronotropic. nerve influence. So we must 
assume that the systole destroys the stimulating matter and that 
every time the latter must again develop itself after every systole 
to active power. The law of the preservation of the physiological 
period of stimulation dominating the duration of the compensatory 
pause and all the important data come to light by means of “the 
method of the extra-systoles” for the frog’s heart have been traced 
by Cusuxy and Marrnnws (1) for the mammalian heart. These in- 
vestigators showed that the mammalian heart obeys the same laws 
as the frog’s heart, that its activity is dominated by the same fun- 
damental properties of the fibres of the heart muscle, that the same 
theories hold good for both. 

Only in one respect they found a difference: when the auricle is 


( 381 5 


artificially stimulated, the compensatory pause after the extra-systole 
is not as in the frog’s heart truly compensatory but mostly of too 
short a duration. Sometimes if was completely compensatory, it was 
never entirely missing, it was generally shortened and then at any 
rate not equally shortened. 

They say on this subject (l.c. page 226): „As long as the interval 


i 


“A—A. is of considerable length the compensatory pause in the 
“auricle is truly compensatory, that is the interval between the last 
“spontaneous contraction and the post-compensatory is equal to two 
“auricular cycles. When however the stimulus falls earlier in the 
“irritable period, no true compensation occurs, the post-compensatory 
“contraction being premature,.... when Ad, is short the com- 
“pensation (of time W.) before the first natural contraction is always 
“imperfect.” 

The explanation of this difference is according to them: “either 
“ihe contraction wave passes from the auricle to the great veins 
“and there sets up a forced contraction which returning to the 
“auricle causes the premature systele, or the irritability of the auricle 
“oradually increases until if culminates in a contraction which is 
“independent of the great veins and initiated in the auricular muscle 
“itself. As to which of these two is the correet explanation we are 
“unable to give any opinion and feel that it would be useless to 
“balance probabilities before the movements of the great veins have 
“been exammed.” 

Formerly I myself expressed the supposition, that the mammalian 
auricle might possess a greater automatic irritability, because in the 
phylogenetic development a part of sinus and vena would be taken 
up in the auricle. 

H. E. Herine (2) has also been able to establish the difference 
deseribed for the first time by Cusiyy and Marrirews; he says: 

“The earlier the moment of stimulation falls in the irritable period 
“of the auricle, the shorter the artificial bigeminus is (interval between 
“last spontaneous and post-compensatory systole); the later it falls, 
“the more the duration of the artificial bigeminus approaches that of 
“two normal cardiac periods.” He continues: “the pause (after the 
“extra-systole of the auricle) lasts longer according to the moment 
“of stimulation falling earlier in the irritable period.” So here too 
he assumes the law of the conservation of the physiological period 
of stimulation: “aber die Beziehune ist keine so einfache wie am 
Ventrikel”. 

We had all overlooked, that Mackrnzin (3) had beeome convinced 
already in 1894 after a careful analysis of the venous and liver pulse 


( 38201 


that also in the human heart a “premature” contraction coming from 
the auricle is often succeeded by a too short compensatory pause. 
The possibility of distinguishing in this way between auricular and 
ventricular extra systoles had not escaped his attention. 

When reflecting upon the consequences which extra systoles coming 
from the auricle must have on the action of the heart and the cir- 
culation of the blood of man, I found the following simple explanation 
of the above mentioned phenomenon, an explanation from which 
ensues that we have not got anything to do with a difference in 
principle between the frog’s heart and the mammalian heart and 
that it is founded on an anatomic difference between the two hearts. 

ENGELMANN (5) has shown that in muscular tissue of equal com- 
position the stimulus to contraction is conducted also at an equal 
rate in all directions. So when an artificial stimulus is given to the 
auricle, a contraction stimulus and with it a contraction wave will 
pass from the stimulated point not only to the lower parts of the 
auricle and to the ventricle, but also to the higher parts of the 
auricle and to the vena cava, so to the place where normally the 
stimulus is formed and the contraction begins. ENGELMANN (6) has 
already pointed to the importance which this “antiperistaltie”” move- 
ment may have for the action of the heart, Cusuyy and Marrinws 
have also seen the possibility of it. 

When a stimulus is applied late in the irritable period of the 
auricle, so just before the moment when the following physiological 
stimulus was to come from the vena cava, the stimulus (and the 
contraction) will not be able to reach the vena cava any more 
before the physiological stimulus has had its effect there: auricle and 
ventricle will obey the extra stimulus, the spontaneous contraction 
already begun will not go on, but the rhythm at the venae is not 
disturbed. 

If the extra-systole sets in a little earlier, the extra contraction 
might reach the vena cava just at the moment that the physiological 
stimulus had developed to the necessary intensity ; then also auricle 
and ventricle obey the extra stimulus, the physiological stimulus is 
neutralized or it finds the whole heart refractory, but here too the 
rhythm of the formation of the stimulus is not disturbed and the 
pause of auricle and ventricle is completely compensatory. 

When however the auricle is stimulated still earlier, the extr 
contraction will reach the vena cava before the moment, in which the 
stimulus to contraction forming there, had attained at sufficient strength 
to cause a contraction. The stimulating matter found there at that 
moment will be destroyed by the extra contraction : from this moment 


new stimulating matter is being formed and after a certain time 
equal to the normal period it will have obtained enough intensity to 
cause another contraction. So the following spontaneous systole will 
not fall in the moment it would have done so if an extra systole 
had not been set up, but just so much earlier as the extra contrac- 
tion reached the vena cava before the moment in which the following 
spontaneous contraction would have occurred. 

In the diagrams I] and HIL an attempt has been made at making 


these observations clear for a particular case. 


In fig. H the auricle is artificially stimulated respectively 18, 15 
and 12 units of time after the previous spontaneous contraction ; 
auricle and ventricle follow the extra stimulus; in the first two cases 
the extra contraction moving to the vena cava intercepted the spon- 
taneous contraction coming from the vena cava. In the third case it 
arrives in the vena cava just at the same time as the physiological 
stimulus becomes active. In all these cases the rhythm remains un- 
disturbed and the compensatory pause is complete for the auricle as 
well as for the ventricle: the interval between the systole preceding 
the extra systole and the one following it is double the period of 


the heart, in this case = 40. 


In fig. HIL an earlier stimulation of the heart is shown, 10, resp. 
8 and 5 units of time after the preceding systole the auricle is 
stimulated. The extra systole formed by the first stimulus arrives in 
the vena cava 4 units before the following spontaneous contraction. 

The stimulating matter present at that moment is destroyed and 
a certain time — 20 has to pass before the stimulus has increased 
to sufficient strength. So the interval of the spontaneous contractions 
is not = 40 but = 16 + 20= 36. 


According to the extra auricular contraction falling earlier, this 


interval must become shorter, a fact which goes without saving, in 


fie: Il resp. — 35 vand = Bd, 

From this ensues, that when the stimulation ¢s ejected late in the 
irritable period the com pensatoriy pause is complete and farthermore, 
the earlier the stimulation ts efiected the shorter the interval between 
preceding systole and following spontaneous systole. 

Another influence is still at work, which also governs the length 
of the pause. The earlier the stimulation is effected in the irritable 
period of the auricle, the slower the stimulus is conducted through the 
wall of the heart, for the conductive power of the cardiac muscle 
returns but gradually after the preceding systole. So the interval A.— Je, 
will be longer according to the stimulus being effected earlier and 
as this interval also dominates the moment in which the stimulating 
material is destroyed by the induced extra contraction it will also 
influence the length of the auricular interval. In fig. HL where the 
slower conduction when the stimulus is effected earlier is taken into 
account this influence is illustrated. And in this way it is to be 
explained, that the interval ts longer after an auricular ertra-systole 
according to the moment of stimulation falling earlier in the irritable 
period of the auricle following quicker upon the preceding systole. 

The differences in length of the compensatory pause after stimu- 
lation of the auricle are in this way easily explained and it appears 
that the rules established for the amphibian heart hold good for the 
mammalian heart, in the sense however, as HeRING says, that “die 
Beziehung keine so einfache ist” 

The peculiar modifications in the course of the extra contiaction 
when the auricle is stimulated, derived by Mackenzin from the venous 
pulse, by Cusaxy and Marruews from the tracings of the auricular 
movements, Will probably find their explanation in the way in which, 
as is proved in fig. IL, the contraction waves meet here in the auricular 


( 385 ) 


wall and the differences ; will depend upon the spontaneous or the 
extra contraction being the most considerable. 

The question must however now be put: why does a complete 
compensatory pause always (or almost always, ENGELMANN ®) follow 
the extra systole of the auricle in the amphibian heart and why in 
the mammalian heart only under certain conditions > 

The answer may run as follows: In equally built up parts of the 
heart muscle the stimulus is also equally conducted to all sides, but 
Where for whatever reason the state of the muscle fibres is not 
everywhere the same, the conduction of the stimulus will neither be 
the same. This is the reason that the conduction of the stimulus of the 
auricle on the ventricle, in general of one division of the heart on 
the other, takes place much slower than inside the wall of auricle 
or ventricle. When conduction takes place in the direction opposed 
to the normal, this distinction will not make itself less felt. And 


just as the slower conduction may be the cause that extra-systoles 


of the ventricle never recede quickly enough to have a disturbing 
effect on the rhythm of the great veins, the differentiation between 
veins, sinus and ventricle in the froe’s heart will be the cause, that 
here a stimulation of the auricle is not quickly enough conducted 
through the transition places to disturb the rhythm at the venae 
cavae. Moreover this possibility seems so much the slighter, because 
in the frog’s heart muscle fibres with a strong automatic irritability 
ascend high up in the vena cava and so cannot be reached so easily 
by an extra stimulus. As this differentiation of the cardiac muscle 
between vena cava and atrio-ventricular limit is missing for the 
mammals, it is no wonder that the disturbing influence on the for- 
mation of the stimulus at the vena cava occurs just in the mammalian 
heart. 

If finally this explanation is the right one, the place where the 
auricle of the mammatian hearth is stimulated, will have its effect 
on the length of the compensatory pause: perhaps it will be possible 
to establish for not too small hearts and where the conduction 
of the muscle has already somewhat slackened, that for auricular 
stmulation far from the vena cava the compensatory pause is 
longer or even complete, whilst the pause becomes shorter according 
to the auricular stimulation taking place closer to the vena cava. 
For such an experiment the stimulation would always have to be 
effected exactly in the same moment of the heart period, every time 
equally long after the preceding systole. 


( 386 ) 


LITERATURE: 


|. Cusuny and Marrnews, Journal of physiology. Vol. XXI, 

9. H. E. Henine, Pflüger's Archiv. Bd. LXXXII. 

3. J. Mackenzie, Journal of Pathology and Bacteriology. Vol. IL. 

4. K. PE, WerereBacn, Zeitschrift fiir Klin. Medicin. Bd. XXXVI. 

5. TH. W. ENGELMANN, Sur la transmission réciproque et irréciproque. Archives Néer- 
landaises XXX. 

6. Tu. W. ENGELMANN, “Onderzoekingen” Physiol. laborat. Utrecht. IV Series, III 
Vol. 1895. 


Mathematics. “On the geometrical representation of the motion 


of variable systems”. By Prof. J. CARDINAAL. 


I. Im two communications ') some theorems have been developed 
by me, relating to the motion of variable systems. Also in this sub- 
division of the doctrine of motion the method of the geometrical 
representation occurring so frequently in Mathematics can be applied. 
The following communication has in view to mention some parti- 
culars on this subject. The representation in question is treated *) 
by R. Srurm. From this treatise L derive the short summary, which 


must needs appear here as an introduction to the subject. 


2. In the quoted considerations two complexes of rays played 
an important part, namely the tetrahedral complex formed by the 
directions of the velocities of the points of the moving system and 
the ravs of a focal system belonging to it; the latter consists for 
the motion of an invariable system of the normals of the trajectories 
of the points and for a projectively variable system of rays whose 
construction took a great part of the considerations. The purpose 
must be to obtain a simultaneous representation of complex and focal 
system; it will prove desirable to give the foremost place to the 


representation of the focal system. 


3. Let thus be given the focal system A situated in the space >, 
According to the method of Syivester let us suppose two planes 
Sand § with two projective pencils of rays situated in them with 
their vertices VY’ and NV situated on the line of intersection §§' w, 


!) Proceedings of the Kon. Akad. van Wetensch., section of science, vol. IV, 
pages 489 and 58s. 


ORT 


*) Die Gebilde ersten und zweiten Grades der Liniengeomelrie, 1, p. 257, 


( 387 ) 


v being an homologous ray of both pencils. The rays of A are the 
transversals of two homologous rays of (Y§’) and (NS). 
Let us now take two sheaves of rays in the space , with the 
and: A7 
= / 


these sheaves and the pointfields s and §’, in such a way that the 


vertices _X, , and establish a projective correspondence between 


pencil of planes through the axis YA, is homologous to the pencils 
CYS’) and (X's). Let / be a ray of A, cutting two homologous ravs 
of CNS) and (NS), to which in the homologous plane 4, a ray /, 


, and /, intersect 


out of NX, and a ray /’, out of X’, correspond; / 
each other in a point ZL. This point is homologous to the ray /. 
So a projective correspondence is established between the points of 
the space =, and the rays of the focal system 4. 

As is the case with every representation, also here the knowledge 
of its principal curve cannot be dispensed with. It is a conie A? 
through the points Y, and WX’, 
homologous to the pencils of rays of 4 situated in planes through. 
The plane 5, (principal plane) itself is homologous to 2. 

To an arbitrary pencil of rays of {a right line corresponds cutting 


situated in a plane §,. Its points are 


NG, to a hyperboloidic system of focal rays a conic having two 
points in common with .X,*, to a linear congruence belonging to La 
quadratic surface through WX’. 


4. Let a projectively variable moving spacial system be given: 
let as before PQRS be the tetrahedron of coincidence of two suc- 
cessive positions and let the corresponding focal system A be deter- 
mined by PQ and RS as conjugate polars and the conic A? touching 
PR and PS in Mand S. According to the indicated method the 
focal system can be represented in the space 2; for the tetrahedral 
complex of the directions of the velocities, however, we need an- 
other representation, which can be taken in such a way that the 
same principal curve is retained; we shall succeed in this if we do 
not represent the complex itself, but its section with the focal system d. 
This gives rise to a congruence (2,2) which we shall first investigate 
more closely. 


5. Let A be an arbitrary point, @ its focal plane; at the same 
time <A is the vertex of a quadratic cone, geometrical locus of the 
directions of the velocities through A, but of which only one is the 
direction of velocity of A itself. This cone will cut in general « into 
two rays belonging to the congruence (2,2); in this way we can 
construct the whole congruence. Bv this we have determined the 
construction, but not the geometrical character of the congruence ; 
this can be done in the following manner; 


( 388 ) 


Let the direction of the velocity « of a point A intersect the 
plane of coincidence PRS in L; now the focal plane of A intersects 
this plane in the polar p of 4 with respect to the conic A. The 
rays of the complex, at the same time rays of the conjugate focal 
system, are situated in the focal plane @ of A; from this ensues that 
these rays intersect the plane PAS in two coincident points, at the 
same time conjugate with respect to A“; so these rays will intersect 
A* and now ensues the theorem: 

“The rays of the congruence (2,2), which is the section of the 
complex with the focal system, have a point in common with the 
conic A?; so they are found as rays of A cutting K?.” 

So the congruence (2,2) arising from this belongs to those con- 
gruences, not possessing a focal surface, but a singular or double 


curve'), geometrical locus of the first series of foei of the congruence. 


6 The congruence can be constructed as a whole out of points 
of the conic A: for these points have the property of being the 
points of intersection not only of two but of a whole pencil of rays 
of the congruence (2,2), situated in the focal planes belonging to 
each of the points. These focal planes envelop a quadratic cone 2, 
with the vertex ?; so the congruence must touch the cone. From 
this ensues the following construction: 

“Let a point A. be taken on A, the focal ray. PA Dendranane 
cutting A for the second time in il’. Let the two tangential planes 
to P? be brought through PA; each of these planes contains a pencil 
of rays of the congruence, the vertex of one pencil being A, of the 
other. A’ 


7. We now proceed by giving some visible properties of the con- 
oruence (2,2). 

a. The two foci of each ray are the points of intersection with 
K*® and the point of contact with 2. The focal surface of points 
becomes /??; the focal surface of tangential planes consists of the 
tangential planes of A. 

Db. All rays of the congruence (2,2) belonging to a congruence of 
rays (1,1) of A cut two conjugate polars of 4, and cutting at the 
same time A® they form a ruled surface of order four with a simple 
come and two double lines. 

c. The rays of the congruence (2,2), lying on a hyperboloid of 
1) Gongruences of this type are ranged in the “Index du répertoire bibliogra- 
phique des sciences mathématiques” under V*? le and placed by R. SruRM in 
a separate division; see “Liniengeometrie”, Il, p. 323. 


( 389 ) 


A, pass through the points of intersection of the latter with A, so 
they are four in number. 

d. Let K? be real and let ? be situated within A?; all focal 
rays through P, the focal point of plane PRS, now cut A*: so all 
pencils of rays are real. If P lies outside A? two tangents out of 
P can be drawn to A?; these tangents are the lines of intersection 
of the cone P?? with plane PAS. The planes touching /?? according 
to these lines of intersection are focal planes, in which two pencils 
of rays have coincided; rays through /, not cutting A®, give rise to 
imaginary pencils of ravs of the congruence (2,2). Further ensues 
from this: 

“If A? is real and all the vertices of the tetrahedron of coinci- 
dence likewise are real, the congruence (2,2) is built up of real 
and imaginary pencils of rays, where as a transition two are double 
ones; if A? is real but the vertices A and S are imaginary, all the 
pencils are real.” 

e. The cases in which A? is imaginary, or also those in which 
all the vertices of the tetrahedron of coincidence are unaginary, do not 
give real congruences; so they are not under consideration. 


8. We now pass to the representation of the congruence (2,2) 
by which the image is obtained of the connection of focal system 
and tetrahedral complex. 

a. The congruence containing 2 pencils of rays which are 
represented in >, by straight lines having a point in common with 
X,*, the whole congruence is represented by a ruled surface passing 
through N°. To a straight line /, in 2, a hyperboloidic system of 
focal rays corresponds, which has four points in common with A?; 
so it contains four rays of the congruence and the representing sur- 
face S,* of the congruence (2,2) is a ruled surface of order four. 

hb. An arbitrary pencil of focal rays of 4 contains two rays of 
the congruence; the straight line in 2, corresponding to them cutting 
A” has another two points in common with N,*: so \,* is a double 
conic: of 5S,*. 

¢. To the pencil of rays in > with P as vertex and PRS as 
plane a straight line p, in 2, corresponds, cutting V,*. Each ray of 
the pencil P/ PFS belonging to two pencils of rays whose vertices are 
points of intersection with A, in all points of p, two generators 
ot 8,5 concur; from this follows that St is a ruled surface having 
as doupie curve a conic with a straight line cutting it; with this the 
type of S\* has been established. 

26 

Proceedings Royal Acad. Amsterdam. Vol. V, 


( 390 ) 


9. A closer acquaintance with the form of S,* is obtained by 
tracing the pinchpoints on the double curve; there can be two of 
them on p, and two on X,’. Those of p, depend on the position 
of P with respect to A?. 

a. Let P be outside A’. When a ray through P cuts A? in two 
points, we get two pencils of rays of the congruence, to which two 
real generators of 5,* correspond, concurring in a point of p,. For 
the tangential lines out of P to A? these two generators coincide, 
so the point of S,*, from which they are drawn is a pinchpoint; so 
for this position there are two real pinchpoints on p, ; from this ensues : 

“If P lies outside A’, p, has one part appearing as double line and 
another which is isolated; two pinchpoints separate these two parts.” 

hb. Let P lie within A’. All focal rays through P cut A’; there 
are no tangents to A*, so there are no pinchpoints on p,. So the 
double line p, is in its whole length really double line. 

Besides the pinchpoints on p, the surface S,* has also pinchpoints 
on X,*. To find these we must keep in view that the points on X,* 
correspond to the pencils of rays whose vertices lie on YX’ — w, 
which are thus situated in planes through w. Let y be a plane through z 
and ( its focal point; the pencil of rays (Cy) has two rays cutting 
Kk? viz. the two rays connecting C and the points of intersection 
B and B of y and K*. These two rays are represented in =, 
by a single point B, of X,’. Now CB belongs still to another 
pencil of focal rays, viz. to the pencil whose vertex is B and whose 
plane is the plane CbP=—?. The latter pencil belongs to the con- 
gruence (2,2) and is thus represented by a straight line through B, 
lying on S,*. In a similar way it appears that also a second straight 
line of S,* passes through 6,, namely the one which is represented 
by the pencil of rays (5's') lying in plane CL'P. Now again two 
principal cases may occur: 

a. « euts the plane PRS in a point 7’ outside A*. The pencil 
of rays 7 lying in this plane has rays cutting A’? in two points, 
touching A* or having two imaginary points in common with A’’, 
In this case these are parts of X,* through which two generators 
of S,* pass, which have thus to be regarded as points of a double 
curve, and parts which are isolated; the transition is formed by two 
pinchpoints, through which two coinciding generators pass; and these 
last correspond to the pencils of rays, having their vertices on the 
tangents drawn from 7’ to A*. 

b. The above mentioned point of intersection 7’ lies within X,’. 
All rays through 7’ cut A’; through each point of X,* two generators 
pass, so the whole conic X,° is a double curve. 


( 391 ) 


10. Among the particular sections of S,‘ the conics of this surface 
come into account. These conics have two points in common with 
N°: so (8) to these must correspond in 2 hyperboloidie systems of 
focal rays of A. These can be constructed in the following way : 

Let again a point A be taken on A, its focal plane « be deter- 
mined, moreover the second point of intersection A’ of @ with A* and 
the focal plane a’ of A’. If now a pencil of rays be drawn in a’ 
through A (which rays are not focal rays) and likewise through A’ 
in a, the pencils (4, a’), (A’,a) consist of conjugate polars of A 
between which a projective correspondence is established by means of 
the focal rays. In connection with X,* each pair of conjugate polars 
causes a hyperboloidie system of focal rays to appear. These two 
pencils generate them all, so their number is oo. 


11. Finally a few particular cases ask for our attention. 

a. The line of intersection w cuts the plane PRS in a point of 
the tangent plane PR. The pencil, of focal rays in the plane PR 
has as vertex this point of intersection; to this pencil corresponds a 
pinchpoint on X,°, but at the same time this pencil of rays has more- 
over a ray in common with the pencil of rays in the focal plane of 
the point 2; so the obtained pinchpoint is at the same time a point 
of p,; from this follows that in the point of intersection of Y,* and 
p, two pinchpoints have coincided; so through this point only a single 
generator of S,* can be drawn. 

6. Application to the motion of an invariable system. In this case 
K* is imaginary (the imaginary circle in the plane at infinity); so 
the congruence (2,2) consists entirely of imaginary rays. The pencil 
of rays P/PRS, however, remains real; so the representation in + 
becomes an imaginary ruled surface $,* with real double curve con- 
sisting of a straight line and a conic intersecting it. The same obser- 
vation can be made for other cases where K* becomes imaginary. 

c. Another particular case occurs when the ray AX’ — « is taken 
in such a way that it cuts the conic A,’; by doing so the character 
of the congruence does not change, but its representation does. If 
we now consider a pencil of rays in a plane brought through «, it 
is apparent that always one of the two rays of congruence to A’? coin- 
cides with w. Of the two rays cutting in >, the double conic N° only 
one is situated on $S,*, the other one passes into a ray situated in §, ; 
from this follows: 

“When the focal ray wv cuts the conic A? the surtace S,* breaks 
up into §, and a cubic ruled surface S,* of which p, 1s a doubte 
line; so this gives a simpler representation of the congruence ‘2.2) 

I6* 


( 392 ) 


Physiology. — “Ll new law concerning the relation between stimulus 
and effect” By Dr. J. K. A. WeRTHEIM SALOMONSON, commu- 


nicated by Dr. C. WINKLER. (Communication IV). 


In three papers, bearing the title “a new law concerning the relation 
between stimulus and effect I, Il and Il, I have tried to prove that 
by iereasing a stimulus, the effect too will increase in a definite 
manner. . 

The relation was expressed by the formula 


== Ate BAREN PTA ie tye a 


In deducing this formula I assumed that the transformation of 
chemical substance caused one and only one well-defined effect. 

In most cases however from such a transformation several conse- 
quences will result, constituting together the total effect : e.g. a mecha- 
nical, a thermal, a chemical, an electrical effect may be caused simul- 
taneously by some changing of the protoplasma. 

The question arises, whether our mathematical expression may be 
applied as well to the different parts of an effect as to the total 
effect. In order to obtain an answer to this question, we have to con- 
sider again the differential equation: 

OEZ 1 IRN SS Oy Ses (2) 
expressing, that by an infinitesimal increment of stimulus an infini- 
tesumal proportional part of the transformable substance was trans- 
formed, and at the same time stating the quantity of this transforma- 
tion. The quantity —d/ represents the increment of the effect. In 
the case of the effect being composed of several different parts, 


; 1 
the same equality will prevail for any of them, e.g. the — part, and 


1 
so we shall obtain for a partial effect the equation 
UE en k 
ADE OR ee Ds: Toa 
Nn 
in which n > 1. 
From this formula we get the expression 
Bahl =e BR ne 


wherein @ represents another constant than A, and wherein » is a 
number larger than 1. 
This formula for a partial effect is identical to the formula for a 


total effect the only difference being that the exponential constant i 
the ease of a partial effect is larger than in that of a total effect. 

The muscle may be taken as an example. Every contraction brings 
about a mechanical effect, whilst at the same time an electrical response 
is given. Finally the production of heat may be taken for the total 
effect, at any rate in the case of isotonic or isometric contractions 
where the mechanical effect is afterwards converted into heat. Thence 
we are justified in presuming that our statement about the formulae 
for total and partial effects, may be applied to the thermal effect and 
mechanical effect of muscle-contractions. 

I have tried to ascertain whether the numbers, given for the thermal- 
effects by different authors are in accordance with our law. 

In Daninewsky') | found several series of numbers, from which 
the following tables were calculated 


TAB: EE 
DaniLewskKy, 1.c. pag. 184. 
Isometrical contraction. Initial 
load 40 eram fie. 1. 

AS" Di P= 008 OERS 


i 


R Bw cal. 
ie observ. 


OOo | Lee ALT 
30 | 6.97 1,5 
koe) GO. Th td 
50 | 14.18 | 46.9 
80 | 19.38 | 49.2 


100 21.00 19.8 


300 99.98 90.5 
600 93 22. 

| 
800 93, ND) 


In this table, as in the following /? represents the magnitude of 
the stimulus; /2,, observ. the thermal effect as observed by DANILEWSKY. 


') B. Danitewsky. Ergebnisse weiterer thermodynamischer Untersuchungen der 


Muskeln. = V.e. A. Fick. Myothermische Untersuchungen 1889. 


( 39a) 


ii, cale. the thermal effect, as calculated with the constants given at 
the head of each table. 


TABLET 
o Ib. Initial load 80 Gr. fig. 2. 
A = 24.2 B= 0.0324 C= 20. 


i Salted Ey 

> fora : 

JR | Lw calc. observ. 
30 Gey 6 
50 15.3 18 
100 9 4 Ots 
300 94.2 94.8 


TABLE IIL 
Ib. Initial load 300 Gr. 
fig. 3. 
A= 7) 8. «B==002875 2 = 16:42 


| Ew 
R Ew calc. Obd 
30 Ds DI 
100 17 4 18 
400 2087 20 
800 20.8 ALAS 


The first of the next-following tables, which are much more 
important, is also taken from the experiments of DANILEWSKY Lc, 


( 395 ) 


whilst the observations in the 5 and 6 table have been published 
by Nawaticuin'): the school of Hemrnnain and that of Fick are 
both represented. 

The higher importance of the series given hereafter, consists chiefly 
in the fact of their having served to determine as well the mechanical 
response as the thermal effect with stimuli of increasing magnitude. 

In the series of Daninuwsky a double thigh-muscle-preparation of 
the frog after the method of Fick was employed, whilst NAWALICHIN 
made use of a single gastrocnemius. 

The muscle contracted isotonically, whilst simultaneously the thermal 
and the mechanical effect of each contraction, were recorded. As it 
has been proved with sufficient accuracy in our first papers that 
our formula may be applied to isotonic twitches, these may now 
serve us as a means of control. 

In the following series the magnitude of stimulus is again indicated 
in the first column by AR. The second column contains the calculated 
height of twitch, the third column the observed height; the fourth 
column the calculated and the fifth the observed thermal effect. 
The constants A,, B, and C were used for calculating the thermal 
effects, the constants Aj, Br and C), for calculating the heights of 
the contractions. 


TAB TBE: 
Danitewsky Le. Load 60 Gr. fig. 4. 


An — 40 Bj = 0.05 Cy = 14.4 
Ay, = 14.55 By = T02 Cw 14.4 

> 7 : En a 4 Ew 

R En calc. | observ. Ew cale. | observ. 

20 On <98 1.54 Oe 

30 .| 21.66 Dirt 3.90 4 

50 Br) 33 a eka | hot 

400 | 39.45 39.4 11.92 4404 

| 
300 | 40.00 40 | 14.50 | 14.5 


pn ee - 


. ee fo Je Wi 
1) NawazicHiN, Myothermische Untersuchungen. Pfluger’s Archiv, Bd. 14, p. 297. 


NAWALICHIN Le. pag. 297. Load 30 Gr. 
Ay ERS B, = 0.0036 Cy 
A ae B. = 0.00085 Cz 


En 


observ. 


Ew 


Rh 7% calc. | : 
observ. 


Zw calc. 


1,0 SRT ae 2.60 3 
450 3.66 3.8 Be) 3.5 
500 4.08 4,9, 3.78 / 
600 474 49, 4.81 4 
SOO 509, 5.4 6275 7 
1500 6.48 Tey A ere 10.5 
2000 OE 6 13.30 (325 
2500 6.25 6.2 14.60 15 


2500 6.95 OE 14.60 14 


| 


TABLE VI. 
Ib. Load 90 Gr. fig. 6. 


Ag OS b= 00185 C; == 660 
A= 7D By = 0.008 Cy, == 660 
PD hs gn En EE Lw 
R | Zn calc. observ. Ew calc. observ. 
700 3.40 3.5 4.70 45 
750 5.27 5.3 8.80 9.5 
900 | 6.42 | 6.4 14.61 12 
1000 6.50 65 | 46.00) |) 46 
| 
1500 “| 6.50 | 625: he ATEGO ME 
| | 


Considering that the degree of accuracy with whieh the thermal 
effects were measured is not very high, we have some cause for 
satisfaction about the results of our caleulations. Though only a first 
approximation has been effected throughout all these series, the errors 
remain wholly within the limits of the mean errors of observation. 
Moreover in some cases it is even possible to apply a correction. 


Looking at series VI, we see immediately that the observed numbers 


( 398 ) 


corresponding to the stimulus 900 are rather too small, as well for 
the height of twitch as for the heat-production. Calculating from the 
observed lifting-height the corresponding magnitude of stimulus, we 
find 810 instead of 900. Now taking this number 810, to caleulate 
the heat-production, we obtain 12, in perfect accordance with the 
observation. The supposition that the number 900 is an error and 
that 800 was meant is not very hazardous. 

From the communicated series we may draw firstly this conclusion 
that the heat-production, considered as total effect, increases virtually 
with increased magnitude of stimulus in the manner indicated by the 
established formula. 

In the three last series B, the increment-constant for the thermal 
effect, proved to be always smaller than the B, corresponding to it, 


a fact predicted already in our deduction. We found for the number 


By en : 
n —— in series IN , V and VI the value 2.5, 4.23 and 2.31. Though 


w 
of course even by this fact our deduction may not be deemed absolutely 
proven, it nevertheless affords a valuable support for considering the 
deduction proposed by me as a most useful working-hypothesis. 


Bacteriology. — “On a colourless bacterium, whose carbon food 
comes from the atmosphere.’ By Prof. M. W. Berrerinck 
and A. vaN DELDEN. 


We give the name of Bacillus oligocarbophilus*) to a colourless 
bacterium, whose carbon nutrition in the dark (and likewise in the 
light), takes place at the expense of a not vet well-known atmospheric 


1) It is probable that W. Herarvs (Ueber das Verhalten der Bacterien in 
Brunnenwasser sowie tiber reducirende und oxydirende Eigenschaften der Bacterien. 
Zeitschrift f. Hygiene, Bd. I, pag. 226) already in 1886, has had cultures 
of B. oligocarbophilus before him. He says the following: .... „Ausser- 
ordentlich auffallend war das Ergevniss dieser Versuche in der Hinsicht, dass eine 
Vermehrung der Bacterien in einer Flüssigkeit eingetreten war, welche keine 
organische Verbindungen sondern nur Salze enthielt. Ein unansehnliches, kaum 
sichtbares Piinktchen von Bacterienzoogloeën hatte sich im Verlaufe vom zehn Tagen 
so stark vermehrt, dass die ganze Oberfläche der Lösung vor einer dicken Haut 
bedeckt war.” Analytical results are not given, and the remark makes the 
impression of being accidental and is lost among insignificant observations. — 
Winoerapsky’s statement, concerning the accumulation of organic carbon in nitri- 
fying solutions, evidently refers likewise to this microbe, but his description suffers 
of indistinctness (Annales de l'Institut Pasteur, T.4 pg. 270 et 462, 1891).-— In the 
experiments of GopLeswx1 (Bulletin international de |’ Académie d. sc. d. Cracovie, 
Dec. 1892 pag. 408 et Juin 1895 pag. 178), the vanished CO? is not, as he thinks, 
absorbed by the ferments of nitrification but by the Mg O.Mg CO5. 


t Soa) 


carbon compound (or compounds), from which the energy, wanted 
for the vital processes, is also derived *). 

The culture of this bacterium on solid media or in nutrient 
solutions, containing soluble organic substances has not yet succeeded, 
which may, of course, have been caused by an erroneous choice of 
these substances. On the other hand, pure cultures on solid and in 
liquid substrata, without soluble carbon compounds, are easy to be made. 


1. CRUDE CULTURES OF BACILLUS OLIGOCARBOPHILUS. 


Bacillus oligocarbophilus is obtained by the following accumulation 
experiment, which, because of the purity of the thereby resulting 
vegetation, may be called a “perfect accumulation experiment.” 

Into a large ERLENMEYER-flask a thin layer is introduced of a 
nutrient liquid of the same composition as used for the water culture 
of higher and lower green plants, but with alkaline instead of acid 
reaction. 

One takes for instance: 


Distilled water 100 


Kaliumnitrate 0.01 to 01 
Dinatriumphosphate _ 0.02 
“Mineral solution” 1 drop. 


This “mineral solution’ contains in one drop: 


8 Merms MgsO, . 7 H,O 
0.05 " Mnso, . 4 H,O 
0.05 ' FeCl, . 3 H,O 


If from this liquid nitrogen, phosphor, kalium or magnesium is 
left out, special experiments have proved, that no, or but an insigni- 
ficant growth is obtained. As to the necessity of the likewise added 
elements sulphur, manganese and iron, there still exists some doubt. 

The inoculation is made with a not too small quantity of garden- 
soil, the flasks are closed with a cotton plug, or with filter paper, 
without impeding the entrance of air by diffusion, and the culture is 
left in the dark at 23—25° C. After two or three weeks, the fluid, 
which itself remains perfectly clear, is seen to cover with a thin, 
white, or feebly rose-coloured, very dry film, difficult to moisten, 


and macroscopically resembling a Mycoderma-film, but consisting of 


minute bacteria, microscopically often invisible without staining, and 
sticking together by a slimy substance. This is Bacillus oligocarboplulus. 


1) We also found another, rarer species, belonging to the genus Streptothrix 
Coux, with corresponding properties. It will not, however, be further discussed here. 


, 


( 400 } 


The growth of the film continues for months, whereby a considerable 
accumulation of organic carbon may be observed, which is not only 
visible to the naked eve by the vigorous bacterial growth, but can also 
be proved by direct weighing, and by a comparison of the perman- 
ganate numbers found before and after the experiment, of which some 
instances are given below. 

As there is. reason to admit that our bacterium is generally dis- 
tributed in garden-soil, and was without doubt always present in the 
crude material used for the inoculation, the failing of the film-for- 
ination in some of the flasks must necessarily result from the chosen 
culture fluid being less favorable to the feebler germs and not allowing 
their growth. So we observed that water, distilled in a copper apparatus, 
caused many more failures than when distilled in glass; we there- 
fore afterwards always used the latter. In other cases monads, which 
immediately devoured the bacteria, were cause of the failure; by transfers 
and by the use of pure cultures, these voracious organisms could 
be rendered harmless or removed. When the distilled water is replaced 
by tap-water, the number of flasks remaining without growth after 
inoculation with the same quantity of garden-soil is much smaller. 

If once a pellicle has formed, transfers into the said culture liquid, 
prepared either with distilled or with tap-water, come easily and 


without exception to development. 


2. SOURCE OF NITROGEN REQUIRED. 


In the above mentioned nutrient liquid we have chosen kalium- 
nitrate as source of nitrogen. As well, however, kaliumnitrite or 
some anorganit ammonium salt may be used. Very good results were 


obtained with: 


Distilled water 100 
Ammonium sulphate (or NI, Cl) 0.01—0.1 
Dikaliumphosphate 0.02 
“Mineral solution” 1 drop 
and with: 
Distilled water 100 
Kaltumnitrite 0.01—0.1 
Dikaltumphosphate 0.02 
“Mineral solution” sdi: 


As both these liquids answer to the conditions of life of the microbes 
of nitrification, the formation of nitrite or nitrate is actually to be 
observed when using them, and when inoculating with garden-soil 
or with crude cultures. With the easily produced pure cultures 


( 401 5 


of B. oligecarbophilus, of which more below, a good development of 
the film is possible, by which experiment it can at the same 
time be proved, that this microbe itself does not nitrify. Hence, 
ammonium salts or nitrites, added to excess can, even for a 
year or longer, continue unchanged under the luxuriantly growing 
pellicle of B. oligocarbophilus, whereas, in the presence of nitrifying 
ferments, they completely disappear in a few weeks, being then 
found back as nitrates. If the ferments of nitrification alone are 
present, there is no question of film-formation and = the nutrient 
solutions remain perfectly clear. 

Not only the nature of the nitrogen-furnishing substances, but also 
their quantity can in these experiments, as already inferred in the 
recipes, vary between fairly wide limits, and the same may He said 
concerning the conditions for the water culture of higher and lower 
green plants. The limits allowable for B. oligocarbophilus, have 
not yet been precisely fixed, but they certainly have a broader range 
for this organism (circa O.1—10 pro mille) than for the higher 


plants (0.5 
By many experiments it was established, that in absence of kalium, 


5 pro mille). 


phosphor, and magnesium, a still slighter growth occurs, than when 
no nitrogen compounds are given. Evidently B. oligocarbophilis finds 
in the almosphere, in a condition fit for nutrition, a quantity of 
nitrogen, which, although insufficient, should not be overlooked. 

If the distilled water in the artificial solution is replaced by tap-water, 
a somewhat higher rate of organic substance is produced. As in tap- 
water a small quantity of nitrogen compounds occur, — here, at 
Delft, about 0.4 milligrams of combined nitrogen per litre, 
whilst it contains the other necessary elements (phosphor and kalium, 
of course, excepted) in an obviously favorable form for the nutrition 
of our mikrobe, one can simply use for its culture: 


Tap-water 100 
Dikaliumphosphate — 0.02. 


It should, however, be kept in view, that the productivity in bac- 
terial substance, in consequence of the film formation, is not deter- 
mined by the volume, but chiefly by the extent of the surface of 
the medium, which is in free contact with the air. Hence, in a very 
thin layer of tap-water, the nitrogen may soon be consumed, whereas, 
with tee same amount of nutrient liquid, but with a smaller surface, 
cor seqpuently in a thicker layer, the provision of nitrogen will suffice 
for a longer time. Therefore, in order to obtain from a flask of 
determined size, the maximum production of B, oligocarbophilus, a 


( 402 ) 


nitrogen compound should be added when a small quantity of tap- 
water is used, which addition is not necessary when cultivating in 
a greater quantity in a flask of the same size. 


3. PURE CULTURE. 


Our bacterium does not grow at all or only to a slight extent 
on the commonly used bacteriological media, these containing too 
much organic food. But it is easy to produce pure cultures on solid 
media, when observing the same precautions which I described in 
the Meeting of the Academy of 27 June 1892 for the pure culture 
of the ferments of nitrification on agar-plates*), and to which I 
referred in the Meetings of 30 March 1901 (Proceedings p. 586) and 
25 May 1901 (Proceedings p. 5) when discussing the culture condi- 
tions of the oligonitrophilous Cyanophyceae. 

In all these cases it is necessary as completely as possible to 
remove all soluble organic substances from the solid medium, which 
is to be effected by a prolonged washing with distilled water. The 
agar thus prepared, with the required nutrient salts, for instance in 
the proportion : 


Distilled water 100 
Agar 1.5 
K, HPO, 0.01 
KNO, (of NH,Cl) 0.01 


is boiled and plated, and used for strew-or streakcultures originating 
from a film of B. oligocarbophilus. Very soon the common saprophytic 
bacteria which never lack in the film, are seen to develop on the 
plate and when these by their growth and respiration have consumed 
the soluble carbon compounds, which were not yet removed from the 
agar by the extraction with water, B. oligocarbophilus itself begins to 
erow. This is usually the case after 14 days. Then, however, the 
colonies become easily recognisable, our bacterium being the only 
species which in the given circumstances can feed on the atmospheric 
carbon, and so go on growing, whilst the growth of all other 
species soon comes to a stop. 

Even the colonies of the nitrifying ferments, which, as I have 
demonstrated before (Ll. ¢.), can grow fairly well on this medium, when 
instead of nitrate an ammonium salt is used, remain very small, 
never exceeding 1 mM. or less. On the other hand, the colonies 
of B. oligocarbophilus attain dimensions of 1 cM. and more and 
may then easily be transferred in a pure condition into test-tubes 


1) Nature, Vol. 46, pag. 264, 1892. e 


( 403 ) 


on the said medium. They grow on the agar as thin, snow-white 
or rosy-tinted, very dry, flatly extended layers, which strongly remind 
of the pellicle floating on the liquid. 

Also on silica plates, prepared in glass dishes, which, after extraction 
of the chlorides are soaked with a nutrient solution, B. oligocarbophilus 
can produce very fine cultures, appearing after some weeks, as 
snowwhite colonies with indented margin, and which by a right 
selection of the salts, can finally spread over the whole plate. 
Then the remarkable phenomenon is observed, that the silica liquefies 
a little in the centre of the colonies and sinks in by evaporation. 

The silica plates are made as follows. A commercial solution of 
potassium silicate, diluted with a known quantity of water, is titrated 
with normal hydrochloric acid. As the solidification is much favoured 
by an alkaline reaction, a complete neutralisation at the preparation 
of the plate should not occur, and as a plate, with a high percent- 
age of silica, contracts strongly after coagulation, and expresses much 
water, the dilution must be sufficient for this contraction to be delayed. 
Into a small beaker-glass was introduced, in a certain case, 5 cM° 
of potassium silicate diluted with 25 ¢M* of water, and into a 
second glass the required quantity of hydrochloric acid, amounting 
to 10 cM*® of normal acid. The acid is mixed with the diluted 
silicate and the mixture poured into a glass dish. The solidification 
delays the longer as the mass is more diluted, but it is easy, after 
some practice, to make very solid plates. The plate is first freed 
from the chlorides by streaming tap-water, then washed out with 
boiled water, and afterwards treated with the solution of nutrient 
salts. When these have sufficiently diffused into the plate, the glass 
dish is gently warmed at the underside, until the adhering water 
has evaporated and the plate shows a “dry”, glossy surface. The 
surface is flamed in the Bunsen-burner, by which only a partly but 
sufficient sterilisation is to be attained. 

Not only B. oligocarbophilus, but also the ferments of nitrification 
grow on this medium very well. By mixing of the diluted solution 
of the silicate with chalk, magnesium carbonate, or ammonium- 
magnesium phosphate, snow-white plates may be obtained, which 
are particularly fit for the culture as well of all these microbes as 
of several lower algae. Even earth-diatoms, of the genus Nitzschia 
will grow thereon. 

Once more it must be observed, that in the silica plates organic 
substances must be absent, even fragments of cork, fallen into the 
silicate solution, may disturb the experiment. 

The pure cultures, obtained on agar or silica plates, are as well fit 


( 404 ) 


for the further experiments on liquid media as the crude cultures, 
of which many experiments, continued for years, have convinced us. 
Every thought of symbiotic relations on which the carbon assimilation 
by our bacterium might repose is thereby excluded, so that at least 
the biological side of this part of our problem is clear. 

Concerning the further properties of our bacterium in pure cultures, 
we can be brief. In the films, as well as on in the colonies on the 
solid media, it consists of minute, thin and short rodlets, probably 
always immobile. They are ca. 0.5 u wide and 0.5—4 long. The 
length however is very variable and frequently particles are seen 
0.5 u wide and 0.7—1 u long. Often, when not using reagents, such 
as dyeing substances or acids, no structure at all is to be observed, 
neither in the colonies nor in the flowing pellicle, but the bacteria 
at once become visible by staining the preparations. The thick cell- 
walls form the chief constituent of the colonies; albuminous matter 
is only present in a slight quantity in this bacterium, 


4. THE NUTRITION WITH ATMOSPHERIC CARBON. 


A good appreciation of the carbon accumulation may be had as 
well by a direct weighing as by the permanganate method. 

For both determinations it is possible, to suck off the fluid, which 
is. practically free from bacteria, wholly or partly from beneath the 
film, so that the quantity of the culture material, destined for the 
filtration or the determination of the permanganate number, is not 
foo voluminous. 

In our experiments there only resulted a precipitate of caleium- 
phosphate or calciumearbonate, when we had used our tap-water, 
which is rich in lime, and when kaliumphosphate to excess had 
been added. These precipitates can, however, be dissolved beneath 
as well as in the film bv dilute acid, and then the acid can be 
expelled by further washing. The film is so dry and wetted with 
so much difficulty, that all these manipulations may be effected 
without much loss of material. 

The permanganate number was determined after KeBer’s ') method. 

In relation to the quantity of organic matter found by direct 
weighing or by the permanganate method and formed from the 
atmospheric carbon, the following should be well observed. 

As B. oligocarbophilus grows only on the free surface of the 


1) TrEMANN-GÄRTNER's Handbuch der Untersuchung der Wasser, 4e Aufl. pag. 205 
1895, 


( 405 ) 


medium, and not in the depth, the thickness of the layer of the 
nutrient solution and consequently its volume, is, as already observed, 
actually indifferent. That is to say, by enlarging the surface of the 
solution, a bacterial film of any dimensions is to be obtained, which 
circumstance is of importance for appreciating the productivity of a 
certain quantity of a nutrient solution, the more so as the thickness 
of the bacterial film is usually only one cell-layer. How very thin 
the required thickness of this layer can be, growth being. still 
possible, may be derived from the fact, that, especially when using 
distilled water with nutrient salts, the film can mount at the appa- 
rently dry glass-wall from 1 to 1.5 decimeter high, and not seldom 
extends on it nearly to the cotton plug. Only in certain vinegar 
bacteria I observed the same. 

As it seems that our bacterium forms no compounds prejudicial 
to its growth, so the only circumstance, which governs its increase 
relatively to a given volume of liquid, provided its surface be of a 
sufficient extent, is the lack of one or more elements necessary for 
the nutrition. Carbon cannot be among the number, our experiments 
being made with free entrance of air. 

Although it is thus established, that only the number of bacteria, 
produced in a certain time per surface-unit, indicates the rate at 
which the atmospheric carbon is assimilated, we will yet give the 
quantities in relation to the volume of the solution, because then a 
comparison can be better made with the numbers found by other 
authors for polluted waters. 


5. HOW MUCH CARBON IS ASSIMILATED. 


First we determined by an experiment, in which, after vigorous 
shaking, a culture was divided into two equal portions, how much 
one half contained at direct weighing, of bacterial substance, whereas 
the other half was titrated with kaliumpermanganate. We used for 
this a three months old culture on: 


Tap-water 100 


Na, HPO, 0.02 
KCl 0.02 
KNO, 0.02 


The film from the part, destined for the weighing, was separated from 
the liquid by filtration, washed out on the filter with strongly 
diluted hydrochloric acid, and subsequently with distilled water, to 
remove the chlorids. Subsequently the filter with the film was 

27 


Proceedings Royal Acad. Amsterdam. Vol. V. 


( 406 ) 


dried, first at 40°—50° C. and then at 100° C., until the weight 
remained constant. So we found that per litre 180 milligrams of 
bacterial matter were produced, and that, after deduction of 14 
milligrams, used by a litre of our tap-water itself, the corresponding 
permanganate number was 94. We can thus, with an accuracy 
sufficient for our purpose, accept that the relation between the two 
figures is as 2:1, that is to say, that the doubling of the permanganate 
number gives the weight of the dry bacterial substance, and, as 
this latter number is much more quickly to be found than the 
weight, we have contented ourselves with it in most of our further 
determinations. 

We shall now give some more figures. Like the preceding they 
all relate to bacterial films produced in ERLENMRYER-flasks on 100 cM’. 
liquid with a free liquid-surface of about 80 cM’. 

By weighing we found in one case on: 


Tap-water 100 


KCl 0.02 
KNO, 0.02 
K, HPO, 0.04 


after 5 months’ culture 235 milligrams per litre. On: 
Distilled water 100 


KCl 0.02 
KNO, 04 
K, HPO, 0.02 


“Mineral solution” 1 drop 


after 5 months 220 milligrams per litre. 

Some numbers, found by the permanganate method follow, and 
in the first place some relating to tap-water. 

The greatest production which we had, was obtained with tap- 
water 0.02 K,HPO, and 0.02 KNO,, after a year’s culture and 
amounted to 250 mers. of permanganate per litre, nearly corresponding 
with 250 * 2— 500 milligrams of dry bacterial substance. 

After a shorter time the production is likewise smaller; so we 
found in a culture on: 


Tap-water 100 


Na, HPO, 0.02 
KCl 0.02 
K NO, 0.02 


after 5 months’ culture (January to May) 202 mers. of permanganate, 
corresponding with 404 mers. of bacterial matter per litre. 


( 407 ) 


If the tap-water was replaced by distilled water, the production 
of dry organic substance was commonly smaller, which cannot, how- 
ever, result from the nutrition by substances in the tap-water, oxidisable 
by kaliumpermanganate, for the 14 mers. of permanganate, which 
our tap-water consumed per litre, we found quantitatively back, at 
the end of the cultivation period, in the clear liquid beneath the 
pellicle of B. oligocarbophilus, which liquid can easily be sucked off 
with a pipette, without any considerable bacterial contamination. 
Moreover the experiments with distilled water have likewise exhibited 
great divergency in production, and though the cause has not been 
established with perfect certainty, we still think it probable, that 
these differences result from the greater or smaller density of the 
cotton plugs, by which the speed of air entrance is greatly influenced. 
We base this supposition on results obtained with flasks, only 
differing in the width of the mouths, and to which we shall refer 
later. It is furthermore certain that we have not to do here with 
the infection of other bacteria, or with monads, for the pure cultures 
displayed as considerable divergency as the crude ones. Neither can 
the chief cause be attributed to a change in percentage of the air 
in gaseous carbon compounds, the differences being observed simul- 
taneously in cultures placed side by side in the same locality. 

But we now give some further numbers. In an experiment with: 


Distilled water 100 


K, HPO, 0.02 
KNO, 0.1 
KCl 0.04 


“Mineral solution’ 1 drop 


sterilised and inoculated with a pure culture of B. oligocarbophilus, 
were found, after 37 days’ cultivation (2 Jan.—19 Febr.) at 23° C., 
66.6 mers. of permanganate, corresponding with circa 133 mers. of 
dry bacterial substance per litre. 

In another experiment with: 


Distilled water : 100 


Na, HPO, 0.02 
KNO, 0.01 
“Mineral solution” 1 drop 


likewise sterilised and after a culture of 40 days, at 23°C. the per- 
manganate number amounted to 60 mgs., corresponding with 120 
mers. of dry bacterial matter per litre. 


‘ 408 ) 


In a third case in: 


Distilled water 100 
KPO, 0.02 
(NH,), SO, 0.02 
Na, CO, 0.01 
“Mineral solution” 2 drops 


after cultivating from 5 May to 1 Dee, 155 mers. of permanganate 
per litre were found. 
In a culture in: 


Distilled water 100 

Na, HPO, 0.02 
KC] 0.02 
KNO, 0.02 
“Mineral solution” 1 drop 


from 1 June to 1 Dee. we found 165.5 mers. of dry bacterial sub- 
stance, corresponding with ca. 83 mers. of permanganate per litre. 
As we see, the differences are considerable. 

When a little natrium acetate was added to the anorganic solution, 
and when using a pure culture for inoculation, we could neither 


state an augmenting nor a diminishing of growth. 


Thus we obtained in: 
Distilled water 100 
KC] 0.02 
KNO, 0.1 
Natriumacetate 0.02 
KHBO, 0.02 
“Mineral solution” 1 drop 


by means of weighing, 220 mgrs. of dry bacterial substance per litre, 
corresponding with 110 mers. of permanganate, which figures are 
not exceedingly high and might likewise have been producedi n the 
same time (4 months) from the air alone, without acetate. 

In all these experiments with distilled water, the free surface of 
the liquid was also 80 cM’, and the air had to pass through a 
dense cotton plug, with which the ERLENMEYER-flasks were closed. 
Already before we drew attention to the importance of the way in 
which the flasks are closed; be here still mentioned that we made 
some special experiments, which proved that a very narrow opening 
of the flasks, slackens the growth of B. oligocarbophilus, so that years | 
may go by before the film has vigorously developed. We could 
not, however, expected anything else, for the considerable volume of 
air, required for the growth of the said quantities of bacteria, can 
oniy very slowly diffuse inward and outward through the narrow canal. 


( 409 ) 
6. CARBONIC ACID CANNOT SERVE AS FOOD. 


Various experiments were made to establish what may be the 


volatile atmospheric carbon compound which renders the growth of 


B. oligocarbophilus possible. That it cannot be carbonic acid, whether 
free or combined, resulted from the following experiments. In closed 
culture-flasks with the best nutrient solutions, and arranged in such 
a way, that at times a little free carbonic acid mixed with pure air, 
could artificially be introduced, it was not possible to get any growth. 
This experiment, which seemed of particular interest, has been so 
frequently repeated, and so long continued under different conditions, 
that we consider it as quite certain, that free carbonic acid cannot 
serve for the nutrition of B. oligocarbophilus. 

For testing the influence of combined carbonic acid, cultures were 
made, firstly in the following solution: 


Tap-water 100 
Dikaliumphosphate 0.01 
Kaliumnitrate 0.01 


Natriumbicarbonate 0.1 


When cultivating at the free air surely a luxurious growth was 
obtained, but it was by no means more vigorous than when the 
bicarbonate was left out. | 

If in this liquid the nitrate was replaced by an ammonium salt, the 
result was quite the same. 

Secondly, the bicarbonate was replaced by common natrium car- 
bonate, the same quantities of the different salts being used. But in 
this case the action proved rather injurious than favorable. It is true 
that the film had become considerable after a few months, but it 
was directly to be seen that the growth was so much inferior to that 
of cultures obtained in the same circumstances but in absence of car- 
bonate, that the determination of the permanganate number seemed 
superfluous. Here, too, the replacing of nitrate by an ammonium salt 
or by a nitrite caused no change. 

As a remarkable fact it may be mentioned, that in these experi- 
ments, in our large flasks, containing a litre of air, the thin bacterial 
film mounted very high up the dry glass-wall, which is likewise often 
observed in the solutions made with distilled water, and may repose 
on the absence of dissolved lime salts. 

If the tap-water was substituted by distilled water, the addition 
of natrium carbonate did not cause an increase of bacterial growth 
either. We found, for instance, in: 


( 410 ) 
Distilled water 100 
HPO, 0.02 
(NH), SO, 0.02 
Na,CO, 0.1 
“Mineral solution’ 1 drop 


Pd 


after 7 months (5 May—1 Dec.) 155 mers. of permanganate, corre- 
sponding with ca. 300 mers. of dry bacterial substance per litre, 
which production is less than that, obtained in other cases under 
the same circumstances but without carbonate, so that here also, 
the action of the carbonate, the long time of cultivation being taken 
into consideration, was not favorable. Quantities of carbonate, 
smaller than 0.1 °/,, were neither successful. 

The results of this examination can be thus summarised, that for 
the growth of B. oligocarbophilus an atmospheric carbon compound 
is actually consumed, but that this cannot possibly be free carbonic 
acid. Furthermore, that also combined carbonic acid cannot serve 
for its nutrition. 


7. NATURE OF THE ASSIMILATED ATMOSPHERIC CARBON COMPOUND. 


If the carbonic acid of the air cannot be the food of B. olgo- 
carbophilus, what other atmospheric carbon source might then come 
into consideration ? 

It is clear, that we should think here of the carbon-containing 
component of the air, discovered in 1862 by the botanist Hrrmann 
KARSTEN *), and recently discovered anew by French experimenters, 
especially by Mr. Henrier’). It is true that the chemical nature of 
this substance has been hitherto unknown *), but yet it is certain that 
we have here to do with an easily oxidisable compound (or com- 
pounds), for a prolonged contact with alkali and air will already 
suffice to split off carbonic acid from it. Furthermore, according 
to the statement of the French investigator, the substance probably 
contains nitrogen. 

This latter circumstance gives rise to the question whether this 


1) H. Karsten. Zur Kenntniss des Verwesungsprocesses. Poggendorff's Annalen 
Bd. 191, pag. 343. 1862. To this place, as also to the not unimportant older literature 
on the carbon compound of the air, my attention was drawn by Mr. G. van ITERson. 

*) Comptes Rendus T. 135, pag. 89 et 101. 1902. 

3) Henriet thinks that the substance must be a monosubstituted formamid with 
the formula HCO.NHR, where R represents a still unknown alkylrest. But then it 
is not easy to understand, why the production of carbonic acid takes place so 
readily. It might then rather be expected that, with an alkali a formiate would 
result and no carbonate. 


( 444 ) 


nitrogen, like the carbon, is fit for assimilation by our microbe. 
Though this question has already partly been answered in the negative 
by the preceding experiments, it should still be remarked here that in 
nutrient liquids, without an expressly added nitrogen compound, for 
instance in: 


Distilled water 100 

Kr HBO, 0.02 

Mg, S, Mn, Fe traces. 
Or still better in: 

Tap-water 100 

K, HPO, 0.02 


without any further addition, a not inconsiderable growth of B. oligo- 
carbophilus may occur, so that at least traces of an assimilable nitrogen 
compound may be drawn from the air by this bacterium, whereas, 
for the possibility of assimilation of the free atmospheric nitrogen 
no indications were found. 

We now turn to another question, which the assimilation of the 
atmospheric carbon gives rise to, namely: How great is the quantity 
of the volatile substance wanted for the formation of the bacterial 
film produced in our cultures? This question is closely connected 
with the following: How much of the compound is moreover consumed 
by the respiration of our bacterium, escaping as free carbonic acid? 
For answering these questions we have to measure the quantity of 
the carbonic acid corresponding with a determined weight of dry 
bacterial substance, granted that the carbon percentage of this sub- 
stance be known. 

Our experiments relating to the measurement of the quantity of 
carbonic acid produced, are not yet closed, but as to the first part 
of the question, we give the following calculation to fix the volume 
of air wanted for the production of the carbon, actually accu- 
mulated in the bacterial films. We hereby make two chemical 
suppositions which, to be sure, are fairly well in accordance with 
truth. First, we admit that the carbon, freed from the unkown 
compound, as carbonic acid by a prolonged contact with alkali, 
is consumed quantitatively by our bacterium and, secondly, that the 
bulk of the bacterial cells consists of a substance possessing nearly 
the composition of cellulose *). 


1) If accepting that the composition of the bacterial cells corresponds with 
that of albuminous substances, then, instead of 44°/) C., 52 to 55°/, C. should be 
brought into account, and in this proportion the volume of the air should be 
augmented. 


( 412 ) 


Let us now consider the case when, in */, litre-flask with 100 cM’. 
of fluid and a free surface of 80 cM’, after a month’s culture a 
quantity of 20 mers. of dry bacterial substance is formed, which, 
calculated as cellulose, contains 44 °/, C.; we then find in the 20 mers. 
of dry matter 8.8 mers. of carbon. According to Hrnrimr the atmos- 
pheric carbon compound, present in a certain quantity of air, under 
prolonged action of alkali, gives out as much carbonic acid as occurs 
already in a free state in the same volume of air, that is per litre 
0.3 cM*.—0.6 mers., in which 0.163 mers. of carbon are present. 
Thus, for 8.8 mers. are wanted 55 litres of air. Consequently, in the 
course of a month these 55 litres of air must have diffused through 
the cotton plug inward and outward of our */, litre-flasks, in order 
to produce the found quantity of carbon, that is 76 cM*. hourly. 

Though this figure should not be considered à priori as impossible, it 
still appears to be very high, and the difficulty of accepting it increases, 
if still the addition has to be made of a yet unknown, but apparently 
considerable amount consumed for the bacterial respiration, which, as 
remarked above, seems necessary. We therefore think that it 
must be admitted that the quantity of the atmospheric compound (or 
compounds) assimilable by 5. oligocarbophilus, is much larger in our 
laboratory atmosphere, than in that of the Paris boulevard, analysed 
by Henriet, and that we have here to do with an extremely 
variable factor. The circumstance, too, that we have not as yet been 
able in our greenhouse, where the air, in the common sense of the 
word, is surely much purer than in the laboratory, to obtain a vigorous 
growth of B. oligocarbophilus pleads for this view. But here we 
could not always keep the temperature high enough, so that we 
consider our experiments in this direction not yet closed. Besides, we 
should observe, that in an empty, isolated room of the laboratory, 
the quantities of combined carbon drawn from the air, were as great, 
or only little less than in the laboratory itself, where the air was 
certainly impurer. 

We are accordingly conscious that further experiments, with fresh 
atmospheric air are wanted to decide, whether the carbon compound 
occurs in the atmosphere in a constant or in a varying percentage. 
Only thereby it will be possible to ascertain the distribution of this 
compound, by which, at the same time, the signification of B. oligo- 
carbophilus us. nature will become clearer. 

As to this signification, the question arises whether our microbe 
in substrata containing sufficient mineral nutrients (N, P, K, Mg, 5, 
Fe, Mn), but being poor in organic substances, is able to build up the 
latter in the dark from the volatile carbon compounds occurring in the 


( 413 ) 


atmosphere of the surrounding medium. And furthermore, whether 
carbon nutrition takes place exclusively in the floating dry films, 
— hence, in the earth, only on the relatively dry surface of the 
earth particles, — or that also in the depth of fluids growth and 
carbon assimilation be possible. The hitherto gathered experience 
about the self-purification of rivers and the biological purification 
of water in general, seems to exclude the latter hypothesis, and 
our own experiments too, render it not probable. The result of 
these experiments consists, in our opinion, in the very discovery of 
a microbe, which, in consequence of the film-formation, has the spe- 
cifie faculty, to absorb for its nutrition and multiplication, from a 
gas, namely the air, traces of volatile carbon compounds, by which 
the struggle for existence with the rest of the microbie world can be 
successfully sustained. The biological purification of water would, 
according to this view, find a counterpart in the biological purific- 
ation of the air by Bacillus oligocarbonhilus 


a . ? 6 ’ . . 
Physics. — “The calculation of — from the magnetic rotation of 
mm 
the plane of polarisation, for substances without an absorption 
band in the visible spectrum.” By Dr. L. H. Stertsema. (Com- 
munication No. 82 from the Physical Laboratory at Leiden 


by Prof. H. KAMBRLINGH ONNES). 


Starting from FrrzerraLD’s ') simple explanation of the magnetic 
rotation of the plane of polarisation derived from the ZrrManN effect, 
and also from the supposition that the result of the magnetic force 
is only shown by the displacement of the dispersion curve of the 
medium (n==/(a)) over a distance d, Harro ®) finds for the magnetic 
rotation @ 


27 cdl 
| tes) oe 


where z represents the thickness of the medium. Har.ro’s investigations 
are concerned with the parts of the spectrum in the neighbourhood 
of an absorption band and for these we are justified in making the 
above supposition, as appears from a formula derived by Vorer 


1) Frrzgeratp. Proc. Roy. Soc. 63 p. 31. 


2) Harro. Diss. Amsterdam 1902, p. 7. 


( 414 ) 


from a more rigorous theory *). If, however we want to apply it to 
points at a greater distance from an absorption band, as is the case 
with the magnetic rotation of transparent substances, we must turn 
to Vorer’s more general formula *) 


en 9? (9 — H, +c, RD) 
(#— 9), Eep RO)? + HH 
If we may assume that only one term occurs under the summa- 
tion in the second member, and also that ¢,/ and 9, are small 


compared with 9, a simple reduction shows that the new dispersion 
curve may be derived from the original one by moving each point 
2 
over a distance */, er ——, which depends on & and hence also 
9, 
on the wave-length. In this case Harro’s relation will hold, if d is 
not supposed constant, but proportional to 2’. 

Though it is uncertain whether for a given transparent substance 
we are entitled to accept the formula for 7 with only one term 
under the summation, we may investigate to what results this would 
lead. From the elementary theory of the Zeeman effect it follows that 


nlt 3 


ry rj x 
Be ER 


m Az 
whence for the displacement of the dispersion curve 
HIW ‘e¢ Be 


t= f= i= = ‘ 
m Ax m 4a V 


This value has been derived for the absorption band. From the 
above considerations it follows, however, that we may apply it for 
each wave-length, and hence we find 

Ane À dn e 2 dn 


oS 2z2—H — = 2 H— —__ —_, 
rs m AnVd2 m2V da 


Whence follows for the rotation constant @ 


OL AG. ae. 

m 2V da’ 

which formula corresponds with one, given by Vorer®), if we replace 
the / occurring there by: 


o 


ed 
—.—V, 
m 2 

1) Vorer. Wied. Ann. 67 p. 351. 

2) Vorer. Wied. Ann. 67 p. 349. 

3) Vorer. Wied. Ann. 67 p. 351. 


( 415 ) 
which value may also be derived directly, if we equate the magnetic 
1 . 2 ' 
displacement 5 Ch R after Vorer with that resulting from the elemen- 


tary theory. The dispersion of the magnetic rotation expressed by 
this formula is the same as that resulting from BreQqverer’s ') relation 
and found by him to be confirmed in the case of carbon disulphide 
and creosote. 

€ 


U . . . 
The relation found for @ enables us to compute — as soon as we 
m 


5 2 U7 $ 
know the rotation constant @ and the dispersion a of a substance 
a vr 


for the same wavelength 2. For we have 
€ 2V da 


We shall make the calculation for some substances at a value of 
4= 589 uu. The rotation constants 7 being usually expressed in 
minutes we have 


20 
OS Daa 
360 X 60 
and hence we find 
e 2X3X10 ar da da 
ECE ena a a TS ae al es LOA —, 
m 589 360 < 60 wo dn x aS dn 


1. Aw (100 KG., 13°.0). I have found *) r= 553.10—°. Perreau a) 
finds for the refractive index at (1 atm., 0° U) 
A= 644, n—np = 85.10 
538 88,10 
12 
whence = = 0.65 & 10° and 0.58 X 10%, on an average 0.61 10°. 
n 
Supposing #—l proportional to the density, it follows that for air 
(100 kilogram, 13°.0 C.) di/dn = 0.648 Xx 10° and we find: 
“ = 2.96 X 553 X 0.648 10‘ = 1.06 X 107. 
m 


In the same way is found for: 
2. Carbon dioxide (1 atm. 6°.5). += 8.62 X 10-5 


Bl atm., 0°) =342 ><107 
7, | aks Oh See 4 
(1 atm, 6°.5) =3.50 M 107 


1) BecquereL. C. R. 125 p. 679. 
*) SIERTSEMA. Comm. Lab. Leiden. Suppl. N°. 1, p.86; Arch. Néerl. (2) 2 p. 376, 
®) Perreau. Ann. de Ch. et de Ph. (7) 7 p. 289, 


( 416 ) 


© — 0.89 X 107. 
3. Hydrogen (85.0 Kilogram, 9°.5 C.) p= 456 108 
dada atm. 027) == 405 
(S5:0°KG 955 Cj = HIL 10% 
? 


= AO 
m 
4, Water. From refractive indices of Durer *) and the magnetic 
rotation constant O0'.0130 we get 
é 
= 1,25 07 
mn 
5. Carbon disulphide. In the same way with 7+ =0'.042 we 
find from VAN DER WILLIGEN’s *) refractive indices 
e , e 
OY aba KOL 
me 
6. Quartz. r=0.01684 *). By means of VAN DER WILLIGEN’s refrac- 
tive indices we find 
te a he 
= ee Bie 107 


Mn 


Ca. 
It may be remarked that the values of — found here correspond 
In 


in order of magnitude with those found in other ways. 


1) Durer. Bull. Soc. Minér. 8 p. 218. 
2) V. op. Wituicen. Arch. Mus. Teyler III. 1. p. 55. 
3) Borex, C. R. 128, p. 1095. 


(January 24, 1903). 


ie 
EN 
< 


KONINKLIJKE AKADEMIE VAN WETENSCHAPPEN 
TE AMSTERDAM, 


PROCEEDINGS OF THE MEETING 


of Saturday January 31, 1903. 


| oo 


(Translated from: Verslag van de gewone vergadering der Wis- en Natuurkundige 
> r € a « 5 r 
Afdeeling van Zaterdag 31 Januari 1903, DI. XI). 


ORE MN TS. 


A. Smits and L. K. Worrr: “The velocity of transformation of Carbon monoxide” 

municated by Prof. H. W. Bakuvis RoozeBoom), p. 417. 
vee ns “a TE ns : nn AA 

J. J. VAN Laar: “The course of the melting-point-line of solid alloys or amalgams”, ‘First 
communication). (Communicated by Prof H. W. Bakuuis RoozrBoom), p. 424. 

J. J. van Laar: “On the potential-difference, which occurs at the surface of contact of two 
different non-miscible liquids, in which a dissolved electrolyte has distributed itself” (Com- 
municated by Prof. IL. W, BAkuvis Roozrnoom), p. 431. 

J. J. Harro: “The value of some magneto-optic constants”. (Communicated by Prof, P. 
p. 438. 

Se peo “son: € tn Ronn : : 

JE A IE WERTHEIM SALOMONSON : A new Jan concerning the relation between stimulus 

and effect”, (V). (Communicated by Prof. C. Wixkren), p. 441. 
rr No) PA Cis es : MENE . J 

D. J. Korrewee: “Plaitpoints and corresponding plaits in the neighbourhood of the sides of 
the g-surface of van DER Waars”, p. 445. (With one plate). 

A. H. Sirks: “Some remarkable phenomena, concerning the electric 


- (Com- 


ZEEMAN), 


circuit in electrolytes”, 
(Communicated by Prof. H. A. Lorentz), p. 465. ; 
The following papers were read: 
Chemistry. — “The velocity of transformation of Carbon monoride.” 


By Dr. A. Smits and L. K. Worrr. (Communicated by Prof. 
H. W. Bakuvis RoozwBoom). 


(Communicated in the meeting of December 27, 1902). 


Ya vatelet> kh LTA) ‘ *. T T > l 1A ily ” p 1 <_—-(' \ 
From the researches of Boupovarp!) on the equilibrium 2COSCO,-+C, 
where use was made of the accelerating action of the metals Ni, Co, 
Fe, it follows that they do not modify the equilibrium but only 


1) Ann. de Chimie ef de Physique [7] 24, p. 5 (1901). 
28 
Proceedings Royal Acad. Amsterdam. Vol. V. 


( 418 ) 


exercise an influence on the velocity and are, therefore, catalyzers. 
It was shown by Bovpovarp that, whilst CO, in contact with C is 
practically totally converted at 1000° into CO, the amount of CO, 
in the gaseous mixture in equilibrium increases at lower temperatures 
in accordance with the sign of the heateffect CO,+C=2CO—42000 
eal. until at 445° the CO is practically completely converted into 
CO, and C. 

From this follows that below 445°, CO exists in a metastable 
condition, 


INVESTIGATION. 
a. Preparation of the catalyzer and preliminary experiments. 


1. The following research was instituted with the object of 
determining velocities of reaction in the metastable region in presence 
of a catalyzer. The apparatus employed by us was in the main the 
same as that used by van’? Horr in his research on the velocity of 
transformation of detonating gas into water. The reaction vessel, 
however, was filled with a catalyzer obtained in the following manner. 

Pumice stone was broken up into small lumps, drenched with a 
solution of Ni(NO,), then dried, ignited and finally reduced in a 
current of hydrogen or carbon monoxide. 

This reduction, it was observed, takes place in two stages. The 
greyish-blaek surface of NiO first turns yellow owing to the formation 
of a suboxide (Ni, O7) *) and afterwards on complete reduction again 
becomes dark-grev. When operating at a high temperature, reduction 
with H, or CO gives apparently, the same material. If, however, 
the reduction takes place in a current of CO at 445° a layer of 
carbon is deposited on the reduced nickel. 


2. The experiments with nickel-pumice obtained by reduction 
with either H, or CO at a /agh temperature gave the following 
result *). 

At 310° (boiling point of diphenylamine) the activity of the catalyzer 
did not appear constant. Successive fillmgs continually gave smaller 
diminutions of pressure in the same length of time. 


1) Miter, Bell (Chemical News 20, 258). 


2) Coating the inner wall of the reaction vessel with nickel did not appear to 
affect the result, probably because the surface of the glass wall was very small 
as compared with the surface of the catalyzer. 


( 419 ) 


We found for instance: 


5407 
Diminution 
Filling. in mM, He. 


during 10 minutes, 
ee 


dst 5,68 

2nd 5,00 

3rd 3,80 
ect. 


As we suspected that the retrogression of the activity of the 
catalyzer was due to the ever increasing layer of C, which deposits 
on the catalyzer during the experiment and fillings, we next used a 
nickel-pumice which had been reduced at 445° and was in consequence 
already coated with a layer of carbon. Although at first there was 
still a perceptible diminution in the activity, the differences in suc- 
cessive fillings become gradually smaller and finally, the activity 
was constant as seen from the following table: 


3dLO° 


Diminution 
Filling. in mM. He. 
during 10 minutes. 


1st 1,88 
2nd 1,80 
3rd 1,78 
4th 1,74 
oth 1575 
6th 1,74 
7th 1,74 


Being satisfied with this result, we started our investigation with 
the catalyzer of constant activity obtained in this way. 
b. Measurements concerning the order of the reaction. 


For the determination of the order of the reaction the method of 
VAN ‘t Horr was first of all applied. It is given in this case by 
the equation: 


28% 


( 420 ) 


The determination was made at 310°. 

In the first experiment the pressure of the CO was 786,8 mm. 
He at the commencement; after 50 minutes the pressure amounted 
to 739,9 mm. Hg. The diminution of pressure in 30 minutes there- 


fore amounted to 46,9 mm. Heg. 


de EE f 
If we take for = the diminution of pressure per minute then 


d 


iC 
5 becomes 1,56. 
3 


In the second experiment the pressure of the CO was 535,3 mm. 
Hg at the commencement and after 30 minutes the pressure had 
come down to 501,7 mm. Hg. Here, the diminution of pressure 
in 30 minutes amounted, therefore, to 33,6 mm. Hg or = 1,42 

ud 
C,=aver. of press. at beginn. and end at the 1st experim.=763,35mim. Hg. 
ee a a " 0. ho yay ae = od 

If from this we calculate », we find 

7 0-60. 
from which it is apparent that the reaction is a monomolecular one. 
In order to make more certain of this, the order of the reaction 
was also determined at two other temperatures according to the 
method given by Noyes. In this case » is calculated from the 
following formula: 


t 
log— 


t, 
n= + —.— 
Cy 
log— 


C; 


in which 7, and f, are the times during which the same part of the 
original quantity is converted when starting from different concen- 
trations c, and «¢,. 

At 256° we obtained the following result: 


192 
300 
n=i dd 
7 525,1 
770,9 
The experiment at 340° gave 
60 
d ME 0,92 
Oee tn 
loq— 


Rye 


( 421 } 


The observations at the three temperatures 256°, 310° and 340°, 
therefore lead to the conclusion that we are really dealing here with 
a monomolecular reaction. 


e. Determination of the reaction-constant at 256°, 310°, 340°. 


These determinations were conducted with the same reaction vessel 
and the same catalyzer. 


256° (boiling point of amyl benzoate). 


Time in minutes. | Pressure | 1 7 


EN er in ==: log——— = 


| 
1 | 2 ‚m.m. He 


0 761.0 | aa 

5 | 0 Ree 0 00046% 

10 ie? 757-6. 0.000384 
10 | 756.4 | 0.000987 
AD) | | 0.000276 
30) Hse 0.000277 
40 | 0.3 0.000278 


average 0.000279 


The following may serve to elucidate this table: 

At 256° the catalyzer seemed to still perceptibly absorb the CO, 
which caused the diminution of pressure during the first 5 minutes 
to be excessive. The values for / are, therefore, not constant when 
we start from the pressure corresponding with the time O, but they 
gradually diminish which may be seen from the first two figures in 
the last column of the table. To eliminate the error caused by absorp- 
tion, we have, when calculating 4, started from the pressure corre- 
sponding with the time 5 minutes (column 2) and, therefore, have 
called this pressure P,. As the CO concentration had diminished very 
little in 5 minutes the error thus introduced could be disregarded. 
The values obtained for / are found in the last column beneath the 
dotted line. The following table relates to the temperature 310°, 


| Pressure | D 
Time in minutes | in KN == a! log — a 
Al | t A aid 
| mm. Hg | 
| | 
0 | 786.8 
| 
10 | 769.8 | 0.00192 
| | 
20 | 754.8 0.00184 
| | 
30 MEC 4 0.00184 
40 | 795.6 0.00184 


average 0.00186 


As was to be expected, the absorption at this high temperature 
was scarcely perceptible and in the following table, which shows the 
results obtained at 340°, no absorption whatever was noticed. 


340° (boiling point of phenantrene) 
Pressure 1 P 


Time in minutes in k= log aaa 
21 


m.m. He 


0 791.4 

10 746.1 | 0.10524 
20) 709.9 0.00527 
30 668 7 0.00536 
50 612.7 0.00521 


average 0.00527 


In order to make sure that the activity of the catalyzer had not 
diminished during these three series, a series of experiments was 
finally taken at 310° with the following result. 


( 423 ) 


310° 


| Pressure 1 > 


: me 
Time in minutes | in | k = — lo 


/ mm. Hg | 


0 805.5 

10 188.3 0.00189 
20 773.0 0.00183 
30 7157 8 0.00182 
40 742.8 0.00184 


average 0.00184 


The activity of the catalyzer had, therefore, undergone no change 
during these measurements, so that we were justified in calculating 
the temperature-coefficient from the results obtained. The result was 
as follows: 


ki+10 
Temperature. k ab 
hu 
256° 0.000279 
>1,4 
310° | 0.00186 
ke 
340° 0.00527 
| 


d. Mechanism of the reaction. 


What idea are we to form about the mechanism of the reaction 
if this takes a monomolecular course? 

If we assume the formation of Ni (CO), with an immeasurably 
large velocity and the subsequent breaking up of this compound 
according to the equation 

Ni (CO), = Ni + 2 CO, + 2C 
we must also accept the equilibrium 
Ni (CO), S Ni + 4 CO 
of which the constant is given by the equation: 
Ca 


je eae 


’ 


Cv: (co)4 


This would then necessarily lead to the conclusion, that the velocity 


( 424 | 


of reaction should be proportional to the 4% power of the CO-con- 
centration whereas it appears to be proportional to the 1st power 
of the CO-concentration. Rejecting this hypothesis two further sup- 
positions remain. 

Firstly : 

I: CO = C+ 0 (with measurable velocity) 
II. CO +0 = CO, (with unmeasurable velocity). 

Secondly : 

L CO+M=—C+Ni0 
IH. CO+ NiO = CO, + Ni. 

In the last case it need not be assumed that one of these reactions 
takes place with unmeasurable velocity, but only that the second 
one proceeds more rapidly than the first. 

As regards the nature of the catalyzer we think we may conclude 
from the result of several experiments, that if is not the carbon but 
the finely divided nickel which possesses the catalytic action. 

Amsterdam, Chem. Lab. University. Dec. 1902. 


Chemistry. — Professor Bakuuis RoozrBoom presents a communica- 
tion from Dr. J. J. van Laar on: “The course of the melting- 
point-lines of solid alloys or amalgams.” (First Communication). 

(Communicated in the meeting of December 27, 1902). 

1. In the researches of vaN HeTEREN *) on Tinamalgams a mel- 
tingpoint-line occurs?) of a kind, which has not as vet been studied 
over such an extended course (from 0 to nearly 100 atom °/, of mereury). 
This is chietly due to the fact, that the temperatures of fusion of the 
38.6°. In 
consequence the meltingpoint-line of the tin meets that of the mercury 

| practically at 100 atom "/, mer- 
OT cury‚ so that the meltingpoint- 
ft line of the mereury has not even 
been observed. We therefore 

see for the first time a melting- 


two metals are so very different; tin 231°, mercury 


mercury | tin point-line in its full course, and 
the question arises whether the 
course, found by vaN HRTEREN, 
may be predicted theoretically. 

The answer to this is in the 
affirmative. Let us, to start 
with, take the most simple view 
Fig. 1. as regards the molecular poten- 


1) Dissertation 1902. (also Report Meeting 29 Nov. 1902). 
2) l. c. pg. 18. 


tials u of the tin as solid substance and u, of the tin in the liquid 
amalgam, namely that 

eS=e— el | 

Wesen Te RT log: (zen ee nnn St 

In this it has been assumed, firstly that the tin, erystallised from the 

amalgam, does not consist of mixed erystals, but of pure tin 


a suppo- 
sition, which has been proved by experiment to be nearly correct — 
and secondly, that the energy-quantity e is no function of «. Later 
on we will drop this last simplified supposition, and demonstrate, that 
a more accurate calculation of the function u, affects the course of 
the meltingpoint-lines quantitatively, but not qualitatively. Then it is 
our object to demonstrate at once, that the entire qualitative course, 
as represented in the figure, follows from the equations (1) in con- 
nection with the course of the logarithmic function of 1—w. By 
putting the two potentials equal to each-other, we obtain: 


(e, — €) — (ce, —¢e) T = — RT log (1—2), 
or calling e, —e—=q (the heat of fusion of the solid tin, when passing 
into the amalgam), and the quantity c,—c=y: 
q— YT = — RT log (1—2), 


from which follows: 
T= q 
y—Rlog(1—z) 


(2) 


This is then the most simple form of the meltingpoint-line. 
On introducing the temperature of fusion of pure tin 7',, « becomes 
O, and we obtain: 


a 
tf 
so that we may also write: 
r bs le 7: 
acs rr a : Wr pay ye (3) 
RE 1—@ log (1—2) 
— —— log (1—2) ; 


q 


RT 
if we abbreviate —— to 0. 
q 
We notice at once, that on the development of the logarithmic 
function, the formula, for very small values of w, passes into 
Per. 
Ri 
Ise: 
q 


v 


that is to say into TE lee pS Ea 


the ordinary formula of van ’t Horr for extremely dilute solutions. 
If, however, the solutions are no longer extremely dilute, we can 
no longer be satisfied with one or two terms in the development of 
log (A—x), but loy 1—vr) must remain. 
I will now show, that the approximative relation 
1, 


ig iE iecet 
1 — Glog (1—2) 


4 Al 


gives indeed the observed course qualitatively. For BARS find : 
U 
dT de 0 
de (1—@ log (1—z«))?’ i en 
Whilst 7” itself, for «— 0, passes into 7, 


T= 0, which already agrees with the steadily declining course — it 


and for «= 1 into 


ryy 


a. 
appears from —, that this quantity, for «=O, becomes: 


C Ai 
ar RT’ 
Sn Se, 
fo ( da 0 q 


the limiting value of van ’r Horr, whilst for 
v—=1 it passes into — oo. It may now 
still be asked, whether there will be a point 
of inflection or not. In the case, examined 
by vaN Herrren, a point of inflection plainly 
occurred at about « = 0.8, but it may also 
be possible, that the course was like the 
one in the following figure, without point 
of inflection. Let us therefore determine 
dT 

Fig. 2. dx? 


del re i Zie dh 1 jh 0 |: /) | 


0 0 0 


de (1H lop =a) (he). © NE NE 
en 

Evidently i —_=(, when 20= N, that is to say, when 
ax” 


te log (1—a2) = 20 


— log (1—«) iN 
: 0 
7 
As 0———~* will be positive, we see, that the point of inflection can 
qd 


(427 ) 


only occur if @ is situated between */, and oo. For 0='/,,a@=0; 
for 0=o we find on the other hand « = 0.865. A point of inflection 
further than «= 0.865 can only oceur with negative values for 0 
(A= till 0=0, when «= 0.865 till a—1). But there is no 
point of inflection if 6 << '/,, that is to say, if 


MEAT, 


q>A4T,. 
In our case therefore, where 7, = 505 — when q >> 2000 gram-cals. 
This last conclusion will however be modified, when we apply 
the necessary correction to the approximate formula (3). But the 
fact of the possible occurrence of a point of inflection may already be 
completely explained by the simple formula (3), and this by the course 
of the function log (4—2). 


or in gram-cals. 


II. We now proceed to write down a more stringent relation 
than (3). 

Assuming an equation of condition of the var per Waats’s kind, 
the value of gw, (the molecular potential of the component 7,) becomes 
as follows: 


y= kT (log TI) — RT (log (Vb) 1) + (eo. ie (1) EE 
SRT (12 y 
aes b, — 7 DIe a Ma OL OE 10 em se | 


For 6 has been written: 


bn bi ne bo Serkin 
whilst for a the quadratic relation 


ney a. Sieve 
== nN," a, + 2, N, dy, +... 


has been taken. 
Now, loy (V—+) can be supposed to be independent of w, whilst 
the expression 
hy okt L, a ) RE 2 
VEE ER a pr OG Fs) = ane ae ya eas) 


in regard to w will become not of the order, but of v?. Let us, to prove 


this, rather start from a more general expression for the total poten- 
tial § (in our case we have only to deal with two single components 
nm, and 7,), namely 


en ny (u) LN, (u) a 


2 EMG} 2 
a Un He 2 otd, + Ne Mss 


n, +n, 


ryy ny ny \ 
+ Ri ny log —_—. + ny log nn 
n,n, n,-+n, 


+ 


( 428 ) 
We then find: 


1 
w, — moe rie (n,+n,)? (n° Hy, Ae 2 NM, Ny Uy, = na. Mss) ain 


2 n 
- —(n nu RT lo —— 
. ER, 1 Yar Fo Mae) + aT 

With n, + n= 1, 2, Sd, n= we obtain: 
2, —(e,),-[G-2)"4, DE 2u(1-«)u,,+ Haal 20e), + ou} KT log(d- «), 
or after simplification: 

A = (). + bn) — AC — 2 tis + Uae) + RT log (1 — 2). 
In analogy with (4) we may therefore write: 
uw, me —e tT Ha, a? + RT log (l—e). 

The terms with 7'log T have not been taken into consideration, 

because they disappear on account of the equality of the quantities 


k, and Rin the liquid and in the solid phase. 


If, for the sake of a closer approximation, we take up some higher 


powers of «, we finally get: 


(solid tin) p=e—eL ; 
(tin in liquid amalg.) we T+ (0? Bye? +10) RT logde) 
Equating, we then find as in $ 1: s 


y T= — (art + Be +7, 0°) — RT log (lo), 


Yo 

or 
pta BEH) 
The heat of fusion of the solid tin in the amalgam is now plainly : 


Pen UT et Bef Nr ees (7) 
For «= 0, (6) passes into 


ZA Je 
1 = 3 
Y 
so we may again write: 


aat Be ye 
| — eM 


| 
pete EDE 
RT, 
1 — — log (1—2) 
Jo 
a 3 
or with — = 4; oi B, Les =e 

Yo Jo qo 


1-++ (ar?+ Ba’*+y2*) (8 
1—G log (le) EAT PAR, 


( 429 ) 


and this is the more accurate formula, which has taken the place of 
the simple relation (3). 


HI. We will now show, that the above formula quantitatively 
yields the values, found by van Hureren for 7’, in a satisfactory manner. 
dT 5 : 
As t= (|) = T, 0,0 may be determined with great aceuracy from 
ny. 
the beginning course of the meltingpoint-line. From the values, found 
for 7’ (on pg. 16 of the dissertation) for «=O atom "/, of mercury 


(pure tin), « = 0,1005, «= 0,1716 and » = 0,2338, the average value, 
obtained for — = is = 200. From the determinations of Hvycock and 
Av 
NEVILLE between «=O and «= 0,1 it also follows, that — En == 200; 
: Av 
For 0 we may therefore take (7, = 505): 
200 
6—-— = 0,4. 
505 o— 
I calculated the values of a, B and y as follows: 
ea el tel pet 1 ee 8: 


Formula (8) thus becomes: 

1+4(0,8250?—1,11e* + 1,33%) 
: PAV Aloo ( toon te FE 

and so we find the following values for 7. 

The agreement is as good as can be expected : the difference between 
the calculated value of 7’ and the observed value generally amounts 
to fractions of a degree, average 0°,8; as regards to the absolute 
temperatures the deviation is only average 0,2 °/,. Only the two last 
values are too low (the last 8 °/), but then the influence of a small 
inaccuracy in the determination of the coefficients 8 and y makes 
itself strongly felt. If we except these two last values, the calculated 
meltingpoint-line fully coincides with the observed line in the scale 
of the figure in the dissertation. And by means of a slight alter- 
ation in the value of 8 and y we might perhaps cause the two last 
observations to agree. Let us not forget, that the formula (8) 
always remains an approximate one. In the last values of z the 
composition of the separated tin must also make its influence felt. 
For this is no longer pure tin but contains certainly 1°/,, or perhaps 
even 6°/, of mercury. 

As regards the value of ¢ (the heat of fusion of tin, when passing into 

RT 1010 


0 


the amalgam) — when « — 0, q = q,, that is to say = —— = —— 
8 ) / / . () 0.4 


= 2550 gram-cals. At 25° our formula is no longer available, as 


El 


| 


ons O73 | 


ea a | de | vs ie fag A) Numer, | Denom. | ES 

| | | | | | | | 
0,1005 | 0,0101° | 0,001015.0,0001%| 0,1059 | 1,023 | 1,044 | 2194 | 211,6 | 08 
0,1716 | 0,0294 | 0,0050% 0,0008% | 01883 | 1,0051 | 1,0758 | 1989 | 198,6 | 0,3 
0,2338 | 0,0546 | 0,0127* 0,0029** | 0,2663 | 1,0076 | 1,1065 | 186,7 | 483,72 3,02 
0,2969  0,08815 | 0,02617 0,007" 0,3523 | 10099 | 1,1409| 173,8 | 1730 | 08 
03856 | 0/1487 0.0573" 0.02911 | 04872 | 40144 | 11949 | 155,4 | 155,9 | 0,9 
0,5001 02501 0,1251 (00625? 0,693 10256 12773 | 199,3 | 135,4 — 4,1 
0.5973 | 03568 | 02131 01273 | 09095 | 4,0488 | 1,3638 | 115,9 | 4152 0 

| | | | 
0,6467 | 0,182 0,2705 0,1749 10404 | 41,0682 | 1,4161 | 107,7 | 107,4 | 0,3 
0,6754 | 04562 — 0,3081 0,2081 41959 10830 14501 | 404,0 | 4034 | 0,6 
0,6813 © 0,4642 0.3162 0,2155 11435 | 1,0866 | 14574 | 1033 | 1024 | 0,9 
0,7104 | 0,5047 | 0,3585 '0,2547 19393 | 11047 | 4,4957 | 998 | 99,0 | 0,8 
0,7155 | 0,5119 0.3668 0,2620 1,2570 | 1,1083 | 4,5028 | 992 | 98,8 0% 
| | | | 

0,7477 | 0,5591 | 0,4480 0,31% | 4,3772 | 11935 | 14,5509} 95,9 | 95,4 | 0,5 
0,7547 | 0,5696 | 0,4299 03244 1,4053 | 1,1393 | 45621 | 95,1 94,0 | 4,1 
0,7963 | 0,634 | 0,5049 0,401 | 41,5912 | 41,1805 | 41,6365) 91,4 90,0 411 
0,8189 | 0,6706 | 0.5492 04497 | 4.7087 | 41,2064 1,6835 | 887 | 884 | 03 

| | | | 
0,8921 | 0,7958 | 0,7100 06333 | 2,926 1,318 1,8906 | 77,5 | 79,7 —22 
0,9483 | 0,8993 | 0,8598 0,8087 | 92,9693 | 41,4212 | 2,1849 | 55,3 | 65,2 ips: 

| | | | | | | | 


according to the above table it only yields trustworthy values for 7 
up to about 90°. At 90° r == 0,8, and then, according to (7), we have: 
g=Qll + (aa? + Ba? + yet], 

or q = q, {A 4- 0.325 wt — 1.11 a + 1.33 wf], 

that is to say gq == 1.185 gq, = 9020 gram-eals., 

whilst van HerereN (at 25°) found + 3000 gram cals, by means of 
electromotive measurements '). The concordance is absolute. 

We, finally, wish to remark, that according to the determinations 
of vaN HerrereN and of Hnycock and Nrvintin, regarding the lowering 
of the temperature of fusion of tin on adding small quantities of 
mercury, g, must be = 2550 cals. We therefore see, that the value, 
assigned by Prrson, namely 14.25 118.5 = 1690 gram cals., is much 
too small. In a later communication | will show, that the heat of fusion 
of mercury, given by Person, is also many times too small. 

Dec. 1902. 


1) Dissertation pg. 49. 


( 481 ) 


Chemistry. — “On the potential-difference, which occurs at the 
surface of contact of two different non-miscible liquids, in 
which a dissolved electrolyte has distributed itself.’ By Dr. J.J. 
van Laar. (Communicated by Prof. H. W. BaKuuis RoozuBoom.) 


(Communicated in the meeting of December 27, 1902.) 


|. It has already been demonstrated by Nernst!) in 1892, that 
a potential-difference must occur at the surface of contact of two 
liquids, which lie together in layers, such as for instance water and 
phenol, on account of the unequal distribution of the neutral molecules 
and the Ions of a dissolved electrolyte. It is true, that his expression 
for the electromotive force relates to the case, that one of the two 
phases is a so/id solution, but it will be perceived at once, that the 
same formula also applies to our case *). 

There is, however, at present no prospect of obtaining direct 
measurements of this potential-difference *). But as RiesenrEnp*) has 
lately been experimenting on the subject, although in another direc- 
tion, it may be as well to give the exact theory of the phenomenon, 
which I worked out about a year ago, when engaged in writing a 
book on electro-chemistry, which will be published later. 

Suppose we have a solution of KCl in the solvents A, and A, 


A, A, 
Vials rl. a eon 
| a C1) K | 
| Gi. Ollie, RER 
CIK 


If now equilibrium has been established between the non-dissociated, 
electrically neutral portions of the dissolved KCL in the two phases, 
there need not be equilibrium between the Zons in the two solvents. 
Indeed, equating the thermodynamic potentials for equivalent quanti- 
ties of the non-dissociated portions in the two phases (equilibrium 
of partition), we get: 


== zal 

Uc, — "xc. (1) 
But the two dissociation-equilibria give: 

=: JE a =f | Pre = aS Oh 2 

Crone eg, “ch, Pra Mie et gr (+) 

Consequently it will suffice if 
- = ~ AE TR ne ELC. 
Br + Bey = By, + UG), (5) 


1) Zeitschr. fiir Physik. Chemie 9, 137 (1892). 

2) Compare Rresenretp, Wied. Ann. (4) 8, 617 (1902). 

Sy bids dc 

4) Nernst und BurserreLp, Le. p. 600—608; Riesenrerp, 609—615; 616—624; 
id. Inaug. Diss., Göttingen 1901; Hrrrorr, Wied. Ann. (4) 9, 243—245 (1902). 


( 432 ) 


and it would be a sheer accident if we also had: 
Be = Bg i Bey = Hor 

There exists therefore as a rule no equilibrium of partition 
between the /ons in the two solvents. For example there may be 
in the second solvent relatively too few K-Ions, too many Cl-Ions. 
Since a system out of equilibrium tends to pass into a condition of 
equilibrium, K-lons from A, will migrate to A,, and remain there 
in the boundary-layer, while the corresponding liberated Cl-lons 
remain in the boundary-layer of A, (inversely Cl-lons will migrate 
from A, to A,, whilst the corresponding liberated K-lons remain in 
A,. Both add themselves to the above mentioned similar ions in the 
boundary-layer). The consequence is the occurrence of an electrical 
doublelayer and therefore of a potential-difference. And it is this 
potential-difference, which will restore the originally non-existing 
equilibrium between the Tons. 

All this may be put into a very simple mathematical form. 

Let V, be the electrical potential of A,, V, that of A,, so that 
A= V,—V, represents the potential-difference at the boundary (in 
the case we are dealing with, 4 is therefore positive), then the 
formula for the equilibrium of the K-lons will be: 

HP, 
aaa 


de + Ade=0, 


which is at once obvious, when we consider the virtual passage 
from the left to the right over the boundary of such a quantity of 
K-Ions, that the quantity of electricity transported is de. As the 
quantities pg relate to equivalent-quantities, and as these do not cor- 
respond with one electric unit, but with ¢ (= 96530) electric units, 


IH, must be divided by «. 
Ky Ky . . . k Dn, 
For the equilibrium of the Cl-lons we find in the same manner: 


ea Js 
EA Ee — À de —= 0. 


& 
The sign at 4 is now negative, because on account of the negative 

charge the change in the electrical energy is — 4 de. 
We therefore obtain from the two relations, after dividing by de: 
ih a Ee ee 

é é 
That these two equations for A are not conflicting, is at once 
apparent. For the relation, resulting therefrom 

u 


LE NT tn 


leads at once to (3). 


ET 


( 438) 


If we introduce: 
— u + yc A log Cy 


in which e is the concentration of the Tons, we may also write: 


A LAs ee 
cece (u Kk Ki + RT log =| 


) 


\ 1 ! ! ry eo 
A= (Www) + RT log — 
€ Cl, Ch b CCh 
Il. Now everywhere cx =cq (only in the boundary-layer an 
excess of positive or negative Tons is present, owing to the for- 
mation of the doublelayer), therefore also 
ON ho Clg 
as B) 
EK, Gen 
and so we find’) by addition of the two equations (5): 


A Wato) — gt) | Me elo GC) 

From this last relation it follows at once, that in d/ute solutions, 

where the quantities w are almost independent of the concentration, 

the potential-difference A will be also independent of the concentration. 

Whether much or little KCl is distributed through the two solvents, 
we will always notice about the same potential-difference A. 

If we deduet the two equations from each other instead of adding, 


: d AE Gan 
then we obtain | observing that — = — |: 
Cp Us 
RT tog Me = — | (uly 0) + Wl (7) 
te ee Cle Ch “Fan Aa baa Soar 
1 
If now we put 
! ! ait ry > 
U Ur = RT log ee | 


(a) 


1 f hes p Es Al dd 3 
WT ber = RT log Kn | 


in which Ag and Ke, are quantities, which depend on the nature 
of the two solvents (and which in difute solutions will only be fune- 


tions of temperature) — they are the so-called partition-coefficients 
of the positive and negative Ions — then (6) and (7) pass into 
E Key a | 
A = — log — gr SAPS Ae pty ee sad er OG 
2e Kk 


EK, i 
(EE) = kx Ka. OTN NOM iP a oe Ae ACER) 


1) The formula (6) was given already, though with a somewhat different notation, 
by Luruer [Z. f. Ph. Ch. 19, 537 (1896)]. The first thermodynamic theory of the 
equilibrium of partition was given by me in a paper of 1895 (Z. f. Ph. Ch. 18, 264—267), 

29 


Proceedings Royal Acad. Amsterdam. Vol. V. 


(434 ) 


Nernst’s formula for A, obtained in a different manner, is identical 
with our formula (5). (As Nernst's # = V,—V,, our A= -— EK). 


F 5 . 5 ‘epl: x ! aa - 4 ee : ! Eel E 
or if we replac Wir, by RT log Kp and Wor Wer by 


RT log Kor, then (5) passes into 

jk KS RT HG 

ha log KK — — —— log Ke —, 
é oh: é CCL, 


and this is Nerrsr’s expression. As has already been observed, the 
quantities Kp and Ay; are the so-called ““partition-coefficients” of the 
positive and negative Ions. For instance for the positive lons we should 
have, when equilibrium of partition occurs: 


HT Ur, = 0, 


or 
an A 
u Et K, + RI log ce =a): 
1 
int 2 
so that we obtain = Kx. The same for the negative Ions. 


Ky 
The relation, given by Nernst *) 


C 
> > 45 | are 
Kx X Ka=  X Axe, 
in which Ae, is the coefficient of partition of the neutral KCI- 
molecules, and C, and C, are the dissociationconstants in the two phases, 
follows directly from the thermodynamical meaning of these quantities. 
For if we write this relation in the form 
RT [log Kx + log Kei] — RT [log C, — log C, + log Kxcr), 
it passes, taking into account equation («) and the relations 
RT log C, =e 


ad Al es ! ee, ! 7 5 il ' = ! . 
RP log Kro ro xe, KOE eo Ck? 
RT loy C, = u 


! ! 
co, “x; Eat 


immediately into the identity 
! ! ! ! 2e ' i 
wt x) +o, a= Ko, 


rae 6 4 Lie 


' 


tee 


Not the formula (5), but the formula (6) or (6a), derived by us from 
(5), deserves however the preference, because the concentrations of 
the Ions have been eliminated therein, and an expression has been 
obtained, in which only the coefficients of partition Ap and Ary occur. 


' ! ! ! 
keh Er Wer) HW xe mE Ke 1: 


HI. If the dissolved electrolyte has now distributed itself so, that 


1) Z. f. Ph. Ch. 8, 138 (1891). 


the total concentration is c, in A, and ec, in A,, we shall have: 
CK, =S OC, 5 EK, == A, Cio 

in which the quantities c, and c, may be found by chemical analysis, 

and «, and a, by determinations of the conductivity. As soon as 4 


- 


Ke 
can be determined by experiment, KR, may be calculated from the 
K 


equation (6a), and Ax & Ker from (7a), and we can therefore get 
to know separately the quantities Ap and A, consequently also 
the quantities 

UK, — UK, and wo, — uci, - 

From (6a) it further follows, that A will be positive (as supposed 
in the figure), when 

Ko > Kx. 

Only when by accident Acj=Kx, A can be 0. In general a 
potential difference will always oceur between two non-miscible solvents, 
when an electrolyte is partitioned between them. This potential-difference 
is given by (6a). 

From the equation (7a) it follows, that the relation of the concen- 
trations of the Jons in the two solvents in the case of d/ute solutions 
will be practically independent of the total concentrations. This 
equation may also be deduced directly from (3). For this, being a 
result of (1) and (2), that is to say of the equilibrium of partition 
and the two equilibria of dissociation, may be written : 

wu) (uu) == RT u “Ky + log = | 
ea K, are oh EA “Ect, : 
and this after substitution passes at once into (7a). For 


CK. Fol. We Ek 
2 1 log — = 2 log — = — log | — |. 
CK, EC | 1 Ch t CK . 


The equations (6a) and (7a) moreover lead to an important conclusion. 
As the quantities Kp and Aj are, in the case of di/ute solutions, 
specific quantities, we must therefore find about the same values for 
these quantities in the case of other salts, when employing the same 
solvents A, and A,. For NaCl for instance we will have: 
Ee 1 ee 
RI ig et. & ) NE 
C Nas 
from which by experimental determination of A' and the quantities 
Cya, and Cy, , the two quantities Kva and Kc, may be determined. 
The value, found for A, from KCl-solutions in A, and A,, must 
then be practically sdentical with the value for K/, determined from 
solutions of NaCl in these solvents. 


log 


29* 


( 436 ) 


The quantities 4 will show an almost complete additive character, 
on account of Ag and A/ being independent of the concentration 
in the ease of dilute solutions. For instance, in the same solvents 
A, and A, we must find: 

Axci—4Anact = Okno,—4ONaNo, « 
And the same for other combinations. 

The above considerations may be readily extended to the case of 
non-binary electrolytes such as CaCl,, ZnCl,, ete. In the different 
equations the valencies » of the Ions will then also occur, because 
the fundamental relation (4) then passes into the more general one: 


$+ $+ = = 


u, u, U, 
AN re 
+ = 


VE VE 


IV. The question in how far and in what manner the value of 


A, given in (6) or (64), is still dependent on the concentrations of 
the Ions, can only be answered, when we calculate the values of me 
A1 


ete. with the aid of an equation of condition. If we accept the 
equation of van per Waars as also applying to liquid-phases, we 
obtain for instance for the molecules Np: 


V—b 
Th ky T (log T—1) — RT (1 zee 1) vn [ed pol si 
1 
-{- nel zn, b,— 2 (” aj J- DEE -}- ms) 2 RT log df 
ae Re ae A age a 


n, stands here for the molecular number of the solvent. For 6 
and a@ we write: 
bb Fn, bd me 
anja de And Ars eS Ny My ln onee 
Let us now calculate the value of 
Wo Ho) — W Pam Kx) 
or, what amounts to the same, of 
(nl mk mn Cy): 
If we indicate the solvent by the index 1, the non-dissociated KCl, 
dissolved therein, by 2, the two Ions by 3 and 4, we obtain for 


u Pa a the expression 
TIE Ns —k,) if (log Th) == (ede) -T ( (1)5)0)—(74)0) | ale 


9 
hen ET oy pln (as daa) he N, (43242) zen (253-443) +, (G54-44,1- 


( 437 ) 


Remembering, that », =n 
simplified to 


4» &,=> djs the last term may be 


2 
= pe 
a rae (ii di) + 2, (daa Bia) tr %; (a,,—4,,)]. 
For w.—wv', we find a similar expression. In this, however 
Ka Cis ae ; Xpression. Ss, however, 


the quantities /,, 4, (the heat-capacities of the same Ions, at infinite 
volume) and (@s)o. (@4)o> (sor (14), (the energy and entropy-constants 
of these Ions) will be exactly the same. a,,,4,,, A and a,, will also 
remain unaltered, so that for the difference Wi Wo) — WW) 


we may write: 


PF bec Dr ETA (nasa) (dpd) 
he en evo |—2] ( RE RA ) i 


Ne te Ns n', 
+ (452-445) TUD + (a;,-4,,) aos 


The quantities, relating to the second solvent, are indicated by 
accents. 


We may now go a step further and accept as a first approximation: 


En ! a ! 8 Tey 
b=}, D=, a, =a, 
If we then also write 
V V' n 
ee ree eer Oe yt My = 70 (es = ae NERC es 
1, u, n, 


we finally obtain for A: 


Rie ule ear gaan ys LL nd 2 
A = ( 31 3 Me 41 „ad, tai a ) { (ago) (} sa =e ( at) )I (65) 
€ v Uv v v 


HEAD en (leeren 
As, in consequence of the equilibrium of partition, tappen, is 
—— IC 
constant, 4 will have the form 
A = as 4- A (l—a)e, 
Aert ra Mee kate ac)” 
or since, on account of the equilibrium of dissociation, tay = 
IG 


constant, also the form 
A= Ay 4 (ei. 


Whether 4 will be positive or negative, depends chiefly on A, If 


! 
Uzi TT 4, @5,;— Gay 
meee 


v v 


A will be positive. We also see, that A—A, will increase or decrease 
with the second power of «ec, that is to say in the case of strongly 
dissociated electrolytes, where « is nearly 1, almost with c’. 


Dec. 1902, 


( 438 ) 


Physics. — Dr. J. J. Harro: “The value of some magneto-optic 
constants.” (Communicated by Prof. P. Zeeman). 


In my doctoral thesis, on The magnetic rotation of the plane of 
polarisation in the neighbourhood of an absorption-band 5, T have cal- 
culated the values which three of the constants, occurring in Vorct’s 
theory of magneto-optie phenomena, assume ina particular case. I did 
not then know as yet, that Drvpr had already tried — in his Lehrbuch 
der Optik (Leipzig, 1900) — to make some estimate as to the order 
of magnitude of a constant 7, introduced by him, which is connected 
in a simple manner with one of the constants of Vorer’s theory, of 
which I have determined the value. Therefore I beg to be allowed 
to mention here my results and those of Drupn, and to examine in 
how far these results agree. 

If X, 9, 3 are the components of the electric polarisation in some 
medium, Voigr assumes that every one of these components exists 
of a part X, Y, Z, relating to the free ether, and a series of other 
parts X,, Dj, 31, indicating the state of the ponderable matter. He 
therefore assumes: 


EKL SE ete: 

A representation of the phenomena of selective absorption, in which 
the influence of a magnetic field with components A, B, C is also 
taken into account, is gained when the sets of vector-components 
A, B, C are subjected to the conditions: 

VP A2 § A 
Er + ay Bal + by, OE + ¢y (ci —_ B =) = Bj, ONG ues 
Ot dt t 

The constant Dj, appears to be equal to 7,7/42°, if ty, is the vibratory 
period of a free vibration of the absorbing medium; I have derived 
the values of the constants aj, cy and ej, for the line D, from the 
results of my measurements in a particular case (for a flame which 
contained very much sodium); the values I have found are (vide 
p. 85 of my thesis): 

Urd SAlOrete 
0 02. Osea 
Sy Wee 10a ae 

The constants a, and «, depend on the density of the sodium- 
vapour in the flame, the constant c, does not so far as we know. 

The data which served for the calculation of these constants are 
the following: «a, was calculated from the width of the absorption- 


1) Amsterdam, 1902. 


( 439%) 


band, which is proportional to it; this width was about 1 Angstrém 
Unit; c, was caleulated from the magnitude of the Zreman-effect ; 


for this magnitude in the field which I used — of 9000 C.G.S. 
Units — I took '/,, part of the interval between the two sodium- 


lines; e‚ was calculated from the value of the rotation of the plane 
of polarisation in the neighbourhood of the absorption-band; on the 
magnitude of this rotation as a function of the wavelength, for dif- 
ferent intensities of the magnetic field and different widths of the 
absorption-bands, I have made measurements of which the results 
have been recorded in the tables given in my thesis. From these 
tables I shall quote one series here, giving the numbers from which 
the above-mentioned value of e, was deduced (vide p. 42 of my 
thesis, table 24 1): 


d Bas x 

| | 
15 88 50 11 
20 51 55 10 
25 31 60 9 
30 23 65 8 
35 18 70 6 
40 14 75 5 
AD Thies 


Here dis proportional to the difference between the wavelength 
of a given kind of light and the wavelength which corresponds with 
the middle of the line D,; the coefficient of proportion may be found 
from the fact that the difference between the wavelengths of the two 
sodiumlines corresponds with a value d= 1380; x represents the 
rotation of that particular kind of light in my experiments, expressed 
in a unit of which the value is determined by the fact that a rotation 
of 180° corresponds with a value y= 105. Thus we read from the 
series, given above, that for a value of d corresponding with 
35 18 
<6 A. U. the rotation of the plane of polarisation is aT 507; 


130 
from these corresponding numbers the value of e, is deduced in the 
way which I explained in my thesis. 

Drove, in his Lehrbuch der Optik which 1 mentioned above (p. 353), 
in his version of the theory of dispersion gives the equations of 
motion of an electron in the form: 


dS Ane? ds 


nae Sr. 


Ot 

Here m is the mass, e the charge of the electron, § its displacement 
parallel to the axis of X from a position of equilibrium, A the com- 
ponent parallel to this axis of the external electric force acting on 
the electron; 7 and 9 are positive constants. 

In working out the theory it appears that Voier’s constant aj 1s 
identical with the expression 7/4a of Drupe. Now the value of 3 
was calculated by Drupr himself (p. 490) from the vibratory period 
of the sodiumlines; he finds the value of this constant to be 7,6 . 10-27; 
from this value and that of Vorier’s constant a, which I mentioned 
just now, we find: 


r= 16502 
here we must bear in mind that this value applies to the particular 
sodiumflame to which my measurements relate; 7 must, as well as 
dj, depend on the density of the sodiumvapour in the flame. 

Drupe tries in his book to fix limits, between which the value of 
r must lie. He finds a lower limit by deducing from theory the 
proportion between the quantity of light, which the absorbing sodium- 
flame itself begins to emit under the influence of incident radiation, 
and the quantity of incident light which is absorbed. This proportion 
he finds to be 0,126/r. From the fact that reversal of a sodiumline 
is possible, he concludes that this proportion must be considerably 
smaller than 1, and he therefore fixes the lower limit for the value 
of 7 by assuming: 

ro >A. 

A higher limit is found by Drupr from the consideration of the 
phenomena of interference. He deduces theoretically the value of the 
coefficient of damping y of the free vibrations of the electron and 
finds for this: | 

y=0,6.r. 107. 

Now this coefficient must be small, as with great phase-differences 
interference-phenomena can still be observed. With sodiumlight inter- 
ference-phenomena have been observed with a phase-difference cor- 
responding with 200000 wavelengths; therefore 200000 y must still be 
smaller than 1, therefore in this case: 


mz 100; 

It is evident that this result is not at all incompatible with the 
value of # which I caleulated above. In order to observe interference- 
phenomena with such great phase-differences it has been necessary 
to use a source of light showing very narrow sodiumlines; with 


( 441 ) 


the width of the sodiumlines to which my measurements relate 
(which was about 1 Angstrém-Unit) the greatest phase-difference with 
which interference-phenomena can be observed is one corresponding 
with 3000 wavelengths; the higher limit is therefore raised to 7000, 
so that 7 must in this case lie between 10 and 7000, which it 
really does according to the calculations given above. 

Some further deductions which can be made from the comparison 
of Vorer’s equations with those given by Drupe, have already been given 
on pp. 90—95 of my doctoral thesis, with reference to LorENtz’s 
paper in the Report of the Congres International de Physique, held 
in Paris in 1900, and I will here only refer the reader to that part 
of my thesis. 


Physiology. — “A new law concerning the relation between stimulus 
and effect.’ V. By Dr. J. K. A. WERTHEIM SALOMONSON. 
(Communicated by Prof. C. WINKLER.) 


From the law connecting excitation and effect, 


BAL eee EA Ee EAR ence at 10 
we may obtain by differentiating 
dE 


ees Apt BRO) 


or also 
LE end 
diss BRO MN A eect a) (E 
1B 


Introducing differences instead of differentials, with this limitation 
that the differences should be very small, and taking according to 
Frcuner, AZ, the differential sensation-threshold as a constant quan- 
tity, we obtain 

WR By BORON SA tae | pedis (Ards, Dae 
or, by putting the constant e~2°k, =k 
AR Rell Wet urine tte tea ate OOS) 
the latter formula containing an expression for the absolute differen- 
tial threshold-value. We might employ this formula for psychical 
impressions of peripheral stimuli, if the peripheral stimulus had caused 
excitation of only peripheral neurones with equal stimulation-constants 
B, and moreover if all these neurones had been uniformly stimu- 
lated. Under a similar limitation we might also admit the validity of 
the formula for the relative differential threshold-value deduced from 
(4) by dividing both terms by A; we then obtain: 


( 443 ) 
BR 

at ie ed nr Oe cans ae ee 
R R 


As a rule, however, this formula may not be applied in the 
ease of psychical processes, because the above-stated conditions have 
not been fulfilled. It is impossible to suppose the case of a peripheral 
stimulus hitting only one single peripheral neuron, or of one single 
group of neurones being exposed uniformly and with equal force to 
that stimulus. 

Let us see, what happens when a sense-organ in the living human 
organism is subjected to a stimulus. For instance we may consider 
the action of pressure on the skin. 

Suppose the compressing object to be in contact with a limited 
surface of the skin at the moment the pressure commences. We 
may take it for granted that all end- 
organs situated within the limited skin- 
fo hoses oOo. | surface in direct contact with the com- 
lao 0 4.0%0 ©) pressing object, undergo an equal and 
ba AO B 0 uniform pressure, and that in the case 
| | of this pressure being increased, its action 
will remain uniform. To the neurones con- 
nected with the nerve terminations «, ‚aA, 
our deduced law (5) may be therefore 
applied. As soon as the pressure increases 


the skin-surface will undergo a change 
of shape and be compressed (see fig. 1). 
This implies that nerve-endings 4, 4, situ- 
ated outside of the originally compressed 
surface, will also enter into an excitatory 
state. If this deformation be a slight one, 

Fig. 1. only the nearest end-organs 4, will be 
compressed. By increased pressure the more distantly situated ones 


c, c, d, d ete. will also be stimulated. To all these end-organs, 
situated outside of the originally compressed surface, impulses are 
given, which are conducted to the central nervous system. From all 
the combined impressions finally results the sensation by which our 
judgment is decided. 

The neurones connected with 6,4 c,¢ d,d ete. will likewise obey 
the law of stimulation and effect. The intensity of stimulus however 
is different for all these neurones, and also different from that for the 
neurones «a, a, a. Therefore, whilst for the neurones aaa, the expression 

dR EBR 
: R R 


( 443 ) 


might be employed, we must use for the neura 6,4 e‚e d,d etc. 
the expression 
5 ebr je bry _eBry 
9, = K—_, 9, = K—, OC, ue 


ry "s us 


As the stimuli 7,, 7 
stitute for these m,R, m,R, m,F ete. 


etc. 


"> 7, ete. are proportional to #, we may sub- 

The question arises next: how shall we psychically combine these 
impressions in order to make use of them for the special purpose 
aimed at by our experiment, i.e. to decide whether two stimuli are 
different from one another? Summation or addition is out of the 
question: this would be in contradiction with the experience that by 
fixing our attention on a definite sensation, other sensations are 
weakened. It is clear that we will conform our judgment to that part 
of the’ sensation that is best fit for our purpose. Starting from this 
fact we may continue to treat the question mathematically. 

In the first place it ought to be taken into consideration, that by 
increment of a stimulus not a small number of new peripheral 
neurones are stimulated, but generally a great many. In the case 
of a pressure e.g. not only nerve-endings lying sideways of the 
compressed surface, but also more profoundly situated end-organs 
will be acted upon by increased intensity of stimulus. For every 
individual neuron we shall have to put in another coefficient m. If 


Fig. 2. 


we construct therefore a great many curves @,, 0,, 0, all these curves 
will only be different on account of the constant m being changed. 
We now suppose the final judgment fixed each time by a part of 


a farther situated curve. Thence it may be concluded, that the 


( 444 j 


enveloping curve will represent the manner in which a judgment 
about the final result originates. To obtain the envelope of the 


enb 
group of curves 9 = K Th if the constant 7 is changed, we put: 
embh 
RD ea ae) Pe ae AD 
2» mR (6) 
or 
Caleulatine the value of mz corresponding to —- — 0, and substi- . 
o Lee 
UL 


tuting this value into the equation £’— 0, we find the formula for 


the enveloping curve. We may state: 


ol’ K pp mMBR—1 
— = — —, BR) , 2... «= (%#) 
Om Rk m 


? 
By at 


Oa KBE NA AN he ee eee 
proving that the relative differential thresholdvalue is constant. 

3y this process we have deduced from our formula the law of 
WEBER. 

From our deduction may be inferred that the area, wherein the 
law of Weber prevails, is a limited one. ‘The validity of this law 
commences within the area of the enveloping curve, and a look on 
the figure 2, will make it clear that the first part of the whole 


as 


From which follows m — an which substituted into “= 0, gives: 


sensation-curve is given by the descending part of the curve 


BR 
é yeh 
Kn: The horizontal part then represents the area within 
L 


the limits of which the law of WeBeEr prevails, whilst in the case of 
very great intensities of stimuli the ascending part of the curve 
ebmk 


= Ke 
m 


will appear. 


There remains still another conclusion to be drawn from our 
deduction. This latter was founded on the supposition that the inerement- 
constant B was the same for all stimulated neurones. This, however, 
is highly improbable: in the most favourable cases we may only 
suppose that the A-coefficient of the homogenous neurones will 
possess approximatively the same value, from which follows that 
we may admit the law of Wesrr at best as an approximation. 

Finally it may be mentioned here that apart from the above- 
demonstrated correction for obtaining an approximation in the diree- 
tion of the law of WeBnr-FrcrNeR, probably still another means of 
correction exists in some of our sense-organs; | shall prove this in a 


later Communication. 


r N 5 ie 
A EATERS, 
® fi 


D. J. Korreweo. On plaitpoints and the corresponding plaits in the neighbourhood of the sides of the Wesurface of VAN DER WAALS. 


SIDE OF THE LARGE VOLUMES, 


Temperature slightly lower than the 
critical temperature of the solvent. 


Fig. 1. 


SIDE OF THE LARGE VOLUMES. 


‘Temperature slightly higher than the 
critical temperature of the solvent. 


Case 2. Case 6. 


Case 3. Case 


Case 4. 


Case 8. Absent. 


—— _ 


The figures relate to the v, # diagram. 


K is the critical point of the solvent. 
P the plaitpoint. 
R the critical point of contact 
KP indicates the direction of the plait- 
point curve. 


The traced curve represents the 
connodal curve. 


The dotted curve represents the 
spinodal curve. 


| 


( 445 ) 


Physics. — “Plaitpoints and corresponding plaits in the neighbour- 
hood of the sides of the W-surfuce of VAN DER Waars.” By 
Prof. D. J. Korrewee. 


(Communicated in the Meeting of December 27, 1902). 


First Descrirtive Parr. 


1. As in my “Théorie générale des plis”  T wish to precede in 
this paper the demonstrating part by a short summary of the 
obtained results. 

As we know a plaitpoint may occur on the side «=O of the 
y-surface of VAN DER WAALS, *) which is represented by the equation: 


w= - MRT log( v—b,) — i + MRT be log u+(1—«) log (1—z)} (i) 
DvD 


where: 
a,—=a,(1—«)?+2 a, o(1-wx)-+ a, «’? =a, +2(,4,-a,)e+ (a, Ha,-2 ,a,)a?,. . (2) 
b,=b,(1-#)? +2 ,b, elle) Hb, #?=b, + 2(,b,-b,)e+(b,+6,-2 ,b,)u?, . . (8) 

This occurs only in the case that the temperature 7’ corresponds 
with the critical 7; of the principal component; but in that case it 
occurs always. This plaitpoint coincides with the critical point of the 
principal component for which v= 36, and which in our figures we 
shall always represent by the symbol A; the plaitpoint itself will 
be represented by LP. 

If the temperature varies, the plaitpoint and the corresponding 
plait can in general behave in two quite different ways. It will 
namely either, as is indicated by the jist four cases on fig. I of the 
plate, on which the (v, 2) projections of the sides of the wp-surface are 
represented, at increase of temperature leave the v-axis and move 
to the inner side, therefore entering the surface, and disappear 
from the surface at decrease of temperature, or it will as in the 
last four cases of that figure, enter the surface at decrease and leave 
it at increase of temperature. 

1) Archives Neérlandaises, T. 24 (1891) p. 295—368: La théorie générale des 
plis et la surface # de van per Waars dans le cas de symétrie. See there 
p. 320—368. 

2) We take here the equation of the J-surface as it has been originally derived 
by van per Waars, so without the empiric corrections which seem to be required 
to make the results agree quantitatively better with the experimental data. So is, 
for instance, @z considered to be independent of the temperature, and all the results 
and formulae mentioned are founded on this supposition. It would not have been 
difficult to take such empiric corrections into account, as has really been done by 
VerscHAFFELT and Kersom in their papers, to which we shall presently refer; but 


then the results were of course not so easily surveyed. Therefore | have preferred 
to leave them out of account, at least for the present. 


( 446. ) 


And this different behaviour of the plaitpoint will necessarily be 
accompanied by a different behaviour of the connodal and spinodal 
curves. For they must always cut the v-axis at decrease of temper- 
ature, the connodal in the points of contact of the double tangent 
of the w,v-curve of the principal component, the spinodal in its two 
points of inflection; at increase of temperature above the critical 
temperature of the principal component, however, they get quite 
detached from the y-axis. In connection with this they turn in the 
first four cases of fig. 1 their convex sides, in the last four cases 
their concave sides towards the side «=O of the w-surface as is 
also indicated in the figure, where the connodal curves are traced, 
the spinodal curves dotted. 
cc At decrease of temperature a figure originates in the /irst 
four cases as is schematically given here in Fig. a. At 
increase of temperature, on the contrary, in the fast four 
cases, the spinodal and connodal curves disappear from the 
surface at the same time with the plaitpoint itself. 

Besides to this different behaviour it appeared however 
desirable, to pay attention to two other circumstances. /irst 
to the direction of the tangent in the plaitpoint, whether 
if prolonged towards the side of the large volumes, it 
inclines to the immer side of the y-surface, as in cases 1, 2, 5 and 
6 of fig. 1, or whether it inclines to the outer side, as in the 
remaining four cases. For on this it will depend which of the two 
kinds of retrograde condensation will eventually appear *). But besides 
we have to pay attention to the question whether the plaitpoint, 
entering the y-surface, either at decrease or increase of temperature, 
will move towards the side of the larger volumes as in cases 1, 3,5 
and 7, or whether it will move towards that of the smaller volumes 
as in the other cases. In connection with this question we may point 
out here that the line KP in fig 1 of the plate may everywhere be 
considered as a small chord of the plaitpoint curve of the v,-diagram 
and accordingly indicates the initial direction of that curve, which it 
has when starting from point A. 


The three different alternatives, which we have distinguished in 
this way, give rise to the eight cases represented in fig. J, and we 
may now raise the question on what it will depend which of these 
eight cases will occur at a given principal component with a given 


1) See on these two kinds of retrograde condensation inter alia, the paper of VAN DER 
Waars: “Statique des fluides (Mélanges): im Tome | of the “Rapports présentés 


au congrès international de physique, réuni à Paris en 1900”, page 606—609. 


( 447 ) 


admixture ; of course only in so far as with sufficient approximation the 
conditions are satisfied on which the derivation of the equation (1) 
of VAN DER WAALS rests. 


2. The answer to this question is given in the graphical repre- 
sentation of fig. 2. If appears, namely, that the case which will oceur, 
by 2 


. . ODE ( ) d 
is exclusively determined by the quantities — =x and Zot which 
a ) 


1 1 
have already played a prominent part in my above mentioned 
“Théorie générale des plis.” 

In accordance with this a x- and a y-axis are assumed in fig. 2 
of the plate and the regions where the points are situated whose x- 
and y-values give rise to the appearance of each of these cases, are 
distinguished by different numbers and colours. 

For instance the white region 1 indicates the x- and y-values for 
which the plaitpoint enters the y-surface at rising temperature, moving 
from A to the side of the large volumes, while in the well-known 
way we can derive from its situation on the connodal curve on the 
right above the critical point of contact A (for which the tangent 
to the connodal curve runs parallel with the v-axis) that the retrograde 
condensation will be eventually of the second kind i.e. with tem- 
porary formation of vapour) and also that the temporary vapour 
phase will have a larger amount of admixture than the permanent 
denser phase. 

In the same way the blue field 5 indicates the x- and the y-values 
for which the plaitpoint enters the p-surface at decrease of temperature, 
moving towards the side of the large volumes; whilst the retrograde 
condensation will be of the first kind and the temporary denser phase 
will show a smaller proportion of admixture than the permanent 
vapour phase. 


3. When examining this graphical representation we see at once 
that one of the eight regions which were a priori to be expected, region 8, 
fails. From this follows that for normal substances the combination 
of retrograde condensation of the second kind and of a plaitpoint 
which enters the surface at decreasing temperature and moves towards 
the side of the small volumes, is not to be expected. 

All the other seven regions, however, are represented in the graphical 
representation. 


4. Further the point x= 1, y= 1, is remarkable, where no less 
than six regions meet. This point represents really a very particular 


( 448 ) 


case, namely that in which the molecules of the admixture, both 
with regard to volume and to attraction, behave towards the mole- 
cules of the principal component exactly as if they were identical 
with these latter molecules. 

If at the same time a, —a,, 6,=06,, which is of course not 
involved in the above suppositions, it is easy to see that at decrease 
of temperature below the critical temperature the plait would suddenly 
appear all over the whole breadth of the tp-surface. 

Now it is true that every deviation from these equalities a, =a,, 
h,=6, will prevent such a way of appearance, but it is evident 
that then the behaviour of plaitpoint and corresponding plait will 
depend on a, and #4,, ie. the first approximation for which the 
knowledge of x and y is sufficient and which everywhere else 
suffices to make this behaviour known to us up to a certain distance 
from the side of the w-surface, fails here. 

And also already in the neighbourhood of the combination of the 
values *=1,y=1, this first approximation will be restricted, to 
the immediate neighbourhood of the point A’ and of the critical 
temperature 7), of the principal component. When we are not in 


that immediate neighbourhood the influence of a, and 6,, — of the 
former of these quantities specially, — will soon be felt. On the 


contrary for values of x or y sufficiently differing from unity the 
considerations derived from the first approximation will probably be 
of foree within pretty wide limits, at least in a qualitative sense. 


5. Before proceeding to a discussion of the border curves between 
the different regions, we will shortly point out that we cannot 
attach an equally great importance to all the parts of the graphical 
representation. So all points lying left of the y-axis relate to negative 
values of ,a,, Le. to the case that the molecules of principal com- 
ponent and admixture should repel each other, which is not likely 
fo occur. 

In the same way the negative values of y, so of ,/,, of the points 
below the z-axis, should be considered as having exclusively mathe- 


1 
matical signification. If the relation, ,6,— = (0. +4,); should still be 


applied also for very unequal values of the ’s, then y would even remain 
1 
2 


mk 


always larger than and so the part below the line y = 


2, 
would lose its physical signification. 

6. With regard to the border curves between the different parts, 
we have first to deal with the parabolic border curve separating the 


de at 


( 449 ) 


regions containing blue (blue, green, purple) from the others. It 


, ! Bah. 
touches the y-axis in the point x= 0, y= >. Its equation is: 


(2y—3x-+ 1)? — 8 (y—x) = 0 
or if we transfer the origin to the point y=1, x=1 and therefore 


introduce the new variables: x’ = x—1; y’ = y—1, which brings 
about a simplification also for the other border curves, we get: 
(By Sy =O. ts (Á) 


Then we have everywhere inside that parabola, so in the regions 
BOA: 

Orte 8 —x) 0 
and outside it in the regions 1, 2, 3, 4: 
(2y 4x) — 8 (y'—z') > 0. 

In consequence of this it depends on the situation inside or 
outside the parabola, whether on the corresponding w-surface the 
plaitpoint will enter the surface at decrease of temperature or at 
merease of temperature and whether the spinodal curves turn their 
convex or their concave sides to the side «= 0. 

Fig. b. For points on the parabolic border curve the plaitpoint 
occurring in the point A at the critical temperature of 
the principal component, is to be considered as an homo- 
geneous double plaitpoint at that moment. The projection 
on the v, w-surface appears then as is indicated in fig. 0. 

How the transition to this condition takes place may 
be made clear by the subjoined fig. c, which represents 
the same projection for a temperature slightly below that 
of the critical temperature of the principal component 
for the case that the x- and y-values indicate a Fig. c. 
point, which is still situated in the green region 
6, but on the verge of the border curve of the 
yellow region 2. 

Very near the plaitpoint P we find here already pg 
a second plaitpoint ?’, which at further decrease 
of temperature soon coincides with 7. 


If now the point in the green region approaches 


the border curve of the yellow region, the two 
points P? coincide nearer and nearer to the critical 
temperature of the principal component and to the point A. On 
the border curve it takes place in the point A’ itself. Beyond the 
limit, in the yellow region, the plait of ? does not develop any 
more and P’ takes the place of P. 

30 


Proceedings Royal Acad. Amsterdam. Vol. Y. 


( 450 ) 


7. As second border we get in the graphical representation the 
straight line: 


DE DE SA Ee eV 
It separates the regions containing red 3, 4 and 7, — for which 


2 y’—3 x’<0, and where the tangent in the plaitpoint, continued in 
the direction of the large volumes, inclines towards the side c—=0— 
from the others, where it inclines to the inner side of the w-surface. 

As we saw before, this inclination determines the nature of the 
retrograde condensation. Not exclusively, however. For in the first 
four cases of figure 2 the result of the same way of inclination 1s 
in this regard exactly the opposite of that in the last four cases ; 
henee the parabolic border curve acts here also as a separating curve; 
so that retrograde condensation of the first kind (i.e. with temporary 
formation of the denser phase) occurs in the regions 3, 4, 5 and 6, 
in the two first with greater proportion of the admixture in the 
temporary phase, in the two last the reverse, and on the contrary 
retrograde condensation of the second kind in the regions 1 and 2 
(with a larger proportion in the temporary less dense phase) and 7 
(with a smaller proportion in that same phage). 


8. The third border curve is a eubie curve with the equation: 
(2 7'—3 x’)? —4(4y7'—3 x’) (2 y'—3 x) +164 =0. . . (6) 

It eonsists of two branches, which possess both on one side the 
common asymptote : 

DE pee ee OE OE eel 0 OG 
and which run at the other side parabolically to infinity. 

The right-side branch, whose shape resembles more or less a para- 
bola, touches the curve y’ = 0 in the point #’ =0,7/=0(x=l, y=1). 

Between the two branches, so in the regions 2, 4 and 6: 

(2y — 3x)? —4(4y7' —3x)(2y'— 3x) 4+ 167 <9; 
in all the other regions of course > 0. 

In the former case the tangent AP to the plaitpoint-curve of the 
(v, z)-diagram is directed to the side of the small volumes, in the 
second to that of the large volumes. 

If we, however, examine, whether e.g. at decrease of temperature 
the plaitpoint moves towards the large or towards the small volumes, 
the parabolic border curve acts again as separating curve. 

It appears then that the plaitpoint moves towards the large volumes 
at decrease of temperature in the regions 2, 4, 5 and 7, at increase 


of temperature in the others. 


( 451 ) 


9. The following table gives the characteristics for the diffe- 
rent regions. 
Region 
1 (2y'-3x!)?-8(y'-x') 0; 2y'- 3x0; (2y'-3x')?-4(4y'- 8x')(2y'-3x') + 16y'>0 
2 x Nt: a) 7303 5 <0 
3 zE 0; ” <05 ” >0 
4 3 DRAAK secre O's 7 <0 
5 ie en Re an, oh i 20 


6 7 A a AE rs <0 
7 EE) <0; ” <0; ” >0 
where : 
— b.—b 
et En Gete et) 
a, b, 


A similar tabular survey of the physical properties of the regions 
seems superfluous, as these properties may be immediately read from 
the illustrations of fig. 1 of the unfolding plate. 


10. It seems not devoid of interest to know how the breadths of the 
regions change with regard to each other, when continually increasing 
ralues of y’ are considered. An inquiry into this shows at once that 


the blue region 5, measured along a line parallel to the x-axis, has 
2 
a limiting value for the breadth of —. All the other regions mentioned, 


however, continue to increase indefinitely, and do this proportional 


with Wy’ and in such a way that the yellow and the red region get 
gradually the same breadth and in the same way the green and the 
purple one, but that the breadth of the two first mentioned regions 
will amount to 0,732 of that of the two last mentioned. 

If we also take the white region (reckoned e.g. from the y-axis) 
into consideration then we find its breadth at first approximation to 
be proportional with y', so that it exceeds in the long run the other 
mentioned; the orange region keeps of course an infinite breadth. 

The limiting values of the ratios may therefore be represented 
as follows: 


white yellow _ green blue purple red orange 


eae 007 0 WTS Weg TONE 0) 

We may see that if we keep « constant and make y to increase 
we always reach the white region, while reversively increase of x 
with constant y leads finally to the orange region. Strong attraction 
between the molecules of the admixture and those of the principal 
30% 


( 452 ) 


component promotes therefore in the long run the relations of case 
4, large volume of the molecules of the admixture promotes those 
of case 1. 


11. We may conclude this descriptive part with mentioning some 
formulae which we have obtained in the course of our investigation, 
and which will be derived in the second part. We do not, however, 
give them as new, as they must essentially agree with similar 
equations obtained by Kerrsom’) and VerscHarreLt®), if the simplifying 
hypotheses are introduced on which the original equation of the 
y-surface, used by us, rests. Nor does the way in which they are 
derived, in which the method of the systematic development into 
series is followed, differ considerably from that of VERSCHAFFELT. 

In these formulae we have restricted the number of notations as 
much as possible. They only hold at approximation in the neigh- 
bourhood of point A and of the critical temperature 7), of the 
principal component. 

We shall first give expressions for the radii of curvature Rand 
R'conn. Of the projections on the (r, r)-surface of the spinodal and 
connodal curves in the plaitpoint; from which appears that the radius 
of curvature of the connodal curve in the neighbourhood of the point 
K is at first approximation three times as great as that of the spinodal. 


3 
Rb rie EE 


Hees bt [(2y'—3x')?—8(y'—-x)J=BR'y>. - . OD 

These radii of curvature are here considered as being positive 
when both curves turn their convex sides to the v-axis as in the 
cases 1—4 of fig. 1 and negative in the cases 5—7. 

We may shortly point out here that the corresponding radii of 
curvature on the yw-surface itself, on account of the strong inclination 
of the tangential plane in the neighbourhood of the v-axis, are quite 
different and much smaller, though the relation 1:3, of course 


1) W.H. Keesom. “Contributions to the knowledge of van per Waats’s J-surface. 
V. The dependence of the plaitpoint constants on the composition in binary mixtures 
with small proportions of one of the components”. Proc. Royal Acad. IV. p. 293—307. 
Leiden, Comm. phys. Lab. N°. 75. 

2) J. E. Verscuarrett. “Contributions to the knowledge of van per Waats, 4-surface. 
VII. The equation of state and the #-surface in the immediate neighbourhood of 
the critical state for binary mixtures with a small proportion of one of the com- 
ponents”. Proc. Royal Acad. V, p. 32L—350, Leiden, Comm. Phys. Lab. NO, 81. 


—— ed 


hek Und 


( 453 ) 


continues to exist. They even become zero when the plaitpoint 
coincides with the critical point A, so that both curves have then a cusp. 


12. The knowledge of the radius of curvature Roy, is of importance 
specially because it may be used in connection with the formula: 


Fig. d. 


1 9 ' € ! 
CG Pe = = tb (2y —3x je ps é 
| 


through which we know the small angle which 
the tangent of the plaitpoint forms with the v-axis, 
to calculate in a very simple way the differences 
in density and volume between the phases of the 
plaitpoint Z and the critical point of contact R 
at first approximation '). 

According to fig. d we have, within the indicated 
limit of accuracy : 


(12) 


9D 
7 ker — PO—} = Wa = rae) 2 aa 4 24 hade { de we : v e e 
Vp UR ar OPE = wh conn. 8 ( 7 3x) L( / 3x) 8(y me )] B a) 


1 9 
. ss > 2 | LE OO NS 9 VE A2 (oA 2? é 
# ,—# ,»=RhQ= 5 Fe donne mie 9x) [(2y 3x) —8(y'-x') Ja 5 (14) 


13. We proceed now to give the formulae relating to the plait- 
points phase at a temperature 7, which does not differ much from 
the critical temperature 7% of the principal component. 

They are: 

4 TT 


eeN Rene EEN 
P (Qy'— 8x) B(y'—x’) Ta 


3 j ! € IANS, | € ! ¢ ! € ! a} » 
—3b,= 5 b, { (2y'—3x')?—4(4y'— 3x’) (2y'—3x')+16y'} Ep: (16) 


Pp 
Pp—P, 
(BA Je, + « (11) 
pr : 
By means of (15) we may transform (13) and (14), so that they 
become : 
9b, TE 
b] mm 7) en - 2) gm) 4 = . . Kl © . 18 
ip oT aah 9 ( oe x) yop ( ) 
and 
9 T'—T;, 
tr (2-3) oe . « « (19 
oe ify are 16 ( i 3x ) fp Bt ( ) 


1) A similar method is given by Kerzom at the conclusion of the before-mentioned 
paper of VERSCHAFFELT. 


( 454 ) 


to which we add: 

Pp rl Pen 

Lo ies a 84)" (op) ep = er Bep (20) 
Py 4b, Dj 


14. We shall conclude with giving some formulae relating to 
coexisting phases, where the index one refers to the liquid-, the index 
two to the gas phase. Where the index fails, we may arbitrarily 
take the value for the one or for the other coexisting phase; either 
because it is indifferent at the degree of approximation used, or 
because the: formula will equally hold for either state. 


v,—=3b,—3b LA “Her —3x')?—8(y'—x')Je « (21) 


v,=3b, +3), PA 


P—Pk ae r 


Ar) — ee (22) 


id AA EN EN 
Pk 1 
DS Cr B) (0, =O 20 ck wt NEE 
1 54 ‘ar ce | 7 : 
= rde) —36, = — "enb: b, ——— + 3b, ‘| 5 [2y'—3x')?—8(y'— x) + 


1 Ì 
L = [(2y'—3x')? —24 (y'— x’) (2y'— 3x’) 4+ 16 (8y'—2x')] | Lae (OON 


in which formula (23) holds also for non-coexisting phases. 
SECOND DEMONSTRATING PART. 


Transformation of the Y-sur face and preliminary development 


into series. 


15. We begin with a transformation of the y-surface by intro- 
ducing the following variables: 
v—odb, T— Tr ww 


== AA EE n,n 
ra haat Poy i a eT an 


which means that we henceforth measure the volume v’ from the 
eritical volume and with that volume as unit, the temperature in 
l itl d to the critical Ti we 
the same way with regard to the critica temperature Lenn 

= 27b MR 


and the free energy yw’ with MRT, as unit. 
Ou 


ae 


If we moreover put: 
ils @, ! ey i 1 dd, Pear 
ee ey in eas. (3 
ay b, ‘ ay b ay 
we find easily from (1), (2) and (3) for the equation of the new 
surface: *): 
w! = (LHE!) log 3d, (by! Hv) - 


t 
Ay 


le! 


+ (LHE) tw log w 4- (1e) log (1-a)}, (28) 


where 
TEE 9 9 ! 9 9 ! rl 2 99 
Catal Ma ea de yt ae - 5 . E (29) 
bir cs ate : Zy! =d!) x? 30 
na BEN EAR NEMA CA 
further : 
Ow MRT). ow! 8 dy’ 
ee aida oa oa oe ed (31) 
Ov 3b Ov a Ov 


1 


16. For investigations in the neighbourhood of the sides it is 
desirable to develop the expression for yw’ so far as possible according 
to the powers of w. We write therefore: 


W = (LE) v loge + %, an € vu av av ap iat 7 = (32) 


where in finite form *) 


Xo = — (HL) log b, (243!) — (LF) 


; ie 2y' 9x! 
x= (lt) nk EE Oe OP 
Dy’? ed TN | 9 (2x'—2') 


hae a) = Wige e ael mes (Lo!) 


1) If we wanted to consider az as function of the temperature, the simplest way 
of doing this would be by writing the second term of the second member : 
dell Het Het? +...) | : 8a, 

- Par —. The formula 7; = a7 MR 

x 
hold unmodified for the critical temperature of the principal component, provided 
we take for «dj the value it has at that critical temperature. With Crausius’ hypothesis 
that dr is inversely proportionate to 7, we should get 2, =—1; sal. Also 
(29) continues to hold and the modifications in the developments into series and 
in the formulae derived from them would be easy to apply. 

3) In this form they may be used for investigations concerning the conditions 
at the side of the „-surface at temperatures greatly differing from the critical tem- 
perature of the principal component, as are made by Kresom: Contributions to the 
knowledge of the y-surface of van per Waats. VI. The increase of pressure at 
condensation of a substance with small admixtures. Proc. Royal Acad. IV, p. 659— 


668; Leiden, Comm. phys. Lab. N°. 79, 


9 


(33) 


(35) 


would continue to 


(-456 5) 
or, after development into series with respect to the powers of v’: 
656 be 
e= — (AH) log EE — (as )r ne (vi 5 tort 
DE Ee re EEN MEE Ch NR 
64 160 


Rete 
Am hi A CO naden zer x42 y't fr Eh 
9 9 
Fitr et ree te DD 
1 9 3 | 
Edd ed een arn ma eee eee 


for which last expression we write: 


== Hotter... Ee 


Determination of the plaitpoint and classification of the 


different possible CASES. 


17. For calculating the coordinates pi and ZIjn of the plaitpoint 


we have the following relations: *) 


3 = dy” 
m ete ee ae =v oren lee ee 
ae 07 yp’ 
ss et vt Wc ORNE N = a, 
OTE bene Bs 
93 ,! 33 03 9! 03 U 
on ~ + 3m? Or Ek + 3m- Eos 4- io = Oi, See 


where m represents *) the tangent of the angle formed by the (v’, 2)- 
projection of the common tangent of spinodal and connodal curve in 
the plaitpoint with the 7’-axis. 

If by means of (32), (86) and (387) we introduce in these equations 
everywhere the values of the differential quotients at first approxi- 
mation, in which, as appears, m, Up and Vass may be treated as 
small quantities of the same order, we find: 


ge eR) i nt me 


1) D. J. Korvewec. Ueber Faltenpunkte. Wiener Sitzungsberichte, Bd. 98, 
Abt. IL, (1889), p. 1171. 
2) See l. c. p. 1163. 


3 grt Barink) 
hens IA tn (y—x)e, =0 Prva, A] 
m* 27 27 aon BENN i je 
ET + — 5 Bn ble AN be (45) 
y P — 


from which it is easy to deduce : 


© 


mse A y—3x)e, : (46) 
= t 47 
er A 

1 
= = [(2y—3x!)’—4(4y'— 3x!) (23) + 16y'Je,,. … (48) 


The formulae (12), (15) and (16) of the first descriptive part of this 
paper may be derived from these formulae by means of the reverse 
transformation into the original y-surface with the aid of the formulae 
(26). Applying equation (31) we may also derive formula (17). In 
the course of this we get first at formula (23), which is given at the 
end of the descriptive part as serving also for the calculation for 
coexisting phases. The last statement might be objected to, because 
for those phases not v’ but v’? is a quantity of the same order as 

Oy 


wand t’; but this objection loses its force when we observe that in — 


v 
no term occurs with v’? alone. 


18. From these formulae (46), (47) and (48) follows now imme- 
diately the classification of the plaitpoints according to the eight cases 
and all the particularities of the corresponding graphical representation, 
as described in $ 2—9. It is only necessary to say a few words 
about the construction of the cubic border curve. 


(2 y'—3x')* — Jy!) HTO = Oh), (89) 


A closer examination of this equation shows, namely, that the 
curve possesses a double point, i.e. the point at infinity of the straight 


line 2 y’—dx%’=0. A simple parameter representation is therefore 
possible and it is really obtained by putting 


Af Boe Se oer Te, oa eta Pee 
_from which follows: 
s'—49(s-+-2y) +1670 vn (OD) 
hence: 
oes) SEH EN 


IC ET 


( 458 ) 


The points of the left-side branch are then given by the values 
of s between + co and 2, those of the right-side branch by the 
others. 

For s=2 we get the two infinite branches belonging to the 
asymptote : 

ISU Bie OR Ven goo), ages) a" NR 


19. Nor do we meet with any difficulties in the calculation of 
the breadth-relations of the regions for very large values of y' men- 
tioned in $ 10. 

For the cubic curve we may put: 


Sof 0 yh pial re ee ea 
through which its equation passes into: 
(—FP+ 8h) YVy7'1+16—4h=0 ... . (55) 


from which appears that for very large values of y’ we find 
— 22,0 and +2V 2 for k. We get therefore for the leftside 
branch of the cubic curve approximately : 


2 2 
9 a VY oe ee 
ra ae Vy (56) 
and for that on the right-side: 
2 hare 
C= ei iar oo wee . e . . . . (57) 


while of course the middle branch with asymptote corresponds 
with £=0O. For this branch we have: 


; Ae 2 58 
x = —y'—— . 5 
Ba pier (58) 
In a similar way we find for the parabolic border curve: 
BNE se 
! ! : ! ld 
hr eer A ° e e » e > (59) 
3 9 
Taking this into consideration we may equate the breadth of the 
2 


yellow region at infinity to 5 (3—V3)V2.Vy’, that of the green 


2 2 
one to ae te that of the blue one to a that of the purple 


: 2 
P V6.7’ and that of the red one to 9 BV 3V avy 


one again to 


from whieh the relations of equation (9) easily follow, while 
ia. =O ae, 


( 459 ) 
The spinodal curve. 


20. The equation of the spinodal curve is found by elimination 
of m from (40) and (41). We must, however, take into account, 
when writing these two equations, that v’ along the spinodal curve 
must be considered to be of the order Vz, so that the terms with 
v’? must also be taken into consideration. 

We get then: 


m 3 é 
eae aK ge PA eet Nw tea eget de) a 03 ORD 
Usp. 
and 
a Mn gate ts de ! 0 61 
1 (2y —3x) m 1 iG Usp, 5 Y¥—*) Cop. = oo) AST 


from which follows for the equation of the spinodal curve: 


’2 1 Ns ey Pal ' . 4 ; N 
VEN The [(2y'— 3x)? — 8 (y'—#')] wap. + 5 Ds kers (GA) 

This is, however, its equation on the w’-surface. In order to 
‘know it on the original y-surface, we must transform it with the 
aid of (26) into 
(wap. — 3b,)? — 8,2 [(2y! — 3x')? — 8 (y' — IT wy, + 120,27 = 0. . (63) 

For that of the circle: 

(v—3b,)? + (vld)? = R*, (d small) 
we may write with the same approximation : 
(v—3b,)? — 2Rhe + 2hd —= 0, 

from which we may immediately derive the*expression (10) for the 
radius of curvature of the (v, 2) projection of the spinodal curve. 


The two first connodal relations. Equation of the connodal curve. 


21. We shall „now take -P, (z,,v',) and P,@,,’,), for which 
v', >v',, as denoting two corresponding connodes. 

We put then: 
v=o ns ve Ans e= — Sys Le + Sy; « (64) 
hence : 


1 | 7 : . 
vom = vk) N= (7%); e= 5 rt) Sr ; (65) 


where therefore (x", v") indicates a point halfway between the two 
connodes and § denotes the tangent of the angle which the projection 
on the (+, w)-surface of the join of the connodes forms with the 
p'-axis. 


( 460 ) 


It is then easy to anticipate, and it is confirmed by the calcula- 
tions, that all these quantities 7”, 2" and § with the exception of 1, 
are of the same order with each other and with #; on the contrary 
not 4 but 2’ is of this same order. 


22. Taking this into consideration the first connodal relation : 


Oy’, Oe’, 
ee 


0x, 
yields at first approximation : 


2 


log (2! 489) - 1-3) (v" 4-4) = log (e=) - 4 (273%) (v'-n) . (67) 
or also, subtracting on either side log x": 

log (: zt =) En ss (2y'—38x') 4 = lg ( i =) ees) 
or, as | is a small quantity of the order of 13, we get after deve- 
isomeat into series and division by 7: 
(Er Btn) eee ee ETD 


in which we shortly point out that this formula passes into formula 
(46) in the plaitpoint, and further that it leads immediately to for- 
mula (24) of the descriptive part. 

In the same way the second *) connodal relation: 


ET rn EEE ef CA 


yields at approximation: 


ate Ig ae q Bins 8 
en vand Pe, OERS RAE 
es Vn aren ern 


8 
9 3 3 9 9 
hg AP Ennn tn 
3 q 
Rt (2y'— 3x’) Si ate (ye) JE ee, eN 


or, after reduction and division by %: 


1) We must here have recourse to the terms of the order ¢'? or n°, as all those of 
lower order cancel each other. For the sake of clearness we have kept (v" + 1) 
and also (v" — 7) together, though it is evident, that we may write e.g. for (v" + 9)? 


at once #3 on account of the difference in order of v” and 7. 


9 ! 9 3 5 5 PR Ehh pe a ' ' " q r 
aen -}- ry 1 — 9 (2y'— 3x’) Ss En 9g (y —%) Lv ==); - a (72) 


from which follows in connection with (69): 


n° — [(2y'—3x')? — 8 (y'—z’')Ja" +4! =0. . . . (78) 


23. This formula yields at onee the radius of curvature of the 
(v, w)-projection of the connodal curve. We need only observe that 
according to definition : 

ON ete Meghna Me Sa GMS ha dk en Be GED 
so at first approximation : 


etek ee = edt us Rix dias Modern Gare. eu see eels 
3b 

Substitution of these last relations in (73) now yields immediately the 
equation of the connodal curve and in exactly the same way as for 
the spinodal curve we find from it the value of the radius of cur- 
vature Reon given in formula (11). A further explanation of the way 
in which the knowledge of this value leads to the formulae (13) and 
and (14) need not be given here, nor need we explain the derivation 
of the formulae (18) and (19), (21) and (22). 

But the derivation of formula (20) will detain us for a moment; 
we require, namely, for it a more accurate expression for p than 
that given in formula (23). If we therefore develop (31) as far as 
needful for the purpose, we find *): 


1 


8 3 3 ! 9 | | 3 ! ! 9 ! 1 ! — 
Pil zitt reet ve J, (16) 
OF: 

PP, ! ! | € ! € ! C ! ! ' 

dt — 6td' 4+ 2 (2y'— 38x) « — 12 (y— x) ve, . (77) 

Py, 
thence: 
LRE las 4e} Dele lr —r y= 22 lose) (ast = ay! Jar 78 
Pk a oe vp) ta x) (we, ay? “(Y x) ( P Cr © ol 8) 


for, with regard to the last term, the difference of wp, and Tp is 


AM . » € T Né € 5! 
slight compared to that between 2’, and v'p. 


9 
1) It might appear as if jg v® ought also to be inserted in the following ex- 


pression, but it is easy to see that this term leads to a small quantity of higher 
order than those that will occur in the final result. 


( 462 ) 
It is now easy to find: 


1 3 
Ce fa at (oa U) 7 (2y7'—3x'/) x, (v ao a) ) SEN 


either by paying attention to the fact that we eee in Fig. d, § 12 
(see the first descriptive part), if applied to the (v’, x)-diagram, with a 
sufficient degree of approximation : 


pee 


1 
RQ = PQ.) RPQ= PQ. w=. PQ.tgu == —.PQ.m 


2 
or by application of the formulae (13) and (14), observing that 


v,— Vp= 3b, eae 


P rp): 


This yields by substitution in (78): 


Par Pr . ol 3 sf 9.,!'\3 
EE — 6 + (Be le, Je) (80) 


Pan 

or finally substituting for ¢’ its value from (47): 

Pp: ÔR 3 EE) 3 2 ! VNS I as! 2 4,!\2 81 
p Pld 7s «a Opt BARS Nee Pen 
k 


from which we immediately derive formula (20), applying (18). 


The third connodal relation. 

24. We have now obtained the principal formulae. For the sake 
of completeness, however, we shall treat here also the third connodal 
relation, the more so as this leads to a new determination of the 
formulae (47) and (48), which puts the former to the test. 

This third relation reads: 


Ole, Oe dees oy’, OW, 
Wie igi Gel En oe 
Oxi Lh, ne 
We first transform w'—a« — —v'— , with the aid of (32). It proves 


Our Ov’ 
to be necessary to keep all terms up to the order # or 1°. So we 
find : 

dy’ ò 0 05 
Boat ot ltd (he! Jor. (88) 
Ow Ov’ Ov’ Ov 
From this follows: 


an v; Wie (1-+-#')(a"+-§y)-(1 + ¢)log 20, Se, + 20") + 


9g 63 3 
res 13 Si mA wv poe [(2y'—3x') + 2y't \(4+e") (+n) Ed's 


5 GOH 20") "HE BY- 2a'-0,(4*H2a"E)-20,101"(84) 


sl No) 


aid 


( 463°) 


If we equate this to the corresponding expression for 


Ow, òw, 


U 
1 at -—=— 1 = 
5 ; Ou, ' ov’ 1 : 


which is obtained by changing 4 into — 4, we get, dividing by 7: 
N08 B.A a Ne i 
SIPS Ade ape rites 1 +50 | T5 (2y —d3x) a Syt -|- 


FOT BEI — x) E qt — 18 (y — x) 0a" + 
27 
eu oe A Pe LO 0 Ne tt (85) 
At first approximation this yields: 
En aL (2y'— 8x’) a". 
4 


This relation is, however, identical with the relation (69) which is 
derived from the first connodal relation. So we cannot draw any 
further conclusion from equation (85) without bringing it into con- 
nection with the first connodal relation; but for this it is required 
to introduce a further approximation for the latter. 


Second approaimation of the first connodal relation. 
25. From the first connodal relation in connection with the equation 


Oy 
BS 1E H(LHE) log e+-y,+2y,24-.... . . . (86) 
the following relation may easily be derived, if we take into account 


the terms up to the order ¢? or 7°: 


Sn 
al" 9 
(1+ #') log ir (2y' 3x) Sy nt + Uy xe" — i (By —2x) n° 4 
5 | 
ms 
Hij 
oe LS A RC ER nun, nate Whey iS 
Within the same order of approximation we have however: 
Sn 
IED een 
Ig a" 25m 28m 
0g & a" ar Z's 


In the second term of the second member of this equation, however, 
we may safely make use of the first approximation furnished by 
equation (69). Taking this into account (87) passes after multiplication 
with 2" and division by % into: 


( 464 ) 
5) 
= (27 —3!) nj" — > (27'—82')a"—3 y' at! + 9(y'— —x')v" a" — 


9 
rae (By Zult aL 46.6a" + Agia = Oi ae ee. 


Further reduction of the third connodal relation. 
Derivation of equation (25) of the first descriptive part. 


26. By addition of (85) and (88) we find: *) 
9 roy 9 27 9 

Ev = Een 4___ Q(+! — x’) En —9(y'— Ig! 
ee er boo (y'— #') Sy? —9(y'—x!)vtact + 


3 9 
+ 5 Cr’ —Bulyo'S + 5 (27/3) $16 Gele" = 0... (89) 


When we add to this relation (72), which is deduced ae the 
second connodal relation, after having multiplied it with v7”, we can 
divide by 1? and we get: 


9 9 63 peel | A Wad 9 ! ' > ' ' " 
5 en a yp! + 50 My) + = [(2y'-3z')? + 16(8y'-2z')Ja"=0 . (90) 


. 


Making use of (69) we may solve the quantity 7" from this equation : 
! 7 1 ' ! ! > 3) ! iy " 
y' = 2t +— 7 + 3 - [(2y'-3x')*?-24(2y'-3x') (y'-x') + 16 (By'-2x')J2", (91, 
0 
or finally with the aid of (73): 


18 7 kon 
te Bit Ier — B) — 8 (7) + 


1 3 3 ! ERN ! ! ? Spe € | " 
te a [(2y' — 3x)! — 24 (2y' — 3x’) (y' — x’) + 16 (By — 2a) - (82) 


from which equation (25) follows immediately with the aid of (65) 
and (26). 


In this way we have found the starting-point of the curve in the 
(v, .v)-diagram described by the point halfway between the points 
which represent coexisting phases. The tangent in that starting point 
also is now known. 


1) Remarkable is the disappearance of the terms derived from 7 x?, which makes 


(lo 


D> 
alsbek and dere: ae and b. disappear from the result. We have tested the truth 
1 1 


of this in different ways. 


( 465 ) 


A new determination of the plaitpoint, independent 


of the preceding one. 


27. It is now easy to obtain such a determination with the aid 
of (73) and (91). For in the plaitpoint we have: 
" 


î " 
Wee OE BSS) fy. 8! == oat 


From (73) follows immediately (47); from (91): 
Tyg 
v'p = 2t' + 5 [(2y'— 8x')? —24 (2y’— 3x’) (y’—x') +16 (By'—2x')|wp; « (93) 


from which in connection with (47) we find again (48). 


Physics. — “Some remarkable phenomena, concerning the electric 
. curcuit. in electrolytes’. By Mr. A. H. Sirks. (Communicated 
by Prof. H. A. Lorentz). 


On etching of metal-alloys by means of the electric current, as 
communicated in the proceedings of the meeting of September 27, 
1902, I met with a great difficulty. In some cases the hydrogen 
developed at the kathode was very troublesome, namely when, instead 
of escaping immediately it divided itself in small bubbles through the 
liquid and stuck to the object to be etched used as anode. This 
obstacle was overcome by surrounding the kathode with fine brass-gauze, 
so that the gasbubbles were compelled to escape directly in this case. 
The gauze was hung up apart, consequently there was no contact, 
Whatever, with one of the electrodes. The etching being finished, 
copper proved to have been precipitated on the wires of the gauze, 
which deposit was almost conform to the shape of the electrodes. 

This was still more visible at a second etching-experiment with the 
same copper-alloy: a small cup was placed under the anode, which 
partly hung in it. Again on the gauze a copper-deposit was perceptible, 
which showed at the lower side a distinctly designed horizontal 
margin, nearly as high as the brim of the cup. 

It was to be expected, that copper should precipitate on the gauze, 
placed between the electrodes, as the whole apparatus can be con- 
sidered as two voltameters, connected in series‘). But, why is by this 
electrolysis not the whole side of the gauze, facing the anode, cop- 
pered, as is the case with the kathode by any ordinary electrolysis ? 

To answer this question the experiments were altered somewhat. 


1) The anode and the side of the gauze facing it, are the electrodes of one, 
the other side of it and the kathode, those of the other voltameter. 
31 


Proceedings Royal Acad. Amsterdam, Vol. V. 


( 466) 


Instead of water acidulated with sulphuric-acid a saturated solution 
of copper-sulphate was used as electrolyte; the electrodes were 
formed in future by two equally large Dutch bronze coins. The back 
part of these coins and the battery-wires, to which they were sol- 
dered, were varnished, as far as they were immersed in the electro- 
lyte, in order to be sure, that, during the electrolysis, the facing- 
sides only served as pole-plates. The gauze tube was left away and 
a screen of platinum (44¢.m.), hung up isolated, placed just 
amidst the electrodes, who were 4 ec. m. from each other. If a copper- 
deposit might appear on the platinum, this could be ascribed to 
eleetrolytie actions only. Very soon after the circuit was closed 
(intensity + 0,3 amp; voltage of the battery = 4 volts) there came on 
the piece of platinum facing the anode a sharply bounded copper- 
deposit, which, by continuation of the experiment, changed of thick- 
ness exclusively and not of size. The experiment was continued for 
2 days; still the results remained the same. 

Now I resolved to remove the platinum screen between the electrodes, 
to do the experiment over again and repeat this several times. The 
deposits obtained in all these cases were not exactly of the same 
size. The smallest deposit (diam. 18 mM) was obtained by hanging 
the sereen between the electrodes (diam. 19 mM.), from which we 
can conclude to a small gradual contraction to the middle. 

If two electrodes of different shape were used, then, by removing 
the platinum screen from the anode to the kathode, the copper- 
deposit passed from the shape of one electrode into that of the other. 
This was very clearly visible by using a nut as anode and a square 
piece of sheet-copper as kathode. The hexagonal copperdeposit gra- 
dually took a square shape. 

Superticially one would be inclined to suppose, that the only 
thing, that has happened is the locally making of sections of the 
envelope of the two electrodes by means of the sereen, but consider- 
ing, that, if electricity passes from one electrode to the other, the 


stream-lines divide through the whole fluid — the current-density is 
only larger within the above-mentioned envelope — it will be ob- 


vious, that there must have been another cause, which made 
some stream-lines prefer to take the way round the screen to the 
shorter one through it. Considering, that the resistance of the platinum 
can be neglected in regard to that of the longer way through the fluid, 
the explanation of the deviation of these stream-lines can only be 
found in the polarisation, caused by the screen of platinum. 

To prove the supposal, that stream-lines are going out from the elec- 
trodes in all directions, the following experiment may serve: The 


( 467) 


anode was hung in a platinum cup, which must replace the platinum 
diaphragm and was therefore partly filled with the electrolyte. 
Directly the circuit was closed, the inside of the cup was evenly 
coppered, as high as the surface of the liquid, while at the outside 
an intense gas-development took place, which was soon impossible 
to be observed well, as on account of the polarisation the current- 
intensity was considerably decreasing. In some cases from 0,9 amp. 
to 0,02 amp. If on the reverse the kathode was hung in the 
cup, the development of gas took place at the whole inside. Half 
of the outside of the cup facing the anode was partly and unevenly 
covered with a copper-deposit. 

When making the experiment with a sheet of platinum (5 > 5 em), 
dividing the glass in two equal parts, the results were just the 
same. Here also the platinum was entirely covered with precipitated 
copper. At a distance of the electrodes of about 10 m.m., the copper- 
deposit was pretty evenly spread over the platinum. At a smaller 
distance of the electrodes (4 m.m.) there came between the electrodes 
on the platinum a distinct circular deposit, while the copper precipit- 
ated on the remainder of the screen was very faint. A same deposit 
perfectly corresponds with the sections of the stream-lines we should 
expect. 

The same results were obtained, when using two diaphragms 
dividing the cup into three parts. At the first experiment two dia- 
phragms were used, completely shutting off the fluid and connected 
with a copper-wire. The side of the first diaphragm, facing the anode, 
counting from the anode to the kathode, was entirely coppered; the 
side of the other one, facing the kathode, was covered with gas-bubbles. 

At a second experiment only the connecting wire was taken 
away. The sides of both diaphragms, facing the positive electrode, 
were entirely covered with a copper-deposit. On the other sides gas 
was developing. . 

At a third experiment two platinum screens (4 4 em.) were 
used, thus not shutting off the fluid completely, but connected, 
however, with a copper-wire. The same circular copper-deposit 
came on the first screen, facing the anode, but, when. breaking the 
connection the same side of the second screen was, on the contrary, 
entirely covered with copper. 

The latter phenomenon can be explained in this manner: The 
copper-ions, leaving the anode, yielded their charge to the first screen, 
over which it is entirely distributed and which, over the whole side, 
facing the kathode, serves in its turn as anode towards the second 
screen, which is coppered over the whole surface. If the second 

31* 


( 468 ) 


screen was larger than the first, then, the side of the former, facing 
the anode, was coppered for a part about as large as the latter. 

Then, the experiment was repeated with a screen, dividing the 
basin into two equal parts, but having a small hole in the middle. 
Just as a part of the stream-lines in some of the former experiments 
went round the screen, so here a very great contraction of the stream- 
lines towards the hole may be expected. Some of them will deviate 
from their straight way preferring the way through the hole, to 
the way through the screen. This is confirmed by a circular part of 
the screen remaining uncovered. 

The following data are the results of a series of experiments, taken 
with holes of different size. 


Diameter of the hole. Diameter of the uncovered part. 
1 mm. 7 mm. 
4 14 / 
5 I dr " 
Ay 25 
15 whole screen uncovered. 


distance between electrodes 3 em., diameter of electrodes 19 mm. 


If the smaller sereen is taken, so that stream-lines can also go 
round it as well, then the uncovered part is considerably smaller. 
The diameter of it was 3 mm. at a 1 mm. diameter of the hole. 

It is worth notice, that, while the electro-motive force remained 
the same, the current-intensity increased on increasing the diameter 
of the aperture. If for instance at the experiment with the smallest 
hole (diam. 1 mm.) the intensity after the beginning of the polari- 
sation was 0,1 amp., it amounts under the same circumstances to 
0,3 amp., when using the screen with the biggest hole. 

It is curious, that at the first experiment a copper-deposit was 
seen on the case of brass gauze surrounding the kathode, though 
properly it is nothing but a sereen with a great number of small 
holes. According to what is said before, it might have been expected, 
that all the stream-lines would pass from tise anode through the holes 
of the case to the kathode and therefore not form any deposit on 
the gauze. In connection with this, some more experiments were 
taken with different sorts of brass gauze, but already by using the 
next size — stitches of 2 mm? and 0,3 mm. wires — no traces 
of copper were precipitated. 

If the way through the fluid was made considerably longer, 
then, in some cases, the current still seemed to prefer this round- 


,- 
a 
p. 


A elk 


( 469 ) 


about way to the undoubtedly shorter one through the sereen. 
This was done in the following way: Again the anode was hung 
in a platinum cup, over the brim of which hung a bent glass-tube, 
filled with the copper-sulphate solution, thus forming the connection 
between the electrolyte at the inner- and outer side of the cup. 
Even if a capillary tube was used, a deviation was observed in the 
copper-deposit, namely: a part of the cup near the lower end of 
the tube was not coppered, this, however, only when the tube was 
hung over that place on the brim of the cup between the electrodes. 
A 3 mm. tube, however, caused a deviation of the deposit, even, if 
the tube was hung over the brim of the cup on the prolongation 
of the centre-line of the electrodes. 

Of course, there must be some relation between the coppering of 
the inner surface of the cup in these cases and the circular deposit 
on the screen. It must be possible, therefore, to pass gradually from 
one deposit into the other. Instead of the cup a cylinder of platinum, 
having a diameter of 4 cm., was used, which at the bottom was 
melted in a basin with paraffine and projected from the fluid. The 
anode was hung in it again. The circuit being closed, the inside of 
the cylinder was of course coppered again as far as it was immersed 
in the electrolyte (50 mm.). Then a vertical cleft of 1 mm. wide 
and 1 mm. high was made in the cylinder on the extension-line of 
the centres of electrodes. A part of the inner wall round the cleft 
remained again uncovered. When gradually giving the cleft a height 
of 20 mm., the uncovered part took the form of an ellipse, till ata 
height of 25 mm. a strip of 8 mm. wideness was not covered with 
copper, along the whole height, i.e. 50 mm., of the electrolyte. 
When still enlarging the cleft, the deposit gradually receded more 
from the margins and after unfolding the cylinder into a plane it 
finally took the already known circular form again. 

To make the explanation, given of the deviation of the stream-lines 
on account of the polarisation of the platinum, more acceptible, the 
experiments were made with different electromotive forces by inserting 
resistance. By means of a resistance box, connected parallel with 
the voltameter, the terminal voltage of the latter could be increased. 
The current-intensity could be read on a milli-amperemeter, joined 
in circuit with the voltameter. As long as the potential difference 
was less than the electro-motive force of the polarisation, nothing 
was precipitated. After more resistance had been inserted in the 
resistance box, a current began to pass through the voltameter, but 
without forming a deposit on the sheet of platinum, although the 
experiment was carried on some hours. For that reason this current 


( 470 ) 


could not have chosen its way through the sereen and must have 
gone therefore round it. If some more resistance was inserted, then 
a deposit came gradually on the screen, smaller and more uneven 
than in the ordinary ease, but also taking the normal size and 
thickness as formerly, when going on inserting more resistance. 


Different salts were used as electrolyte, in none however, a deposit 
was so easily formed as in cupricsulphate. The phenomenon, when 
using this salt, was so clear, that once a deviation in the shape of 
the deposit was observed, because the wire which was connected to 
the anode, was not sufficiently insulated. In saturated solutions of 
zine-, aluminium-, nickel-, cobalt-, ferrous- and ferricsulphate deposits 
were formed, one clearer than the other even if in all these cases 
the constant current-intensity was secured by inserting resistance. 

Chlorides were also used as electrolytes. In chlorides of zine and 
cadmium exactly the same circular deposit was formed, but in those 
metals, which can form more than one chloride (e.g. iron), a secondary 
phenomenon always appeared. When a solution of cupric-chloride 
was electrolysed, copper precipitated on the kathode; when, however, 
a platinum screen was put between the electrodes, again a circular 
deposit of a white substance was formed on the screen, quickly getting 
green in the air and being hygroscopic then; probably it might have been 
cuprous chloride, afterwards becoming cupric chloride again. When using 
a solution of Hg Cl, as electrolyte a white deposit of Hg Cl came on 
the platinum. A solution of Au Cl, gave conformable results; a brown 
red deposit was formed. Using H, Pt Cl, and a sereen of gold-leaf, 
a yellow brown one was formed on the latter. When a solution of 
ferric chloride was used no deposit was ever formed. The explanation 
may be found perhaps in the solubility of ferrous chloride which 
is precipitated on the platinum as copper before. 


Though in many of the former cases an explanation could be found 
in the polarisation, yet, however, there is one thing, that cannot be 
explained, i. e. the curious sharp margins of the deposit. It seems 
as if the stream-lines keep their original direction within a certain 
tubular surface also in the presence of the platinum screen, while this 
screen has a strong influence on the lines outside of it, which change 
their direction and go round the screen. Perhaps the explanation 
may be found by calculating the course of the circuit, but I am 
not able to do it. 


In the making of all these experiments I have become indebted 


ATL} 


to professor ARONSTEIN and professor SCHROEDER VAN DER Kork for 
their assistance of various kinds and to these I tender my best thanks. 
Also to Professor H. A. Lorentz, professor at the Leyden University, 
for his help and information. 
Mineralogical Laboratory. 
Polyt. School. Delft, Jan. 1903. 


(February 25, 1903). 


KONINKLIJKE AKADEMIE VAN WETENSCHAPPEN 
TE AMSTERDAM, 


PROCEEDINGS OF THE MEETING 


of Saturday February 28, 1903. 


(Translated from: Verslag van de gewone vergadering der Wis- en Natuurkundige: 


Afdeeling van Zaterdag 28 Februari 1903, DL XI). 


CONTENTS. 


J.P. Kuexen: “Critical. phenomena of partially miscible liquids—ethane and methylalevhol’” 
(Communicated by Prof. H. KAMERLINGH Onnes), p. 473. 

A. P. N. Fraxcuimonr: “On the so-called compounds of salts of sulphonearboxylic acids with 
sulphuric esters”, p. 482. 

JAN pe Vries: “On the spheres of Moree belonging to ordinary and tangential peneils or 
quadratic surfaces”, p. 484. 

J.D. var per Waars Jr.: “The variability with the density of the quantity bof the equation 
of state”. (Communicated by Prof. J. D. van per Waars), p. 487. 

J. W. Morr presents the dissertation of Dr. J. C. Scnoure: “Die Stelär-Theorie”, p. 497. 

H. Kamer tiscu Onnes: “Methods and apparatus used in the cryogenic laboratory. ILI. Bath 
of very uniform and constant low temperatures in the cryostat”, p. 502, (with 6 plates). 


The following papers were read: 


Physics. — “(Hitical phenomena of partially miscible liquids — ethane 
and methylalcohol.” By JP. KvexeN. (Communicated by 
Prof. H. KAMERLINGH ONNES). 


(Communicated in the Meeting of September 27, 1902). 


Some years ago Mr. W. G. Rosson and 1 began a systematic 
investigation of the phenomena of condensation for mixtures of liquids 
Which do not mix in all proportions '). Shortly afterwards Prof. vax 
peR WaAALs communicated to this Society an important paper in which 
he discussed our results?) and again in the second volume of his 


4 


treatise on the Continuity *) he devotes some pages to the conside- 
1) Zeitschrift für Physik. Chemie 28, p. 342-565, Phil. Mag. (5) 48, p. 180—203e 
2) Kon. Ak. van Wet. Amsterdam 25th March 1899. 

3) Die Gontinuität etc. If 1900. p. 184—192. 


ho 


Proceedings Royal Acad, Amsterdam. Vol. V 


(474) 


ration of the same phenomena. After the publication of Prof. van 
DER WAALS’s paper I approached him privately with some objections 
to his views to which he replied in the most courteous manner. 
Though not completely satisfied it seemed unnecessary at the time 
to publish my views until T should be in a position to add to our 
knowledge of the phenomena by further experunents. 

| have recently resumed the investigation and the results obtained, 
though naturally far from complete, seem of sufficient importance to 
deserve an immediate publication and to be discussed in connection 
with previous experiments. 

For various reasons we had fixed our choice on mixtures of lydro- 
carbons — first of all ethane — and alcohols. Briefly our results 
were as follows: 


(Te, 


a 
é. 


For mixtures of ethane with ethyl-, propyl-, isopropyl- and butyl 
alcohol there are two temperatures 4A and 5 (Fig. -1) between which 
three phases — two liquids and vapour — are possible and the 
critical (i.e. plaitpoint) curve accordingly consists of two branches, 
CA and C,B, C, and C, representing the critical points of ethane 
and alcohol respectively and A/ the three-phase curve. For ethyl- 
alcohol A and B are comparatively far apart: for the higher terms 
of the series these points gradually approach each other and with 
amyvlaleohol no separation into two liquids could be observed; in 
this case the critical curve was a continuous curve joining the two 
eritieal points CL and (, in the usual manner. 

For mixtures of methylalcohol and ethane we found a branch C\A 


(475 ) 


and a three-phase curve ending at 1, as with the higher alcohols, 
but not a limit 2 below which the liquids mix in all proportions. 
The character of the other branch of the critical curve which 
begins at C), the critical point of methvlaleohol, therefore remained 
uncertain. 

Prof. van per Waats’s remarks concerned firstly the explanation 
of the behaviour of the first group of mixtures and secondly of the 
different behaviour of methylalcohol and the prediction of the phe- 
nomena outside the limits of our researches. ‘The experiments com- 
municated in this paper have reference to the latter problem. 

First of all Prof. van per Waats shows how the two branches 
CA and C,B may be made into one continuous curve by producing 
them in the region of the metastable and unstable conditions, a region 
which I shall call the “theoretical” region. In our paper we had 
pointed out that the phenomena were completely explained by the 
formation of a new subsidiary plait with plaitpoint emerging out of 
the main plait on the y-surface and the subsequent withdrawal and 
disappearance of the main plaitpoint ). Having regard to VAN DER 
Waars’s original investigation and to Korrmwna’s treatise *) on the 
properties of the y-surface, the simplest interpretation appears to be 
to assume that at some temperature higher than 7, a closed plait 
begins to develop on the spinodal curve, increasing in extent as the 
temperature falls, until one of its plaitpoints — that of the first kind *) — 
at A pierces the connodal curve of the main plait, thus giving rise 
to the formation of the subsidiary plait and the three-phase triangle. 
On further fall of temperature the inner plaitpoint exchanges partners, 
so as to form a closed plait with that branch of the main plait: on 
which the original plaitpoint lies: at B the connodal curve of the 
main plait begins to enclose this closed plait. We may moreover 
assume the latter to contract on further cooling and ultimately shrink 
to nothing‘). Transferring the above changes to the p-f-diagram 
we obtain the figure deduced from ours by Prof. van pir Waars. 


1) |. c. p. 358—359. 

2) Arch. Néerl. 24 p. 295—368 in particular p. 316 etc. 

5) Comp. KoRTEWEG p. 67. 

‘) Whether this actually takes place seems at least doubtful. The formation 
of the plait on cooling is hardly open to doubt, seeing that at high temperatures 
the Q-surface cannot show any abnormalities in the region under consideration ; 
but this condition does not hold at low temperatures and the contraction of a 
closed plait. on cooling is in contradiction with the rule enunciated by Prof. van 
pen Waars regarding the influence of temperature on the extension of plaits. 


32% 


( 476 ) 


The possibility of producing the theoretical curves in the p-/-diagram 
had escaped our notice *). 

In the first place Prof. var ber Waars observes that the completed 
figure is in contradiction with the law previously deduced by him?) 
that a mixture of non associating substances may have a maximum 
or minimum critical temperature, but not both. To this point one 
of my objections refers. The law depends entirely on the simple 
characteristic equation, but apart from that it only refers to the 
critical point of the homogeneous mixtures and it must be looked 


upon as a possibility that the curve of the critical points — the 
plaitpoints ——- should have both a maximum and a minimum. 


Prof. var per Waars replies to this*) that near a maximum or 
minimum the two curves in question are so close to each other that 
no such difference between them can be admitted. This argument 
does not satisfy me. The two curves touch each other at points where 
a maximum or minimum rupourpressure exists and the two phases 
have the same composition, but points of that kind do not exist in 
the case under consideration. [t is true that a maximum or minimum 
occurs on the plait when the connodal curve intersects the spinodal 
curve, but the character of these points is entirely different from 
that of the points referred to. The three-phase pressure for mixtures 
of ethane and the alcohol is between the vapourpressures of the 
components and there is thus no occasion for assuming the existence 
of another maximum or minimum. That being the case, there is 
no reason for a close resemblance between the two curves nor any 


1) Note added to translation. 

The above was wrilten by me in the conviction which I then held that Prof, 
VAN DER WAALS’s views of the formation of the new plait — although arrived 
at in a different way — still agreed essentially with my own: indeed I do not 
even now see, how else the phenomena could be interpreted. From the paper 
contributed by him in the October-meeting of this society (critical phenomena of 
partially miscible liquids. Kon. Ak. van Wet. Amst. 25th Oct. 1902) it appears 
that such was not the case and that I ought to have been more careful in accept- 
ing the theoretical curve drawn by him as corresponding to the changes on the 
p-surface as understood by myself. Doubt never arose in my mind on this point 
at all and I never considered the question. Still I ought to have noticed that the 
theoretical curve has no vertical tangent at its extreme points, but ends in cusps, 
corresponding to the circumstance that the curvature of the connodal curve is the 
same in both plaitpoints of the closed plait. This is the only respect in which I 
think my paper requires emendation although some of my arguments would have 
been presented in a different manner had I realised how completely lis views 
differed from mine, 

2) Arch. Néerl. 24 p. 23. 

5) Continuität IT p. 188 1. 17. 


ate eld 


( 477 ) 


ground why the “homogeneous” eritical eurve should have a loop 
as well as the plaitpointcurve. 

I am strengthened in this opinion by the fact, that even in the 
“symmetrical” case Prof. Korruwee has come across similar peculiarities 
in the plait and it follows, that theoretically even those mixtures 
Which obey VAN DER Waars’s equation may have a critical curve 
with a loop in it. 

| do mot mean to maintain that the homogeneous eurve in our 
case does not possess a loop or to deny the probability of Prof. 
VAN DER Waatrs’s hypothesis according to which the association of 
the aleohols plays a part in producing the abnormality. What 1 
want to point out is that it has not been proved that with normal 
mixtures the abnormality cannot oceur, although it is very probable 
that this abnormality and in general the formation of two liquid layers 
— While theoretically possible for normal mixtures with special values 
of the constants — in reality occurs with associating substances only *). 

The critical curve in the p,é-diagram having been completed in the 
way deseribed one feels inclined to say with Prof. vax per Waars 
that the case is one of a modified eross-plait and not of a true liquid- 
plait. According to VAN DER Ler’s experiments *) the liquid-plait for 
mixtures of phenol and water has its plaitpoints turned in the direction 
of the positive volume-axis and above a certain temperature is entirely 
independent of the cross-plait. Prof. van per Waars seems inclined 
to look upon those properties as characteristic of the liquid-plait and 
to withhold this name from that part of the plait which in our case 
is turned towards the w-axis. It will appear presently that this view 
cannot very well be sustained so that at any rate this ground for drawing 
the distinction in question disappears. Still the peculiarity remains *) that 
the critical eurve is a continuous curve, at least when no account is 
taken of the objection urged above against joining the curves beyond 
B. Even then however it will be observed that on the y-surface two 
independent plaits exist completely or partly inside each other and 
thus when the y-surface itself is considered the contrast between 
our case and one in which a true liquid plait would exist disappears. 


Moreover the abnormality is ascribed to the same cause — association — 
as the formation of the liquid plait; if both are due to the same 
cause, one feels even less inclined to maintain a distinction in the 
nomenclature. 


1) Continuiliit IL p. 176. 1 doubt the possibility of deducing a relation between 
djs on the one side and @, and dy, on the other. 

2) Zeitschr. Physik. Chemie, 33, p. 622, 630. 

5) Continuität IL p. 188. 


( 478 ) 


The following may be added in further explanation: there is a 
well defined contrast between the two plaits as regards the causes 
of their existence. The cross-plait depends for its existence on the 
shape of the y-curves for the separate homogeneous mixtures, the 
liquid-plait on the other hand is due to the manner in which these 
curves change with the composition. In the formation of the latter 
plait association seems to be the principal factor. But notwithstanding 
this distinct contrast there must be a number of cases in which it 
will be impossible to say which kind of plait one is dealing with 
and to which sort of plait a given plaitpoint belongs. We shall 
presently come across a striking instance of this kind where a 
cross-plait with its plaitpoint gradually changes into a plait: with its 
plaitpoint turned towards the w-axis from which it is impossible to 
withhold the name liquid-plate. 

Let us now consider the case of methylalcohol and ethane. 
Before communicating the new results T will discuss Prof. vax DER 
Waars’s views of these mixtures. He assumes that the critical curve 
is again a continuous one but with a loop turned upwards this time 
instead of downwards as with the higher terms.) There are some 
serious objections to this theory. 

The critical curve, starting at the critical point of ethane (5, 
disappears from the practical part of the surface at a1, as in the 
former case, and the part bevond can therefore only represent a 
theoretical plaitpoint whieh remains hidden, because at higher tem- 
peratures no three phases coexist. Beyond 1 the curve should there- 
fore be dotted throughout, and it cannot be interpreted as in part 
real. In this case as in the other the shape of the curve was 
deduced by keeping in view the homogeneous critical point and a 
striking instance is afforded of how this curve does not give us 
any clue as to the shape of the real critical curve. 

In the second place I think the bending upwards of the critical 
curve assumed in this ease is open to doubt. At somewhat high 
temperatures there is probably no abnormality on the surface and 
no plait except the cross-plait: as the temperature falls a closed 
curve develops one of whose plaitpoints pierces the main plait at 
A and moves from there towards €,. As in the other mixtures the 
three-phase pressure is lower than the vapour pressure of ethane ; 
it follows that the subsidiary plaitpoint is turned towards the .r-axis 
and represents a maximum pressure on the closed plait. This being 
so the simplest) supposition to make is that the other plaitpoint of 


1) Comp. his diagram Kon. Ak, v. Wetensch. Amst. March 25th. 1899 p. 5, 


( 479 ) 


this closed plait is one of minimum pressure: starting from this 
point the pressure on this plait passes through a maximum and a 
minimum successively and reaches its highest value in the real plait- 
point. In other words the theoretical part of the bent critical curve 
in the p,f-diagram should lie below the practical part, as with the 
other alcohols. This supposition seems so much simpler than the 
opposite one that I feel prompted to state the following rule: shen 
the three-phase pressure is between the vapour pressures of the com- 
ponents the theoretical eritical curve bends downwards, when it is 
higher than the vapour pressures of the components (as with ether 
and water’) ) the curve bends upwards. 

In his book on the “Continuity” *) the author discusses the pro- 
bable behaviour of the mixtures at higher temperatures. Apart from 
a possible plaitpoint on the side of the small volumes on the liquid- 
plait, there is no practical plaitpoint left above A. Prof. vax DER 
Waars assumes that this condition will continue up to the critical 
point of methylaleohol, that the plait will close itself here, gradually 
contract and ultimately disappear either at the limiting liquid-volume 
or by its plaitpoint meeting with a possible liquid plaitpoint. 

This expectation has not been realised by my experiments and 
must in itself be looked upon as improbable. The formation of the 
liquid-plait is aseribed to the association of methylaleohol. Above a 
certain temperature this abnormality has disappeared and in any case 
at the critical point it is for most substances very small. Considering 
the great difference between the critical temperatures of the two 
constituents of the mixture an admixture of ethane to methylalcohoi 
cannot but lower the critical point, even if the mutual attraction 
of the components were comparatively great. As a matter of fact 
methylaleohol seems to have some association left at the critical 
point *). Bat this association has the effect of making the mutual 
attraction appear even smaller and thus increases the probability of 
a lowering of the critical temperature by the addition of ethane. It 
follows that the cross-plait has to appear on the y-surface in the 
usual manner with fall of temperature, with its plaitpoint turned 
towards the ethane side. 

In view of the fact that at low temperatures there is a liquid- 

1) Kuenen and Rosson |. c. p. 351. 

2) Continuität Il, p. 189 verv. 

3) Ramsay & Smierps, Zeitschr. Physik. Chemie 15, p. 115. Nobody seems to have 
observed as far as | know that the comparatively high value of the eritieal temp- 
erature of methylalcohol may be explained by association, as also the deviation 
from Koprp’s law for the boiling points of series of organic substances, 


( 480: } 


plait there are still two possibilities with regard to the development 
of this cross-plait: (1) the plaitpoint continues by itself and gradually 
begins to form the closing plutpoint of the liquid-plait which may 
disappear at the limiting liquid volume or (2) it disappears by meeting 
With a second plaitpoint belonging to an independent higuideplait so 
that the two plaits then form one large one, with or without a 
closing plaitpoint on the liquid side. 

The experiments confirm the above view of the effect of an 
admixture of ethane on the critical point of methylaleohol and as 
far as they go seem to show the first alternative to be the correct 
one. It appears that the general behaviour of mixtures of methyl- 
alcohol and ethane thus disclosed agrees with that of ether and 
water as predicted — without however any grounds being given — 
by Korrrwue ®) and laid down in some r-r-diagrams. On the grounds 
set forth above L support this expectation as regards ether and water. 
Addition of ether to water will lower the critical Lem perature. 


„lm, 


OR 
~e&e 


JIJ 


300 


The results for methylaleohol and ethane are laid down in figure 2. 
| can give only a short explanation here. Starting from C, — the 
critical point of methylaleohol — the critical curve runs in a per- 
feetly normal way at first, owing to the influence of the association 
being as yet insufficient. It ascends, passes through a maximum 
at 120°, and then falls, evidently tending towards the critical point 


2) Arch. Néerl. 24 p. 338— 340. 


ae 


( 481 ) 


of ethane; the association however becomes gradually stronger: the 
dip in the surface caused by this’) gradually modifies the shape of 
the cross-plait: the plaitpoint passes through a minimum pressure 
between 25° and 380°, and the eritical curve then begins to rise 
rapidly. The end of the eross-plait thus changes without a disconti- 
nuity into a liquid-plait; in the mean time the main plait goes on 
developing on the approach of the critical point of ethane: as explained 
a small subsidiary plait is formed which appears at f on the pract- 
ical part of the surface. Probably an exchange of plaitpoints occurs 
on the theoretical part, of the same nature as with the higher alco- 
hols, the result being that at low temperatures the eross-plait is cut 
through by one self-contained liquid-plait. But as far as the phen- 
omena are concerned this is entirely immaterial. 

As far as the experiments could be carried (i.e. up to 275 
atmospheres) the critical curve continued to rise towards the left, so 
that there is no indication of the existence of a different plaitpoint. 
The rapidity with which the mixing-pressure inereases is truly 
remarkable. 

If we compare the figures for methylaleohol and for the higher 
terms, a certain resemblance will be noticed, especially if we do not 
assume the contraction of the closed plait to nothing in the latter 
case. The association tends to produce the same modification in 
the usual diagram in both cases, but the acting causes appear to be 
much more effective with methylalcohol — the stronger association 
of the alcohol, possibly a smaller mutual attraction or the influence 
suggested by Prof. vax per Waars of the small molecular volume of 
the aleohol may contribute to this result. For this substance the 
plaitpoint remains outside the eross-plait at low temperatures, with 
the others it succeeds in disappearing inside, Whether inside this 
plait any changes take place similar to those occurring with methyl- 
alcohol on the practical part of the surface we cannot tell. But in 
any case T have assured myself that with ethylalcohol a new plait- 
point curve does not appear down to — 78 : ethylaleohol and ethane 
remain miscible in all proportions. ; 

Methylaleohol and ethane mir by pressure. Im this respect they 
contrast with mixtures phenol and water for which the liquid plait 
above a certain temperature far below the critical region separates 
completely from the cross-plait and thus has a plaitpoint on the side 
of the positive r-axis. In view of the probable disappearance of the 
association at high temperatures it is possible that in the latter case 


1) Continuitét ete. I. p. 191. 


( 482 j 


further experiments will disclose a second plaitpoint on the liquid 
side of the plait, as predicted many years ago by vAN DER WAALS 
from the value of the volume-constants. L expect to be able to throw 
more light on this subject by the continuation of my investigation with 
the higher hydrocarbons. Ether and water behave in all probability 
in A manner similar to methylalcohol and ethane. 


Chemistry. — “Ou the so-called compounds of salts of sulphon- 
carboxylic acids with sulphuric esters”? By Prof. A. P. N. 
FRANCHIMONT. 


(Communicated in the meeting of January 34, 1905). 


The first of this kind of compounds was obtained accidentally by 
Lacee in 1879 in the laboratory of Grerner in Jena. He wanted to 
reduce sodium sulphonacetate with soditun amalgam and water, but 
after acidifying with sulphuric acid, evaporating, and extracting with 
absolute alcohol, he obtained an acid liquid which gave with barium 
carbonate a salt of the empirical composition C, H,, Bad, O,,. This 
salt has, therefore, the composition of one molecule of barium 
sulphonacetate plus one molecule of ethyl sulphate plus one molecule 
of water and may, according to Gmrurmer, be considered as a deriv- 
ative of a disulphurie acid in which two hydrogen atoms have been 
replaced by ethyl groups and one OH group by the group CH,—COOH. 
He obtained the same compound by digesting a mixture of sodium 
sulphonacetate, sodium-hydrogen sulphate and alcohol. The acid was 
called “ Diaethylessigdischive felsinve”. Acetic acid itself did not yield 
wv similar compound. 

In 1885, in the same laboratory, STENGEL successfully attempted 
to obtain a similar compound with metasulphobenzoie acid; the 
analysis gave the composition C,,H,,0,5, Ba + 3'/,H,O. The acid 
was called“ Diaethylbenzordischire felsiure”. Analogous compounds 
were also obtained with methyl and propyl alcohol. _ Benzoie acid, 
however, did not give a similar compound and it is, therefore, attri- 
buted to the sulphonic acid) group. 

ENGELCKE Obtained similar compounds with isethionie acid but not 
with benzenesulphonie acid and _NrermaeK did not obtain it with 
methylsulphonie acid. 

Greener looked upon these compounds as salts of a derivative of 

() () 


/ 


ck © FOCAL 

/ fit 2 u 

disulphurie acid S,O,H, such as C, H, — ae > a 
0 


CO,H OH 


( 485 } 


In Beusren’s “Handbuch”, however, these compounds are deseribed 
as double compounds of salts of sulphoncarboxvlie acid with neutral 
sulphuric esters. 

Kor a long time, however, [| have felt serious objections to this 
theory. T had already repeated the experiments with sulphonacetie 
acid and metasulphobenzoie acid but did not obtain pure compounds. 
To was also unsuccessful in attempting a synthesis by means of the 
salts of sulphoncarboxylie acids and dimethyl- and diaethylsulphate. 
The phenomena observed during this research induced me to request 
Dr. Artema to try to obtain compounds of the same empirical 
composition in a different manner, namely by bringing together 
in molecular proportions the barium salts of the acid esters of meta- 
sulphobenzoie acid with the barium salts of the alkylsulphuric acids. 
If in this proportion they yield a compound this ought then to have 
the same empirical composition as the last named compound. 

Dr. ATrEMA now observed that on evaporating a solution containing 
in molecular proportions the barium salt of the ethyl ester of meta- 
sulphobenzoic acid and barium ethylsulphate, the greater portion of 
the ethylbarium salt of metasulphobenzoie acid was deposited first 
in beautiful crystals; after this a double compound of the two barium 
salts made its appearance im the form of large rosettes of tender 
needle-shaped crystals whilst) from the motherliquor barium ethvl- 
sulphate was obtained. If an excess of barium ethylsulphate is taken 
for instance, 5 grams of the same to | gram of the salt of barium 
ester the double compound separates immediately and from the 
motherliquor barium ethylsulphate is obtained. The double compound 
cannot be recrystallised) from water; its aqueous solution presents 
the same phenomena as one containing in molecular proportion 
the two salts; on evaporation, the salt of barium ester crystallises 
first, then the double compound and finally the barium ethylsulphate. 
As the double compound cannot be recrystallised from alcohol it 
was freed from motherliquor by strong pressure and analysed. The 
results of the analyses of three different preparations were concordant 
and agreed with the formula: 


CO, C, H 


u 


Aa , Ba + (C, H, SO), Ba + 6 H,O. 


Dr. Artema has afterwards repeated STENGEL’S method of preparing 
the compounds, but here he also obtained first the ethyl barium salt 
of metasulphobenzoie acid and afterwards, although less readily, 


( 484 ) 


the double compound. An analogous result was obtained with the 
methyl compound, 

We may, therefore, come to the conclusion that there exist no 
compounds of salts of sulphoncarboxylic acids with neutral sulphurie 
esters; there exist, however, double compounds of salts of the acid 
esters of sulphoncarboxylie acids with salts of the acid sulphuric esters. 
This result gives rise to a number of questions some of which 
Dr. Arrrema intends answering by practical experiments. Both salts 
ave alkyl-metallic salts of dibasie acids whose acidic functions (at 
all events in the case of metasulphobenzoic acid) have a very 
different power, whilst sulphuric acid as oxysulphonie acid is some- 
what comparable to isethionie acid which also exhibits the property. 


Mathematics. — “On the spheres of Moxan belonging to ordinary 
and tangential pencils of quadratic surfaces.” By Prof. JAN 


pr VRIES. 


1. In Part I of the “Proceedings of the Section of Sciences” 
pages 305—310, 1 have developed, making use of FinpiEr’s cyelo- 
graphic representation, some properties with respect to the system 
of the orthoptical circles of the conics of a linear system. By 
extending Firpier’s considerations to a four-dimensional space the 
corresponding case of the three-dimensional space might be treated. 
In the following essay the indicated extension on quadratic surfaces is 
arrived at analytically. 

Given P the point of intersection of three mutually perpendicular 
tangent planes of the quadratic surface S* represented by the equation 
a,, +a, ta, 2+2a,, ey Aa, v2+2 a, yet 2a,, 7+2 a,, yd 
4 2a,,2+a,, =0. 

These three tangent planes form with every fourth tangent plane 
a tetrahedron circumscribed about SS? that may be regarded as polar 
tetrahedron with respect to the point-sphere (isotropic cone) /* repre- 
sented by 

(ee) zie Os Cn la (zz) — 
So the invariant @ belonging to S? and 7? is equal to zero’). 


Therefore we have: 


1) See a.o. Sanmon-Fiepier, Anal. Geom, des Raumes, 3d edition, vol. I, p. 253, 


where S? is represented by an ellipsoid, 


Gi, A, Ais ove Wa | dir UN, 0 di4 
Eend 0 ae yn dan () as, 
en EE 
Uiz M5, gs Ei O13, Ug I Us, 
Gi, yy gy (w? 4 Dn di Gig Cay TT Er Oy, | 
| U () (hs hy, | 1. (ths by, | 
Us I sy ey 0 daa yy gy 
An + = 0 
this () pg «Gas () Cag A gy lbs 
a, fi Ten in as Ch, 4 uly by, Cs, a 14 
If we-vepresent the minor of ain A= = + a,,a,,a,,4,, by 


Aj, it ensues from this relation that-the locus of the point 2 is 
indicated by the following equation (where the indices of the coor- 
dinates are left out) 

rt ron nr es Wee ae (Ay eae yA; 2) zin (hee eet 

So the locus of the points of intersection of triplets of mutually 
perpendicular tangent planes of iS? is a sphere (Moner). 

The tangential cone to S’ with vertex / possessing three mutually 
perpendicular tangent planes, the tangent planes form according to 
a well-known property an infinite number of triplets of mutually 
perpendicular planes. 

For A,,=0 we find S* to be a paraboloid and the sphere ot 
Moncr degenerates into a plane. 

The obtained equation can be replaced by 


ae) ey ae 1 S (A? 1 A) 
U —- ae ee i ——  — _ ar Ka nand — ZZE | 4 d EK ml 4 . 
Ai, 7 8 A A A? 3 2 ke 


/ 44/ 14) 
Now however 4,,4,, — A’,, is equal to (a,,4,, — «?,,) 4. *) 
The radius of the sphere is indicated by the square root out of 


= 1e, = (4,505, — 443) 
Consequently the sphere of Moren will be reduced to a point- 
sphere when S? is a cone (40) or into an equilateral hyperboloid 
if namely the equation 


1) This ensues inter alia from 


Cit Ome Oya Oy a pas AN As A, A Oye ss, 0 
Bie Aer Aas ds | 0 | 0 0 CH Pender dere 0 
OR AT UR cc 0 0) 1 0 rl bs Ca. 0 
(i) ag EE TI An, sage as Ast EET rds PN A 


(See a.o. Batrzer, Determinanten, oth edition, p. 63). 


( 486 ) 


(a,,¢,, — A73) + (¢,,4,,; — @7,,) + (a,,0 


is satisfied. 
In the latter case the asymptotic cone possesses as is known oe! 


triplets of mutually perpendicular tangent planes, 


2. When in the equation 


Bie (dy He = Er Pein | t Age >) + (Aril Aside 0 
we substitute aj, + 2 bij for aj, the new equation represents the 
system of the spheres of Moren belonging to the quadratic surfaces 
of a pencil. 

The equation is a cubic one in 2; so the indicated spheres form 
a system with index 3, that is, through each point three spheres pass. 

If for brevity’s sake we represent the formula 


we -}- a — Py, Lv t 1. U -f- ae 


by Cy, the eubie equation is 
Cea FAG we Al Oelen S20, 
The power of a point with respect to the sphere (4) is then equal to 
LCA HLC A HLC AH CE, 
ER rens 
This expression becomes independent of À for the centre of the 
sphere cutting the four spheres (% orthogonally; all the spheres 
of the indicated system are intersected at right angles by a fived sphere. 
On this orthogonal sphere the point-spheres of the system are of 
course situated; so it contains in the first place the vertices of the four 
cones, in the second place the centres of the two equilateral hyperbo- 
fords”) belonging to the pencil. 
From this ensues that the locus of the centres of the spheres is 


a skew cubic. This is moreover confirmed by the observation that in 


Ek | En A, SA 


24 44 
the aaumerators and the denominators are cubic forms in 2. 

The square of the radius being represented by the quotient of two 
forms of order six in 2, the system contains six spheres with given 


radius, 


3. The quadratic surface indicated by the equation in tangential 


coordinates S, 1, § 


1) Their parameters are determined by 


2 ele A) (a+ ihe A) ae (Gee aes A)*| — ie 


( 487 ) 
pita +22 a, En 220,8 Bij == 0 
€ 5 8 


has for equation in point coordinates 
SS ‚3 RE , ‘ 5 ‘ = 
2A, @ +22 Aa ya 2 AL, e+ His == 05 
3 3 3 


If now ee is the minor of the determinant  -+- A 


LI As Ais Aye 
corresponding to dj, the sphere of Morr of the indicated surface 


is represented by 


Ce py Pe) Sl ,¢4-a,,y--c,,2) + (Ha He.) = 0. 


But we have!) eip=ain£®; so this equation can be replaced bv 
REN Bet ap eee rde daalt dare 4 (0, x], as.) == 0, 


or by 


2 2 3 
“ “ a ] 
14 24 + 34 mie EN 2 
(— ) EE G ) Es (: -—— ) == (Gis ee U): 
Wa a Us Ae as 


So for a tangential pencil of quadratic surfaces we find 


(Apt PI Gey 27) oe = (@,,+6,,4) e+ Bit bin 4) — 0, 
3 


that is, the corresponding spheres of Monon form a pencil. 
To this belong the point-spheres indicated by 


a KCP ker en A) (ast daa ANS 0 


originating from two equilateral hyperboloids, and the plane determined 
by a,,+4,,4=0 belonging to the paraboloid of the tangential 


pencil. 


Physics. — “The variability with the density of the quantity boy 
the equation of state.” By Dr. J. D. van per Waars Jr. Com- 


municated by Prof. J. D. van pur Waars. 


§ 1. If we suppose the molecules of a gas?) to be perfectly 
smooth, elastic spheres, the influence of the fact that their diameter 
is not infinitely small, on the form of the equation of state may be 
allowed for in first approximation by diminishing the volume |, in 
which the gas is contained, with four times the volume of the mole- 
eules. If we understand by distance sphere a sphere described) con- 
centric with a molecule and with a radius 2 6 (where 6 denotes the 
1) See inter alia Barrzer, Lc. p. 65. 

2) | say only “gas” not “gas or liquid”, for we must not apply the formula 
for a liquid without introducing still other approximated terms than those that will 


be discussed here, 


( 488 ) 


radius of the molecule), then we may also say, that we must diminish 
with half the combined volumes of the distance spheres, which 
quantity is usually denoted by 4, or by 6, if we wish to take into 
account the variability of the correction in consequence of variation 
in density. Various methods have been followed in order to investigate 
this influence; all these methods vielded a conformable result, so that 
no reasonable doubt can exist as to the correctness of this statement. 

We should be inclined to deduce from this, that the influence may 
he correctly allowed for in second approximation by diminishing 
I” with half the volume really occupied by the distance spheres, in 
Which a segment which two distance spheres have in common, is 
counted only once, or what comes to the same, by writing hb, — 2S 
instead of b,, 2S representing the sum of all the segments which 
are covered by two distance spheres at the same time. The correc- 
tion has been introduced in this way by Prof. J.D. vax per WAALS 5); 
and Dr. J. J. van Laar?) has made a calculation of a second correc- 
tion term, which is based on a similar supposition. 1 will however 
confine myself to the discussion of the first correction term, for which 

17 15 

we find in this way = = The question whether the first correction 
term is correctly found in this way has not been answered un- 
animously in the affirmative. _ BorrTZMANN *) follows quite a different 


» 2 


le 4] r 
gep. 


communication in these Proceedings expressed the wish that his 


method for calculating it and finds Phough BoLrzMann in his 


publication of this result differing from my father’s would give rise 
to a discussion by which this doubtful point might be elucidated, 
no discussion has followed by which the question has been settled 
conclusively. Now I think I can show that there is no reason for 


pee 17h, 
introducing the correction in the way which yields the value 30 
OL 


and at the same time | will give a reasoning, by which the term 


3}? 


is derived in a shorter way than that followed by BorrzMars, 


8 V 
The simplest way to show clearly what supposition we must 
; ro 
make in order to get the correction term 55 738 to start from the 
og 


1) Versl. Kon. Akad. v. Wetensch. V. p. 150. Oct. 1896. 

2) These Proceedings Vol. I, p. 273. Jan. 1899. 

3) These Proceedings Vol. 1, p. 398. March 1899; and “Vorlesungen über 
Gastheorie” If, p. Lol. 


( 489 } 


virial equation as my father has done for the external pressure and 
for the pressure of the molecular attraction in Chapter IL of his 
“De Continuiteit van den Gas- en Vloeistoftoestand” and for the 
forces eventuating in collisions of two molecules in these Proceedings 
ol Tops too. Oct; 1695. 

First, however, T will point out, that the virial equation need not 
necessarily be applied for a definite quantity of matter, which is 
contained in a definite volume and enclosed within a solid wall, as 
is the usual method of applying it. We may as well apply that 
equation for a part of a homogeneous phase, separated by an 
maginary separating surface from the surrounding substance which 
is in the same phase. We shall not always find the same molecules 
within such a surface, but we may assume, that at two different 
instants f and f, we shall find the same number or at least with 


1 
very great approximation the same number of molecules within it, 


du: 
and that the expression = Mit — Will also have the same value af 
dt 
the instants ¢, and ¢,. We may therefore put: 
dede 
mt = 0 
dt dt 


and also the corresponding equations for the y- and for the z- 
coordinate. 

From this we may deduce ; 

dm din iy din 2 7 
ams == |t -y—t2 ec ie eee 
dt er rel dt 

In the ease that we may neelect the volume of the molecules 
with regard to the volume in which they are contained, and that 
we may assume that the molecular forces act in such a wav that 
they yield on average zero for the force exercised on a molecule 
Within a homogeneous phase, the righthand member of this equation 
has only a value at the border of the volume under consideration: 
it may therefore be reduced to a surface-integral. 

The lJefthand member of this equation is independent of the circum. 
stance whether the space under consideration is enclosed within 
an imaginary separating surface or within a solid wall, and in the 
latter case it is also quite independent of the properties of this wall. 
So the righthand member cannot depend upon these circtunstances 

dm ? 
either. In the case of a solid wall we may write: 2 = ().. -So'-we 


get for the righthand member: 


Proceedings Royal Acad. Amsterdam. Vol, V, 


( 490 ) 


fr roo (a, f) do = 3 PVE > teen ee en 


Here r represents the radius vector drawn from the origin of the 
system of coordinates to a point of the surface, do represents an 
element of that surface, cos (7,7) the cosine of the angle which the 
radius rector forms with the normal to the surface. 7?’ is the force 
per unit of surface which prevents the molecules to leave the space and 
compels them to return towards the inside of it. We may distinguish 


a 


in it the molecular pressure — and the pressure p exercised by the 
: 
wall. 
: , ’ p d's 
For the case of an imaginary separating surface, —m— is the 
i dt dt 


momentum in the direction of the positive v-axis conveyed through 
the surface to the inside of it. Momentum conveyed to the outside 
has to be taken into account with the negative sign. In this case 
also the righthand member may be represented by equation (/) 
though here the symbol 7?’ does not any longer represent a force 
which really acts on the molecules. 

In the case that the volume really occupied by the molecules 
is not so small that we may neglect it, also the virial of the 
forces eventuating in the mutual collisions of the molecules must be 
taken into account. If we denote this virial by / then we may 
write equation (4) in the following form: 


=ms? = — 1 a Pr cos (n, r) do = — I + 3 PV. 


Sms? and J being independent of the properties of the bordering 
surface, P cannot depend upon them either. /? appears to be greater 
than P’; for a wall this is because the number of collisions is 
augmented in consequence of the abbreviation of the mean length 
of path which a molecule describes between two successive collisions; 
for an imaginary separating surface this is because the conveyance 
of momentum through that surface has augmented in consequence 
of the fact that in collisions between two molecules whose centers 
lie at opposite sides of the separating surface, the momentum is 
transplaced instantaneously from the center of one molecule to that 
of the other; so the momentum has been transported with infinite 
velocity. 

But the way in which we have derived the quantity 2? which 
may be estimated to represent the pressure prevailing in the gaseous 
or in the liquid) phase, warrants in any case that this quantity is 


( 491 ) 


independent of the shape of the vessel and the properties of the 
walls in which the phase is enclosed, but on the other hand it 
warrants also that we may find the quantity 2? by calculating the 
pressure which would be exercised against a plane wall if the 


at 
molceules did not attract one another, or by adding —— to the pres- 
i? 


sure exercised by mutually attracting molecules against a plane wall. 

The way in which the virial of the forces eventuating in mutual 
collisions of the molecules has been introduced bij Prof. vay DER 
\Waars is as follows. We assume that in first approximation 7? 
represents also the pressure exercised on the distance spheres of the 
molecules. This would yield the value 2 /%, for the virial. We 
must, however, take only half this value, else all the forces would 
have been counted twice. ; 

The distance spheres, however, cannot be considered as unmoving 
solid walls, but as moving and movable walls and therefore it is 
perhaps not quite superfluous to show expressly that they are indeed 
subjected to a pressure amounting in first approximation on average 
to P.L will give the proof of this proposition in § 2 of this com- 


munication. 
ar ages ; ; Watney 
Phe introduction of the correction term . 5 ir is based on the con- 
Fo a) 


sideration that the value of the virial given above will be too great 
because some of the distance spheres partly coincide. The parts of 
the surface of a distance sphere I falling within a distance sphere 11 
are protected from collisions with all other molecules but LL. There- 
fore the pressure om such parts is assumed to be zero; on the other 
parts the pressure on the distance spheres is supposed to be 2. This 
comes to the same as the assumption that the average pressure 
during a time T (and every pressure which we consider, the pressure 
P also, cannot be anything else but an average value during a certain 
time tr) exercised on an element do of a distance sphere would 
be smaller than /?, because of the fact that the element do is only 
during a part of the time 7 exposed to the pressure 7, during ano- 
ther part of that time, however, it would have been subjected to no 
pressure, because if was protected by the distance sphere of a mole- 
cule IL from collisions with other molecules. 

IT have two objections to the calculations based on these considerations. 

In the first place the assumption is made, that a part of a distance 
sphere would never experience any pressure, when it lies within 
the distance sphere of another molecule. In fact the reverse is true: 
in order that a surface element should experience a pressure, a 


33% 


(492) 


molecule must collide against it and then it lies in the distance 
sphere of that molecule; and the considerations in which the pressure 
inside the distance spheres is assumed to be zero, outside them to 
be P, are certainly not a correct representation of what really happens. 
Yet points lying inside distance spheres are in somewhat different 
conditions as to the pressure that may be exercised on them, than 
points outside distance spheres. It is not clear to me how these 
conditions should be taken into account. It is, however, not necessary 
to know this in order to caleulate the correction term, as will appear 
from my second objection. 

In the second place the fact has been overlooked that not only 
some paris of distance spheres lie within other distance spheres but 
that the same circumstance occurs for parts of the bordering surface. 
It is indifferent whether this is an imaginary surface or a solid 
wall’), in any case a part of it will lie within the distance spheres 
of the molecules, and may therefore with as much (or as little) right 
be estimated to be protected from pressure. Now let 1/4 part of the 
bordering surface lie within the distance spheres. If we must assume 
that this part of the surface experiences a pressure zero, and that the 
free surface experiences a certain pressure, that we will call P,, 


then the quantity 7, which represents — as appears from the way 
in which it has been introduced — the average pressure, would be 
A—l 


Let us now investigate what part of the total sur- 


equal to —— /,. 
4 


face of the distance spheres lies within other distance spheres, and 
let 1/2, represent that fraction, then the average pressure of a distance 


A 5 | 7 
sphere will amount to /?,. If4, were equal to 4, then the average 
R 7) 
1 
pressure on the bordering surface and on the distance spheres would 
be the same, and we should not have to apply any correction to the 


term bon : 


Lip: 
We find the correction ferm 55 5 if we make the following 
rp 4) 
assumption, but only in that case: every surface element, — no mat- 


ter whether it is a part of a solid wall or of an imaginary separating 
surface, and whether the surface is plane or curved and no matter 
whether it hes within or without the distance spheres of molecules — 


1) The virial of the forces excercised by the wall must properly not be integrated 
over the wall itself, but over the surface which contains the centers of the mole- 
cules colliding against the wall, i.e. over a surface parallel to the wall and lying 
at a distance @ from it. 


ee a 


( 493°) 


it will always experience a pressure PP. Only the distance spheres 
make an exception to this rule, for parts of them, falling within 
other distance spheres experience a pressure zero. 
Lean find no reason for this exception and therefore 1 think the 
WIED, it 
value 39 yr incorrect, The question Whether in fact a correction must 
be applied depends on the fact whether 4, is equal to 2 or not. This 
may be investigated in the following manner. 


Let M/ in the figure represent the center of a molecule and let 
the circle described with J/ as center, represent the section of the 
distance sphere (1) of that molecule with the paper. Now we are to 
calculate the average pressure exercised during a time Ton a surface 
element do, the center of which we call the point 7? To this pur- 
pose we describe a circle Il with P as center and with a radius 
26 and we also consider the tangent plane in 7? which we call ZA. 

Two cases may be distinguished: 

Ist The space within sphere Il but outside sphere 1 and at the 
left of the tangent plane (the section of the space in question with 
the paper has been hatched in the figure) may contain the center 
of a molecule; if this is the case P lies within the distance sphere 
of that molecule. 


( 494 j 


2nd The space under consideration may not contain the center of 
any molecule. 
We will call that part of the time + during which the former 


T 
takes place —; so that part during which the latter takes place 
u 


‘ 
ul ik u— 1 Ge. 
7. During the time ~——7 the surface element do is quite in 
u u 
the same circumstances as an element of a plane wall. Therefore if 
will experience on average a pressure 7. This pressure Pis a quan- 
tity which we may derive from the virial equation; in order to deter- 


mine it, it is therefore not required to decide whether the considerations 


„ll 
in consequence of which we find / equal to —~— P, are correct or 
i 
2 4 ; 9 T 
not. But when the former case takes place, so during the time —, 
2 


‘ 
we are certainly justified in assuming that do does not experience 
= ec 
any pressure. The average pressure on do is therefore re 
u 
We may find the value of gw in first approximation by determining 
the volume 7 of the hatched space, and by assuming that the chance 
that a certain definite molecule will lie within that volume is equal 
v ‘ : . 
to 7: If » denotes the total number of molecules, then the chance 
. . v 
that the space contains a molecule will be represented by 7 7 On 


average the value of */u will be equal to this chance: therefore in 
EN 


I 


first approximation (= 7 


We find by a simple calculation for + the value eu r* where 


ry = 2¢6= the radius of a distance sphere. Therefore: 
i 
i May | ’ 
- LA 4 a ei 
u ee = ah 
J Seyi 


„…) 


) he 
The internal virial Z will therefore be 3 2?b, (1 — — zl and 


equation (1) assumes the following shape: 


eel an i a he 
Ems = PVP, Ge 8 = )=P(v bd a 


§ 2. In order to introduce the internal virial / T started from the 
supposition that the distance spheres of the molecules experience a 
pressure which is on average equal to P. As I never found a direct 
proof of this thesis I will give it here. The pressure / namely may 
i. a. be considered to represent the pressure exercised against a solid 
wnnoving wall, disregarding the molecular pressure. The distance 
spheres, however, are not to be regarded as a solid, ummoving wall. 
In consequence of their motion the number of collisions against a 
surface element do of a distance sphere is greater than that on an 
equal element of the wall; moreover the force in each collision is 
proportional to the relative velocity of the molecules, which is greater 
than the velocity of each molecule separately. 

From these two circumstances we are apt to assume that the average 
pressure on the distance spheres would be greater than 7’. 

On the other hand the impulse of a molecule colliding with a 
velocity sx normally against a solid, unmoving wall is 2ms. If, 
however, the molecule collides with the velocity s centrally against 
another unmoving molecule with the same mass, then the first molecule 
will be stopped and the second will obtain the velocity s; so the 
impulse is in this case only ns. 

In consequence of this circumstance we should be inclined to expect 
the pressure on a distance sphere to be smaller than 7. 

The following simple calculation will suffice to show that these 
influences cancel each other and that the pressure exercised on the 
distance spheres is really equal to /, at least in the case that we 
may neglect the volume of the molecules with regard to the volume 
in which they are contained. 

Let us imagine two molecules | and IL with the same mass. The 
same proposition might be proved without difficulty also for mixtures, 
so for molecuies with unequal masses, but 1 will confine myself here 
io molecules with the same mass. The velocities of the molecules 
will be denoted by s ands, and the components of these velocities 
by w,v,2 and wu,,v,,2,. The chance that molecules occur whose 
velocities have these components will be represented by 4 (az, 7, 1) 
and F'(w,,7,,7,) and the relative velocity bv s,. Then we have: 

sp? = (uu)? + (ur) + (rw). 

If we take the direction of s, as the axis of a system of spherical 
coordinates, and if we call the latitude g the longitude yw, then a 
surface element of the distance sphere of moleenle 1 will be repre- 
sented by 97? sing dys. The number cf collisions per unit of time 
of molecules of group IL against such a surface element is: 

F (u,v, vw) F (uy, vy, w,) du de dw du, dv, dw, s, 7° sin p cos p dy di. 


( 496 ) 


Not the total relative velocity s, changes its sign in a collision of 
this kind, but only the component normal to the tangent plane in 
the point in which the molecules touch one another. The impulse 
is therefore ms, cos gy. 

The total impulse of the collisions of the kind under consideration 
will therefore be equal to: 


(u,v) F (ur or) dude die du, de, diy s-° 7? sin op cos” g dg dy. 


be 
The eightfold integral of this expression vietds the total pressure 
exercised on the surface of the distance spheres. We have: 


a) 9 


| | 2 sin gy Cos” Xf dg dw == nr 
AR: 


…) 


if we integrate according to y between the limits O and 2 a and 


according to g between the limits O and > =. The limits for g are 


not O and a, for the parts of the distance sphere of molecule [ for 
which g > > a, cannot come into collision for the given relative 


velocity s,, We may write s?-+s,’, for s,? for the terms ss, cos ($,5,) 
vield zero on average. Doing this we may integrate the term with 


s? according to du,, de, and dir,; so we get: 
|” (rayo V1, te) du, do, dre, =n. 
« 


The term with s,? on the other hand may be integrated according 


to du, de and dir; so we get: 
B (u. raar) du dv dw =n. 
t 


This vields for the total pressure on the surface of the distance 


spheres : 


mr | | ms? fF (7, UW) du de dic Ee | mt EE 1 (Un Vo: ze dit, dr, div, 
=e 


c 
Both integrals in this expression are equal to uus, nes” represent- 
ing twice the mean kinetic energy of a molecule. We may there- 


fore write this expression as follows: 


Dividing this quantity by the total surface of the distance spheres 
Aarm, we get for the value of the average pressure: 


l 


— Nn MS. 


Co 


( 497. ) 


This is the same value as we find for the pressure exercised on 
a solid, ummoving wall. 
In order to ealculate the number of collisions we have here 
neglected the extension of the molecule and the mutual attraction of 
the molecules. Therefore it is apparent that we cannot have obtained 
anything else but a first approximation. 


Botanies. — “Die Stelir- Theorie’. Dissertation of Mr. J.C. Scnourn. 


(Communication of Prof. J. W. Morr). 


According to the idea of van Tinenem, given about the tissues of 
root and stem of the vascular plants, they must be divided into three 
groups or systems of tissues, namely, epidermis, cortex and central- 
cylinder. It is such a natural thing to call the epidermis a separate 
tissue that already a long time before vaN PirGrmMm, it was acknow- 
ledged and is at present generally accepted. 

It is a different thing about the theory that the central part of 
stem and root is taken up by aeylinder of tissue, the central-cy Linder 
(or ‘‘stele”), which may consist of elements differing greatly, but 
Which must nevertheless be regarded as a connected whole, forming a 
certain contrast with respect to the cortex. This consideration which 
can be called the ‘Stelar-theory” is accepted by some, rejected 
by others. It is of the greatest importance for instruction and for 
the construction of deseriptions of the inner structure, and it has 
undoubtedly for both these reasons such a great practical weight, that 
for this reason only it deserves our attention in a high degree. 
The scientific foundations for this theory are not in such a good 
condition and assuredly its non-acceptance is owing to this. Of course 
the important question is, whether this distinction between cortex 
and central-evlinder has made its appearance already at an early 
period in the phylogeny of plants. With the present state of our 
knowledge this can perhaps not be proved with certainty; but to 
be able to answer this question in the affirmative two conditions 
must be put: st. the central-evlinder must be indicated if not in 
‘all, still in the greater part of stems and roots, 294, it must appear 
already at an early period in the development of these organs. 

As for the root these conditions are amply satisfied, which gives 
great support to the theory of vaN ‘TimGHem. But this is not the case 
to such an extent for the stem, partly perhaps in connection with 
the complications formed already at an early period by the develop- 


( 498 ) 


ment of the leaves, partly in connection with the splitting up of the 
central-cylinder in these organs of many plants. Concerning the 
latter point vaN TimGHrem himself and of late a number of American 
and English investigators: GWYNNE-VAUGHAN, JEFFREY, Boopre, FAULL, 
WorspeELL, BRETZAND Farmer & Hir, Miss Farp, TAanstny & LULHAM, 
BREBNER have shed much lieht. In all those cases in which stems 
show a number of loose strings, regarded by some as parts of a 
central-eylinder (schizostely), by others as vascular bundles, a single 
central-evlinder, the monostelic structure, is rule in the voungest 
internodes of the plant, in hvpo- and epicotvl and in the internodes 
following immediately. 

But in most cases there is no question about schizostely and so 
according to VAN ‘TinGikM we must expect monostely. However it is 
a fact, that whilst in every root the most superficial microscopic 
investigation easily proves the existence of a central-cylinder, this is 
not at all the case for many stems. The inner layer of the cortex 
(endodermis), it is true, is often developed as a bundle-sheath 
indicating as that of the root does, the boundary of the central- 
evlinder, or also it contains starch-grains, so that a distinct starch- 
sheath is formed; but in a great many other cases, also in an inves- 
tigation made for that purpose, as was done by H. Fiscumr, it has 
not been possible to point out a well defined central-evlinder. Fiscuer 
found in LOO investigated plants only in 32 cases a distinct endodermis. 

It has now been shown by Mr. ScHourr that this objection to the 
Stelar-theory does not exist in reality. He collected out of the lite- 
rature on this subject numbers of cases, in which a distinct endodermis 
had been observed in some shape or other. He himself studied a 
great number of stems of different plants and then it was evident 
how necessary it is to examine these organs in different and especially 
in voung stages of their development, a thing Frsener kad not done. The 
result of this method of working was, that of about 400 dicotyledonous 
plants only in 7 no distinct endodermis was come across and among 
these 7 there were vet 4 which even showed a sharp boundary of 
the central-cylinder. Also the greater part of the Monocotyledonous 
plants possess an endodermis. It is not to be found in Gymnosperms 
but vet here as is the case in most of the above-mentioned exceptions, 
a distinct boundary between cortex and central-cylinder is often to 
be seen. So this result is very favourable for the Stelar-theory and 
is a contribution to its seientifie confirmation. 

But in yet another manner has Mr. Senovre endeavoured to test 
the Stelar-theorv, a test, which it is true has led to a negative result, 


but which enables us to draw weighty conclusions with regard to 


( 499 ) 


the value of the well known Theory of the histogens of Hansrrr. 

In working out his theory van /PrrGumMm purposely avoided as 
much as possible to make use of the history of development, and as 
has been proved justly. Yet it was quite natural to think that there 
Was a connection between the structure of the full-grown stem and 
root and that of the same organs at avery early period of development, 
in embryo or growing point. For THaxstmin had established a doctrine 
about the structure of the meristems, very much like var Tinguem’s 
theory and had gamed a number of adherents. He thought, especially 
on account of the arrangement of the otherwise equivalent cells, to be 
able to distinguish three tissues in those meristems, called dermatogen, 
periblem and plerome. The last was a column of cells in the middle 
part of the stem and root. Of course it was quite natural to think 
of an identity of dermatogen and epidermis, periblem and cortex, 
plerome and central-eylinder, in such a manner that the latter had 
developed out of the former. Tf it were possible to point out such 
a correspondence, this would be for the Stelar-theorv as well as for 
the Theory of the histogens of great importance, though not of equal 
importance for both. If the eentral-eylinder is already found in the 
meristem as an independent whole, this points to the faet, that the 
differentiation of this tissue is old and then the Stelar-theory has 
gained another support. But as 1 said above, it is fully established in 
another way and can very well do without this support. 

The Haysruiy-theory of the histogens is a different case. Every one 
Who studies the literature impartially, will have to own that this 
doctrine resis on a very weak foundation, perhaps not with respect to 
the dermatogen, but very certainly as far as the plerome is concerned. 
It is true, there are some roots and a very few stems in whose thin tops 
the cells are arranged in a remarkably regular order, so that a central- 
evlinder can be distinguished as plerome. But in many roots and in 
nearly all stems there is no question about tracing such an arrange- 
ment up to the growing-point. It is really to be wondered at that 
this HANsTurN-theory in its generality has found so many genuine 
adherents; this is certainly partly owing to the conviction, expressed 
by many and silently shared by others, that plerome and central- 
cylinder are one and the same. 

Yet this had never been accurately examined till it was undertaken 
by Mr. Scnourn. But it is clear, that a positive result would be of 
the greatest importance for this theory. For there is no sense in 
accepting histogens without full-grown tissues corresponding to them. 
Moreover might be expected of a positive result the possibility. of 
finding an undoubted plerome when following the boundary of 


(900.4 


the central-cylinder upwards, also in those cases in which up till 
now the efforts had not been successful, perhaps on account of the 
ereat number of cells. 

The investigation of Mr. ScHourr was an accurate comparative 
study of connected series of cross and lengthwise sections. It would 
lead me too far if L were to speak of this more in particulars. But 
in general the investigation was conducted in such a way that an 
attempt was made to pursue in the direction of the growing point 
the boundary between the series of cells which could be distinguished 
as endodermis and central-evlinder in the older parts. The results 
were in short as follows. 

Of the root of Hyacinthus orientalis and Linum usitatissimum the 
series of cells of the endodermis and the outer laver of the central- 
cylinder (pericycle) were successfully and uninterruptedly pursued up 
fo the growing-point. In these cases a cylinder of tissue could be 
distinguished in the top, which could quite naturally be compared to 
the plerome of Haxstem and which corresponded exactly to the later 
central-eylinder. Also in Helianthus annuus in the main the same 
was found, though the plerome did not appear here as a complex 
of cells closed at the top. In the stem of Hippurus vulgaris, one of 
the few stems in which different investigators have distinguished a 
plerome, this was not only successfully found back, but also the series 
of cells of endodermis and perievele could be pursued uninterrup- 
tedly to the growing-point. However the cells of the plerome proved 
fo form not only the central-cylinder but also the endodermis and 
two layers of cells of the cortex, so that the required correspon- 
dence did not exist here. In the stem of L/odea canadensis an un- 
certain result was obtained, as here a starch-sheath and a bundle- 
sheath were found, and it was not possible to make out which of 
the two must be regarded as endodermis. But in the root of /icaria 
ranunculoides and in the stalks of Aesculus Hippocastanum, Lysi- 
machia Bphemerum, Heonymus europaeus and Ajuga reptans an im- 
portant negative result was obtained. Here it was perfectly evident 
that the series of cells of endodermis and = pericycle cannot be 
pursued up to the top, but that they very soon stop short and are 
replaced by shorter series of cells not exactly im their prolongation 
and whieh in their turn soon undergo the same fate. In other words 
in all these cases the expectation was not only disappointed that in 
this way in difficult cases a plerome was to be found, but it was 
also irrefutably established that it does not exist here. 

After the above-mentioned explanations it need not be demonstrated 
that these results as a whole must be regarded as fatal to the Theory 


( 501 ) 


of the histogens. That in some selected roots there is some corres- 
pondenee, makes no difference. That in slender tops built up out of 
relatively few, lengthwise series of cells a regular arrangement of cells 
may appear as was described above, is the most natural thing in 
the world. To give a particular explanation of this is unnecessary, 
and in no case are these single indications sufficient to establish 
solely on them a theory of histogens as’ that of Hansrmm. And vet 
this would have to be done if one wished to adhere to this theory, 
for all other facts plead strongly against it. Mippuris, almost the only 
plant showing a plerome in the stem, has a structure altogether 
opposed to the theory. And the irregularly built tops form without 
doubt the overpowering majority. 

It seems to me that bv the investigation of Mr. Scnourn the 
Histogen theory of HANSTRIN is proved to be erroneous. A conclusion 
of somewhat general importance can still be deduced from these 
investigations. Many botanists think that to the celldivision in 
meristems a certain phylogenetic importance must be given, somewhat 
comparable to that of the germinal lavers in zoology. But here is 
forgotten that in zoology in the history of development folds and again 
folds are spoken of, to a certain extent also histological differentiation 
is mentioned, but litthe or nothing of directions of cell-division or of 
arrangements of otherwise entirely equivalent cells. If the zoologist 
attains at beautiful results by the study of the history of development, 
it in nowise ensues from this that the study of the arrangement of 
cells in meristems will be able to furnish these. Rather will the 
hotaunist have to expect such explanations from the study of the 
development of outer forms, and of inner differentiations as a result 
of differences in the nature of cells. Experience has taught us ihat 
this expectation has a right to exist. But the Histogen-theory has 
certainly contributed to nourish the above mentioned wrong opimon. 
Now that this has been proved to be incorrect we may expect that the 
historie and phylogenetic importance which has often been ascribed 
to the divisions and arrangements of nondifferentiated and perfectly 
equivalent meristemeells will be reduced to its right and very slight 


proportion, 


Groningen, Jan. 29, 1905. 


( 502 ) 


Physics. — “Methods and apparatus used in the eryogente labora- 
tory. LLL Baths of very muf orm and constant low temperatures 
in the cryostat? Communication N°. 83 from the physical 


laboratory at Leiden by Prof. TH. KAMERLINGH ONNES, 
(Communicated in the meeting of December 27, 1902.) 


§ 1. By means of the cryostat deseribed in $ 8, Comm. 14. Dee. 


94, and § 3, Comm. 51. Sept. '99 we can obtain a bath of 


liquefied gas which is shut off from the atmosphere and boils at 
ordinary or diminished pressure. In such a bath the temperature 
is sufficiently uniform and constant for many experiments and mea- 
surements. If we use almost pure gases and if the evaporated gas 
is regularly recondensed by means of a compression apparatus, 
which as deseribed in Comms. 14. Dec. °94, 53. Sept. “99 and 54. 
Jan. (00, does not contaminate the gas, the bath may be maintained 
as long as we wish. The operations in the bath itself as well as the 
addition of the liquefied gas can be watched through the observing 
glasses. Vacuum glasses are not required so that similar cryostats 
may be constructed for measuring apparatus of any dimensions, 
Before lone we shall describe a cryostat where the gas apparatus 
and the bath are more independent. 

I was led to deseribe the form of the cryostat, as it occurs in 
Comm. 51, through the communication of the results for the di-electric 
constants of liquid gases. (Comm. 52 Oct. 99), for which measurements 
only the temperatures of — 90 Cor — 182°C. were required. For 
other measurements, however, a measuring apparatus, once immersed 
in the eryostat, has been used at the whole range of temperatures 


between, — 23° C. (boiling point of methyl chloride at ordinary pres- 
sure) and — 210° C. (nitrogen at reduced pressure), given by methyl 


chloride nitrous-oxide, ethylene, methane, oxygen and nitrogen as they 
were successively admitted into the cryostat. 

For a long time improvements have been made in this cryostat 
by means of which we can attain a much greater uniformity ane 
constancy in the temperature, while retaining the afore-mentioned 
advantages. A description of these alterations has now become neces- 
sary in order to judge of the accuracy of the temperature readings 
in the results from various measurements where we have availed 
ourselves of these improvements. These measurements will be treated 
in the next communications. Among others I mention here those 
bearing upon the isothermals of diatomic gases (Comms. 69 March “OL 


= 


( 508 ) 


and 78, March ’02) and the comparison between the platinum resistance 
thermometer and the hydrogen thermometer (Comm. 77 Febr. ’02) In 
this description, as in Comm. 51. Sept. 99, it seems to me desirable to 
illustrate the use of the cryostat by means of a special example. We 
will consider the comparison of the hydrogen thermometer with 
the resistance thermometer where also a thermo-element had been 
immersed in the bath. . 

Plate T shows the cryostat and some of the auxiliary apparatus 
to scale, the connections are represented schematically. It has been 
drawn on a smaller seale than plate L of Comm. 51 Sept. 99, (which 
should be consulted together with the one now given) but it will suffice 
to give a survey of the whole arrangement and to show some 
of the alterations. While the details of the unmodified parts can be 
studied on plate 1 of Comm. 51, plate I of the present Communication 
shows the details of the parts enclosed by the dot-dash-line of plate I, 
as far as they are required for consideration of the new arrangements. 
The connection of the apparatus shown in Pl. | with the gas ciren- 
lation can be seen in Pl. IV Comm. 51. The comparison of the 
platinum thermometer p and the hydrogen thermometer 7% and their 
connections to the other pieces of the apparatus are given in Comm. 77 
Febr. (02 §3. For the comparison of the thermo-element @ 1 amas 
yet obliged to refer to the very rough diagram of 1896 (Pl. 1 of 
Comm. 27 Mai and June °96). The communication, however, of some 
results for which the temperatures have been determined by means 
of a thermo-element will soon call for a description of the recent 
considerable improvements in the use of the thermo-elements. 

On plates Land If a correction thermometer § which is entirely 
independent of the cryostat, will be seen besides the three measuring 
apparatus mentioned above. It serves in our case to indicate the 
mean temperature of the capillary of the hydrogen thermometer, or 
in general, the mean temperature of similar pieces of measuring 
apparatus occupying the same part of the cryostat. For this 
purpose two spirals of platinum wire are wound round a glass rod, 
the one for that part of the rod, where the temperature varies slowly ¢,, 
the other for that part where the temperature varies rapidly &. By 
means of the leads ¢ 


~oo? 


connected to the places of contact §,,, 6,, and 


S,, and emerging through the tube §,,, we can determine the resis- 


tance of these spirals. 


§ 2. First we shall mention some small changes in the cryostat 
of Comm. 5l which have no relation to the question of keeping 
the temperature constant and uniform. 


( 504 ) 


The jet of liquefied gas let in at « (plate T) is directed, by means 
of the cock 4, and the filter f, against a glass wall from which it 
streams along the delivery spout D, into the bath, here a double 
beaker B, B, (Pls. I and ID), placed in the beakers 5,, B, Byot 
PL. 1 Comm. 51. The cock and filter form part of a cover which as 
deseribed in Comm. 51, may be removed together with S, and S, from 
the cryostat and may also be replaced by a syphon or a capillary with 
a cock outside the cryostat. The spreading of the jet over the 
wall may be watched through the windows |,, and the height of 
the liquid in the bath through the windows J’,. The filter / serves 
principally to prevent opaque dust from the lead (oxide of copper ete.) 
from depositing just at the place where the jet touches the glass. In 
many cases, however, it happened in spite of the care taken in purifi- 
eation, that the liquefied gas itself, while evaporating under reduced 
pressure in the cryostat, had deposited a substance, formerly dissolved 
in it but solid at the lower temperature, thus rendering the bath 
opaque. Therefore, differing from Comm, 51, a glass beaker C, (Pls. 
Land U) with numerous openings in the bottom C,, (PL ID and con- 
taining some glass wool was suspended by the regenerator spiral 4 
(Pl. L Comm. 51). This filter may be lifted from the cryostat together 
with the piece S, 

With the arrangement as described in Comm. 51 all the gas, formed 
after the liquid leaves the cock, goes in the direction indicated by 
the arrows on Pl. 1 Comm. 51. With the arrangement as described 
here, however, the gas which is formed while the bath is being filled 
follows in the main a different direction to that which afterwards 
evaporates from the bath. In fact, differing from Comm. 51, a valve 
Duo 
of the delivery spout D, for gas, but allows liquid to flow through 


with a spring D,, has been added, which almost closes the opening 


a very narrow opening D,,, along the gutter D,,. The first consi- 
derable quantities flowing from the coek, serve to cool all the beakers 
and the whole cryostat in the way indicated in Comm. 51 (the arrows 
of plate I might be borrowed: from plate I of Comm. 51), unless the 
supply becomes so great that the valve D,,, is opened and the gas 
also flows out through the opening Zè, im the ring /,, plate IL. 
The eas which later evaporates from the beaker DB, finds the valve 
D 


ned LL 
indicated by the arrows on plate II, so that it serves only to screen 


closed and escapes only through the opening /?,,, along the way 


the immediate neighbourhood of the bath from external heat. 

The difference in form between the rings Mè, and FR, on plate I 
and those on plate | Comm. 51 is very slight. This follows from the 
wish to use the parts that served in the experiments, referred to in 


( 505.4 


Comm. 51, as much as possible in the arrangement of the measuring 
apparatus considered here. Formerly the bath could be excentrically 
mounted with reference to the tube // whereas this time a central 
mounting was desirable. The existing dimensions of parts of the 
apparatus have also had the result that in the experiments described 
here the bath must be placed a little too high with regard to the 
observing glasses V,, which might easily have been avoided if we 
had been perfectly free in our construction. 

The glass ring /è,, not occurring in the arrangement of Comm. 51, 
serves still better to sereen the bath from external heat. Like the 
other beakers and glass cylinders 5, B, B, B, B,,, Bon it is 
silvered inside and outside, leaving open, however, vertical strips 
nearly corresponding in width with the resistance thermometer p. 

The conical rim B, lies loose on the beaker 4,,. When the liquid 
boils up, it streams back to 4,, along the wall of the funnel; if, 
however, B, is filled to the brim and more liquid is poured in, 
this superfluous liquid flows over into the beaker B, which also is 
filled before a measurement is made. If an intense cooling of the 
neighbourhood of the bath is required, the beakers 5, 4,, 4, must 
also be filled. It should be remembered, however, that if this is 
done, the evaporation at low pressure, as long as liquid remains 
in the outer beakers, requires a powerful vacuumpump. 

The bath itself only evaporates slowly. Instead of the double 
beakers 2, B, we might take a vacuum glass in order to diminish 
the evaporation as has sometimes been done (comp. § 3). But it is 
not always easy to obtain vacuum glasses of the required dimensions and 
internally finished with the accuracy necessary for the proper working 
of the stirring apparatus. Moreover one will not be inclined to 
immerse delicate measuring apparatus in the bath before one is suffi- 
ciently certain that the vacuum glass will not burst as such of greater 
dimensions sometimes do. 


§ 3. To make clear the purpose of the arrangements to be described 
in the next sections, it seems to me that the following particularisa- 
tions will be useful. First of all the temperature gradient in the 
bath. Even when the liquid boils regularly we find that in the lower 
layers, as a result of the hydrostatic pressure, the temperature exceeds 
that of the upper layers. If, as often happens with greatly diminished 
pressures when boiling is not produced artificially, only evaporation 
at the surface occurs instead of boiling, the temperature in the upper 
layers of the bath may fall considerably below that of the lower. 
If then the liquid suddenly boils up, which always happens whenever 

34 


Proceedings Royal Acad. Amsterdam, Vol, V, 


( 506 ) 


we do not stir vigorously, an unexpected change takes place in the 
distribution of the temperature in the bath and hence in the tempe- 
rature of any measuring apparatus placed in it. In measurements 
of the kind considered here, we cannot allow such irregularities and 
fluctuations in the temperature of the bath, either as to time or place. 

Of the various methods of preventing this sudden ebullition, the 
simplest is the generation of small bubbles of gas by means of the 
heat of a short resistance (boiling thread). If, however, there are 
ignitible gases among those successively introduced into the apparatus 
and if consequently an explosive mixture with air might be formed, 
this method is not without danger. 

To bring about ebullition a current of gas is often led through 
the liquid, which, however, has the disadvantage of contaminating 
the evaporated gas. To avoid this difficulty I have led through the 
bath a current of the gas itself. This means was applied for instance 
to avoid the retardation in boiling in the vacuum vessel mentioned 
at the end of § 2, and also in order to cause a strong stirring in 
the bath by means of the current of gasbubbles. But this means 
also presents many difficulties, mostly arising from condensation 
phenomena in the delivery tube, or higher temperature of the gas- 
bubbles; I therefore, preferred, the arrangement as described in § 4. 

If the cryostat is used as it was intended to be in Comm. 51, 
the requirements for very accurate measurements would not be 
fulfilled, even though a uniform temperature throughout the bath was 
attained. There still remains a systematic regular rise of the tempe- 
rature, because the gas used is never perfectly pure and the more 
permanent part evaporates first. In cases where measuring apparatus 
require longer to adopt the temperature of the bath than the time 
in which the temperature changes the amount permitted by the 
accuracy of the observation, we cannot reach more accurate results 
without additional means. 


§ 4. We now pass on to the description of the arrangements 
which form the subject of this communication. The uniform tempe- 
rature in the bath is obtained by stirring. The stirring apparatus 
is placed concentrically to the bath, thus leaving room in the most 
profitable way for the measuring apparatus. From this space the 
stirring apparatus (as in Comm. 27 May and June ’96 PI. III) is 
separated by a protecting cylinder §, (comp. the figure to the left of 
plate I). The upper ring ¥,, is provided with small valves y,, 
covering openings of the same form. If the stirring apparatus moves 
in the cylindrical space between §, and B, the valves shut up 


( 507 ) 


during the upward movement and open during the downward 
movement. The upward movement is brought about by means of 


the thin wires x,, the downward movement by the weight of the 


stirring apparatus itself which for this purpose is weighted with the 
heavy ring %, by means of the rods y,,. As yet a more rapid 
motion of the stirring apparatus than this method affords has not 
been required; if wanted a construction with small rods instead of 
threads would be necessary. The valves are hinged on bent pins 
Yo The complete section of the stirrer to the right of plate II 
shows the valves shut, the section of x, at the top shows them 
open. When the stirring apparatus is moved up and down and 
the bubbles of vapour escape the movements of the valves resemble 
those of the fins of fishes. 

It is very important that the up and down motion of the ring 
should be perfectly perpendicular and that the protecting cylinder 
§, and the beaker B,, should have a perfectly vertical position for, 
to make the valves work properly, only a narrow space can be left 
between the stirrer and the cylindrical walls. The cylinder §, is 
enclosed between two rings provided with grooves §, and &, of 
which the upper is connected with the ring §, by means of glass tubes. 
Through the operation of the spring §,, and the arch §,,, this ring 
is pressed against the ring §, on to which the beaker B,, with a 
ground upper rim is fastened by means of cords. To this ring §, 
the hooks §, are also fastened, against which the upper rim of 
the beaker B, is also pressed by means of cords. In this way 
a cylindrical space is reserved for the pumping motion of the 
stirrer. 

In order to admit the measuring apparatus it was advisable to 
leave free the whole space offered by tube /’,, which is equal to 
that in the bath available for a measuring apparatus. To this end 
the threads y,, formed of very thin silk cords enclosed in steel wire 
are led through 3 openings M,, in the cover // of the bath and 
then over a pulley axis,z, with three grooves to a connecting piece 
%;, Which is moved by a single thread passing over the pulleys x, 
and y,. The cord must be moved from outside the case and the 
case must remain perfectly air-tight. This is obtained by passing the 
cord through an india rubber tube 7,,, which at ,, fits hermetically 
on to the cover of the cryostat and in which the thread x,, is also 
hermetically fixed. A thin steel wire is wound spirally round the 
india rubber tube. In this way the walls of the tube offer sufficient 
resistance to the atmospheric pressure to prevent them from collapsing 
when low pressure exists in the cryostat, while at the same time 


( 508 ) 


they remain elastic enough to permit the movements of the cord. 
A regular up and down motion of the stirring apparatus is secured 
by the wheel ¥,. 


§ 5. A constant temperature is attained by continually adjusting 
the pressure, at which the liquid in the bath evaporates, to the 
indications of a resistance thermometer p placed concentrically in the 
bath. A sensitive thermometer forms an inherent part of the cryostat 
under consideration when it is to be used for very constant tempe- 
ratures and the dimensions allowing a resistance thermometer to be 
introduced, the latter has been chosen as the most trustworthy. Its 
inner diameter controls the greatest cross section ot the measuring 
apparatus which can be immersed in the bath, and therefore, as 
in our case, it must correspond to that of the tube /’,. The con- 
struction of this thermometer has been described in detail by B. Mernk 
(Comm. 77 Febr. °02) with a view to a comparison between it and 
the hydrogen thermometer referred to above. The leads pass through 
the openings B, &,, of the ebonite rings R, and A, and then 
through the stopper into the tube 7. On the plates I and IL they 
are indicated by the same letters as on the plate of Comm. 77. 

When the bath has reached the required temperature the galvano- 
meter in the Wuwarstore’s bridge, which serves to measure the 
resistance of p, is adjusted to zero by introducing suitable resistances. 
As soon as the deviations of the galvanometer make it necessary, a 
sign is given to the assistant, charged with the regulation of the pressure 
in the cryostat, who then raises or diminishes the pressure, whereby 
the temperature in the bath rises or falls. The great volume of the 
cryostat is here very useful in checking oscillations in pressure. The 
arrangements required for the regulation of pressure are shown in plate 
I, the separate pieces of apparatus to scale and the connections schema- 
tically. (Comp. Comm. 51 Sept. “99, pl. IV). The assistant uses 
the oil manometer XN, which is connected to the cryostat by X, 
and X, (comp. pl. Il Comm. 51) and the cock X,,, the cock 
X,, being open. If we shut the cock X,, the motion of the oil 
enables us to very accurately watch the variations of the pressure 
in the eryostat by means of the difference between the pressure 
in it and of the quantity of gas temporarily shut off in the reservoir 
Ns. If through some cause or other the variations of pressure 
increase considerably, or if we want to stop the regulation, or to 
proceed to another pressure, the oil is prevented from running over 
by our opening the cock X,,. The pressure in the cryostat is varied by 
more or less opening the fine cocks },, and },, of the regulation 


( 509 ) 


tube}. Two cases are to be distinguished here. With operations 
at ordinary pressure it will be sufficient to adjust the cryostat at 
a pressure a little higher than that of the atmosphere and to either 
connect the cock Y,, with a gasholder Gaz. or to disconnect them, 
as the occasion demands. As soon as the pressure passes a certain 
limit settled for the cryostat, the gas escapes from the cryostat 
through the large safety apparatus. For operations at reduced pres- 
sure, the cryostat, after the pressure has been sufficiently lowered 
by means of the exhaustpump of the circulation Mvh. 1, is discon- 
nected from the latter and connected by means of the cock Y,, to 
the exhaustpump Zeh. 2., and is then reduced to a lower pressure. 
Obviously we can sometimes avail ourselves for this latter operation 
of the same exhaustpump as used with /vh. 1. The evaporation 
will proceed more gradually when a connection is made to a reservoir 
at reduced pressure Vac., plate. If a reservoir of large volume is 
used we can even work without an exhaustpump, which may be 
ralnable when it is necessary to avoid vibration for the measure- 
ments. Thus with the bath of nitrogen under diminished pressure 
the auxiliary compressor of Comm. 54 Jan. ‘OO plate VIT was 
connected near Zeh. 1 to the gaslead and the vessel of 5 m* men- 
tioned above (comp. Comm. 14 Dec. °94 $ 10) served as vacuum 
reservoir, after being exhausted through Y,, and Y,, by means of 
a BurcKHARDT vacuumpump, connected to the gaslead at Lirh. 2. 
This vacuumpump will be described later. 

In a few words we shall indicate the method which we usually 
follow in order to get a wellfilled bath at dtminished-pressure. 
First the double beaker 2, ZB, or several beakers B,, B,, B, 
are filled at ordinary pressure, then we begin to slowly exhaust 
through Y,,; all other cocks being shut by means of the pump, 
generally used for the circulation /ivh. 1; while boiling is prevented 
by rapidly moving the stirring apparatus described in § 4. When 
the required pressure is reached the cryostat is to be connected to 
the great reservoir Vac. at the same pressure. If this cannot be done 
we hardly ever sueceed in admitting through the cock 4, the vet required 
quantity of liquid slowly enough to keep the pressure in the cryostat 
free from undesirably large fluctuations or even to avoid with the 
help of}, momentarily returning of it to nearly its ordinary value. 
Therefore, if a change of temperature for some time is allowed, it is in 
that case better to shut Y,, before more liquid is added and to connect 
the eryostat through },, to the gasholder. As long as the beaker ,, 
is not full the gas leaving the cryostat is allowed to pass through 
Y,, into the gasholder. If the beaker ,, is full, which is shown by 


02 


( 510 ) 


the rise of the level in 6,,, we onee more begin to diminish the 
pressure (17, shut, Jj, open) which process generally takes some 
time. Then more liquid is admitted as before and if necessary this 
process is repeated several times. If the beaker is sufficiently filled 
at the desired reduced pressure we begin to regulate the pressure 
with the duly exhausted vacuum reservoir as described above. 

Plate [IL shows a couple of graphical representations of the varia- 
tions of the temperature of the bath. The ordinates show the deflee- 
tions on the scale of the galvanometer in centimeters. The abscissae 
represent the time in minutes; fig. 1 relates to a measurement in 
methane at ordinary pressure; a deflection on the scale of 1 c.m. 
corresponds to about 0.009 deg. (the open space in the figure indi- 
cates a magnetic disturbance). Fig. 2 refers to oxygen at a diminished 
pressure; here a deflection on the scale of 1 ¢.m. corresponds to 
0.005 deg. They were borrowed from the measurements of Mink 
mentioned above. 

The temperature of the measurement is determined by the help 
of graphical representations, extending over the whole time of 
measurement, from which the portions reproduced on plate [II have 
been taken. For this determination the readings of the galvano- 
meter are noted down about twice every minute. By means of the 
planimeter we derive from the graphical representation obtained, the 
mean ordinate, which mean is considered as the temperature of the 
bath during the whole measurement. 


(March 25, 1903). 


H. KAMERLINGH oj/ow temperatures in the cryostat. 


PLATE I. 


Proceedings Royal 


H. KAMERLINGH ONNES. Methods and apparatus used in the Cryogenic Laboratory. III, Baths of very uniform and constant low temperatures in the cryostat. 


Proceedings Royal Acad, Amsterdam. Vol. V. 


PLATE I. 


H. KAMERLING 
and const 


Proceedings Roy 


H. KAMERLINGH ONNES. Methods and apparatus used in the Cryogenic Laboratory. II. Baths of very uniform 
and constant low temperatures in the cryostat. 
PLATE II. 


Proceedings Royal Acad. Amsterdam, Vol. V 


aa sa taal i 
1 EVA ANITA 


iy haut FA AARLAI LBP 


H. KAMERLINGH ONNES. Methods and apparatus used in the Cryogenic Laboratory. JIL. Baths of very uniform and 
constant low temperatures in the cryostat. 


PLATE III, 
3 4 
a 3 
A 2 
3 3 
® Pie ADU ey | 
| 
A 
He 45 Je 55 rr ED 4e 37 zo u 
i i 5 
i DN ji A 
bane LV 
2 \ 2 
À VE NSA ay ul \ d 
| pv i 
i 
El 25 w 35 ko 45 so 5 ca Ei 40° a zo 5 


Proceedings Royal Acad, Amsterdam. Vol. VY 


KONINKLIJKE AKADEMIE VAN WETENSCHAPPEN 
TE AMSTERDAM, 


PROCEEDINGS OF THE MEETING 


of Saturday March 28, 1903. 


OG 


(Translated from: Verslag van de gewone vergadering der Wis- en Natuurkundige 
Afdeeling van Zaterdag 28 Maart 1903, Dl. XI). 


ROTE EN TS. 


J. J. vAN LAAR: “The meltingpoint-line of Tin-Amalgams” (Communicated by Prof. H. W. 
Baxkuuis RoozeBoom), p. 511. 

A. W. Nievwenuuis: “Influence of changed conditions of life on the physical and psychical 
development of the population of Central Borneo”, p, 525. 

P. H. Scroure: “Relations between diagonals of parallelotopes”, p. 540. 

E. Conen and Tu. Strrencers: “On the atomic weight of Antimony (Communicated by Prof, 
W. H. Junius), p. 548, (with one plate). 

E. Conen and C. A. Lorry pe Bruyn: “The conductive power of hydrazine and of substances 
dissolved therein” (Communicated by Prof. C. A. Lopry pr Bruyn), p. 551. 

A. H. J. Berzer: “The velocity of transformation of tribroomphenol bromine into tetrabro- 
mophenol” (Communicated by Prof. C. A. Lopry pr Bruyn), p. 556. 

J. H. Bonnema: “Some new Under-Cambrian Erratic Blocks from the Dutch Diluvium (Com- 
municated, by Prof. J. W. Morr), p. 564. 

J. J. van Laar: “On the course of the values of 6 for hydrogen, in connection with a recent 
formula of Prof. van per Waats.” (Communicated by Prof. J. D. van per Waars), p. 573. 

W. H. Jusius: “Peculiarities and changes of Fraunnorer-lines interpreted as consequences 
of anomalous dispersion of sunlight in the corona”, p. 589. 

P. Tescn: “On the refractive index of rock-glasses” (Communicated by Prof. J. L, C. ScuROoEDER 
VAN DER Kork), p. €02, (with one plate). 

G. B. Hocenraap: “On an “Eisenrose” of the St. Gotthard”, (Communicated by Prof. J. L, C. 
SCHROEDER VAN DER Kork), p. 605. 

H. A. Lorentz: “Contributions to the theory of electrons, I. p. 608. 

H. KAMERLINGH Onnes: “Methods and apparatus used in the cryogenic Laboratory”. ITI 
feontinued) IV, V. p. 628. 

H. KAMERLINGH Onnes and H. H. Francis Hynpman: “Isotherms of diatomic gases and their 
binary mixtures. V. An accurate volumenometer and mixing apparatus”, p. 636, (with 2 plates) 


The following papers were read: 


Chemistry. — “The meltingpoimt-lne of Tin-Amalgams.”’ By 
Dr. J. J. van LAAR. (Communicated by Prof. H. W. Baxnurs 
RoozrBoom). (2Pd Communication). 


(Communicated in the meeting of January 31, 1903). 


1. In a previous communication (Proc. Dec. 1902) I showed, that 
when the molecular potential of tin in a liquid tin-amalgam is ex- 
pressed by the formula 

Proceedings Royal Acad. Amsterdam. Vol. V. 


u, = f(T) + RT log (le) + (a, 2? + Be +...), 

a very good agreement is obtained between the calculated values of 
the melting-temperatures at various values of «, and the temperatures 
observed by vaN HerEREN (compare his Dissertation), at least up till 
about 80° C. 

In a conference, 1 had since with prof. van per Waats, he called 
my attention to an expression for the correctionterm in u,, which 
may be taken as a fairly good approximation’). This expression is: 


a, x 
(1 + ra)? ; 
After he had first shown (p. 193), that the correctionterm is 
really of the order «* — this I also showed in my previous com- 


munication, but in a different manner and had observed, that (in 
the case investigated by him) the value of a, does not remain constant, 
but decreases when w increases (p. 198), he afterwards arrived at 
the said approximate expression (p. 213, 214), in agreement with 
an empirical relation of THOMSEN. 

Though Prof. van per Waats has briefly given the deduction of 
his formula, it may be useful to state once more how this expression 
can be arrived at. The matter is of great importance, because the 
same quantity u,—(u,),=0 constantly occurs in a great number of 
formulae, such as those for the lowering of the freezing-point, elevation 
of the boiling-point, alteration in vapour pressures, etc. If therefore 
this quantity is once for all accurately known, we may get a better 
insight into a great number of problems relating to binary mixtures. 


2. As the total thermodynamic potential is represented by 


c=—2 (7,/,) T (log T— 1) Se E (2, (e)) Se (n, odo | SE 


— | fre V—p r| de RTS (xn logn,); 


we obtain for the molecular potential of the component 7, : 


05 OV 
Wz == -k, T(logT-1) + edo Md] ge frd Vp | +RT+&Tlogn,. 
n 


n, On, : 


With 


1) Zeitschrift für Ph. Ch. 8, pg. 188 (1891). Also compare different passages in 
the second part of his “Continuität” on p. 43—45; 148; 152. 

Recently, Prof. van per Waats has returned to this question in his * Ternary 
Systems” (Proc. March to July 1902). He gives there a more general and accurate 
expression, wherein occur the critical temperature and pressure of the mixture 
(Compare in particular IV, p. 92—96). 


~ 


( 513 ) 
we find: 
foev = ZE nRT log (V—b) + 5 


and therefore 


=n, RT OCS, &0¥ … BsGg 
Vb. on. 4 dn, Von, 


2 f par = ar ties te 


Deducting from this: 
OE en RT a |0V 
i Dr. V—b On, 


1 


we get: 


ov gE 7" =n, ay, 2 
aa pdV — p rs = RT log (V—b)— en ‚+ 7 a, + n, a,,)- 
a 


Substituting @=n,?a,+2n,n,a,,+7,? a, for a, and the linear 
relation 6=7n,6,+n,6, for 6 in the case of two components, the 
expression for u, becomes: 


u, = — kT (log T—1) — RT (log (VB) — 1) + [ede — Tne] + 
ot Os ue 2 : 
See b, — pm Weald: LOM pres tees Miter A a, aL) 
in agreement with what I wrote down in my first communication. 
If now we write x, = l—e,n, —=w, this then becomes: 
p, = — kT (log T—1) — RT (log (V—b) — 1) + [e), — TO] + 
RT b En 
+o = [(1—a) a, + wal + BT log (1) 


For the determination of the complete function of «, which occurs 
here outside RV log (1— x), we will now determine the value of 
a 
UR V (Ae) a, + va,,]. 


The term with log (V—b) is supposed to be but very little dependent 
on # in regard to these two. If in the equation of condition we 
put p=0, which is certainly permissible in the case of liquid phases, 


r 


gi a 
z may be replaced by rr and the above expression becomes: 


then 


(l—a)? a, + 24 (1—a)a,, de a)b, 2((l—2z)a, + va,,) 
5 EER r ck 


If now we replace V by 6, which will hold for liquids at low 
temperatures in approximation, we obtain: 
35* 


( 514 ) 


((1-x)* a, + 2 a (1-a) a,, + a? a) b,— 2 (1-2) a, + # a,,)((1-#) 6, Hb.) 
ee ’ 


b? 
or: 
— a, ((l—e)° b, 4+ 2e (l—a)b.) — 2.4,, a b, + 4, a7 l 
b? 


which we may also write as 


B OO ME 
se DGN de 
b, b, 
We therefore finally and approximately obtain: 
u, = — kT (log T—1) — RT (log (V,—64,) — 1) + [(¢,).—T(n,).] — 


Bi EF Tog 
it pe + RP lg (le) 


when we call 
a, ba et) ds b, b, — a, be =A. 


The corresponding expression for uw, evidently becomes: 


i, = — kT (log T—1) — RT (log (V,—d,) — 1) le), Tad — 
ds A (1— x)? RT / 

—— ———. dD Ve 
a ee ae 


As (omitting p) it follows from the equation of condition, that 


PPV meen op! Bs 
V—b= = ; 


a a 


) 


and that, therefore, log (V‚—b,) = log 


a 
general: 
Eo mee oee Mine age (May) e 
es e) 
u, =e, — CT — (k, + B) Tlog T+ a, ce ze + RT log « 
(1 ray’ | 
In this equation then 
is Len a, 
Bm nn 
bie Rb,? 
c, = (1), — (4, + R) + R log —; C,=(4),),—(4. + 2) + BR log 
a, : 
whilst 
A ea, d A 
es Ci an RK at, 


and also 


2 
1 . mn . . 
+ log T, we may write in 


Tt SES ee ae 
OS a 


a 
7 
5 


=O} ait b, een 
b aa 


Tr. 
1 


5 
Remark. The quantity u, = 5, may also be obtained by the opera- 
n d 


1 
» 


0g 
tion p, —=$— ex De For the term — fpdV4pV, occurring in &, may 
x a 


. a 
be written — (par — RT-D The required function of x 
may therefore also be found by calculating (VV —/ 


a 3 0 a 
EE Ee de aah 


for which we then find exactly in the same way as above: 
a, , a,b,*+a,b,?—2a,,b 


re Tee 
2 
b, bb 


woe 


The two methods of calculation are, of course, identical. The last 
has the advantage, that we see at once that the differentialcoefficient 


5 ' ; 24e ‘ aly ee 
of the correctionterm of z, 1. €. ze 8 nothing but x sata ase 
Dis dd U ) 


that we have: 


Opes NORE ads OG fi Oe (+) 2A 


PLO E se eh a ees Ox?  Òx? 


when &, w, and w'’, represent the quantities ¢, uw, and gu, with omission 
of the terms containing log(1—a) and loga. As regards the quantity 


ds 


u, =~, we must remember, that this is also obtained from the relation 


Oz’ 
ijs 
U, = 5 = (1—2) aa : 


be’ 


= )= 


3. It is now the question, whether the expression 


a? 


OR ETE 
(1 4-74) 
represents the melting-points of the tin-amalgams as well as, or 
better than my semi-empirical expression 


a, 2 + Be + y, ef. 

Let us first observe, that vaN per Waars always found a, negative 
in the case of electrolytes and other aqueous solutions (l.c. p. 195). 
Now it is evident, that if we may write a,, = Va,a,, the coefficient 
(b Va,-b, Va)’ 


3 
b, 


a, becomes , and ought therefore to be always found 


( 516 ) 


positive. (Ll found for instance «, positive with tin-amalgams). It 
therefore seems, that when one of the components (water for instance) is 
an associating substance, or when the other component is electrolytically 
dissociated, we must certainly not follow D. Brrrnenor in writing 
12 Independent of the fact, that in such cases neither 
a, and a,, nor 6, and hb, are constants. 

The formule (8) in my previous communication now becomes: 


= ey 2 
a,a, — da 


hs ea? 
1+ — 5 
ae — ie Jo (14e) ; 
7 
1— log(1—«) 
Jo 
RT 
or with pee ct, ine 
Yo Yo 
14 ax 
‘1+rex)? 
Aid ne) es (SDi) 


el (LS 

From observations, where the values of « are less than 0,1, the 

value of @ was found to be exactly 0,396 *). If we now further 
accept for the values of the coefficients @ and 7: 
a = 0,0453; r= — 0,74, 


which are calculated from other observations with higher values of x, we 
obtain (1, = 273,15 + 231,63 = 504,8) the survey on the next page. 

We notice, that in this table the agreement is an excellent one; the 
average deviation is about 0,9°, whilst in the case of the empirical 
formula with ge? and y«* (see previous communication), if the last 
value is not counted, it amounted to 0.85°. vaN DER WAALS’s expression 
for the correctionterm, therefore, represents at least equally well the 
course of the meltingpoint-line over the portion, observed from 212° 
to 65°. But what is still more important, is the fact, that whilst my 
former empirical formula does not very accurately represent the two 
last observations (the difference in the last even amounted to 10°), 
VAN DER WAALS’s expression not only satisfactorily represents these, 
but also the four observations at still lower temperatures (compare 
p. 22 of van Hernren’s Dissertation). In this observations the values 
of « and ¢ were determined by analysis of the liquid phase, which 
is in equilibrium with the solid phase at a given temperature. 


200 
1) In the previous communication 0.400 was accepted, but ae = 0,396 is some- 
505 
what more accurate. 


ide 


RN re 
Denom. Numerat. |p 73045] ia. 

2 a av? Lude)? Pre) rat 

1—6 log A—2) | 1 -+- (ra desa ieh 

0.1005 |0.01019; 4.0420 |0.00045°| 0.8567 1.0005 214.6 244.6.) -O 

0.1716 (0.02945; 10745 |0.00433*| 0.7621 1.0018 197:5 {198.6 |—4.4 
0.2338 0.0546° 4.14054 |0.00247°| 0.6839 1.0036 185.2 183.7 |44.5 
0.2969 |0.0881° 1.1395  |0.003993| 0.6089 1.0066 172.8 {173.0 |—9.2 
0.3856 (0.1487 1.4980 (0.00673°| 0.5108 4.0132 155.6 155.2 |+0.4 
0.5001 0.2501 1.2745 {0.01433 | 0.3968 1.0286 134.3 |133.4 40.9 
0.5973 |0.3568 1.3602 (0.01616 | 0.3114 1.0519 1173 (415.2 |42.4 
0.6467 0.4182 1 4119 |0.01894 | 0.2719 1.0697 109.3 |107.4 1.9 
0.6754 0.4562 41.4456 {0 02067 | 0.2502 1.0826 105.0 03.4 |44.6 
0.6813 0.4642 | 1.4528 0.02103 | 0.2458 1.0856 104.0 |102.4 |+1.6 
0.7104 (0.5047 | 1.4997 0 02286 | 0.2250 1.4016 | 99.9 | 99.0 H0.9 
Oerlas: 10.5119 1.4978 0.02319 | 0.2214 1.1048 | 99 2 | 98.8 |+0.4 
0.7477 0.5591 4.5454 (0.02533 | 0.4995 1.1270 95.0 | 95.4 |—0.4 
0.7547 (0.5696 1.5565 (0.02580 | 0.1949 154320 94.4 | 940 |+0.1 
0.7963 (0. 6341 1.631 (0.02873 | 0.1687 1.41703 89.3 | 90.0 |—0.7 
0.8189 0.6706 | RGO Or 03038) 0). 1552 1.4957 86.8 | 88.4 |—1.6 
0.8921 (0.7958 158817 - 0) O8605- 120.4455 1.3491 18.9 | 79.7 |—0.8 
0.9483 0.8993 2.173! (0.04074 | 0.C8898 1.4579 65.5 | 65.2 |--9.3 

T—973.15| id. | 

L ed Denom. aa? |(1-+rz)?) Numerat. 

| | | ealeulated! found 
0.9879 |0.9759 2.7482 (0.04421 | 0.07231 1.6114 22.9 | 25.0;—2.4 
0.9903 0.9807 2.8357 (0.04443 | 0.07140| 1.6223 15.7 | 15.0+0.7 
0.9941 0.9882 3.03826 (0.04477 | 0.06991) 1.6403 sti a 0.0\—0.1 
0.9964 0.9928 | 3.2282 (0 04497 | 0.0690! 1.6516 — 14.9 —18.8 3.9 


The agreement is even unexpectedly great, when we consider, that 
the meltingpoint-line runs here almost vertical, and a quite insigni- 
ficant change in # causes a difference of several degrees in 7’, 


( 518 ) 


4. Let us examine the formula 


xv 2 
1 + 0,0453 | ——___—_ 
ik & =0,74 -) 
1—0,596 log (1—za) 


more closely. ‘With small values of x it passes into 


rr 1 + 0,0453 #° Ti BEE 
die ae ee [1—0,396 x + 0,004 #°]. 
Because the coefficient of «? is accidentally nearly O, the melting- 
point-line i this case runs over a fairly large region (from 232° to 
120°) as an almost straight line. To ensure this, it is generally necessary, 
that 6°? —40-+- a is very small or 0. 


id 1 


As, for equilibrium between the solid tin and the tin in the amal- 
gam, “=U, or 


— uhu, =0, 
we also De 
de 
eee en Ark 
. 0 A 
Now according to a well-known theorem Ui (—yu+u,)=—- 7 


The molecular potential u for the solid phase is moreover not depen- 
dent on w. Therefore: 


( Ou, de 
dz dT’ 
and consequently 
7A ee! i) Pm 
be 
We therefore see, that supposing the solid phase (as in this case) 
contains no mercury, = cannot become 0, unless ot == 0, ba 


then the liquid phase will be wnstab/e, and we find ourselves on the 
spinodal line, so that the liquid amalgam would long ago have broken 
up into two phases of different composition. 


7 


Ou 
Now, 5e and therefore also a, May become zero in the case of 
U av 


two values for «; there are therefore in this case always two hori- 
zontal tangents. A limiting case of this is of course a point of 


inflection with only one horizontal tangent. 
As 


Cote) 


Re Ae) ES 
dz* q Oz dw de \q 
this limiting case will evidently oceur when 


Ou, d'u, 
Se and 72 
are O at the same time. Now 
Ou, RP GA 4 du, RE LT Ope 
Pie de a ey et dy 


so that for this point of inflection we shall have the relations 
v(1—a) aS RT (a «x)?(1—2re) 7, BN: 
(l-Fre)? Za, ° (Lint ien Be, 
On dividing, we find : 
w (1+ re) = (le) (1—2 72), 
or 
re—2(14-rne+1=—0. 
When 7 is either negative or positive, we find from this : 
Lr VIe 


1 


Wve — 


(a) 


when «, indicates the value of vz at the point of inflection. 7, may 
cree rome. (eran — 0) tot (Of 7 = — 1), when. 7 is negate. TE 
however, 71s positwe, «a: runs from */, Gf r= 0) to 0 GE r= o), 


/2 


r NE . . OZ 5 . . . 
The positive sign for W 1 + 7+ 7° would give in both cases impos- 
sible values for «,. 

We now further obtain : 


Pikes ee RT 1 Taede me 


PEER gn ke Ty eT 


ry. 


that is to say, when for — 


rm 
0 


is substituted its value from (8hzs) : 


1 arc 
a(l—a)— 0 | tra) 
(Ll4-ra)? “2a 1—Olog(1-«,)’ 


Ou 
a 5 det 1 : 

where the lower sign indicates conditions, where — < 0, and which 
Aly 


0 


are consequently stable. From this then follows: 


Bella = , 
( re) (1 — 0 log (1—a;,)) ns OQ + ra)? Haa]. 


+7x, 


2a 


Now, from the equation, from which (a) was deduced, we find: 


( 520 ) 


l+r2,—3——_, 
+ 97 x, 5 


so that also 
9 


5 av (2 — «,)? (1 — Glog (1 — w)) Ze OLI(1 —e)? + aa? (2 — a,)’], 


consequently 
== 270(l—e,)? 


a Zi m2) [A2 —a)(1—0 log (1—2,)) ay 30ae| . (b) 


Ou 
If, therefore, @ = or > than this value, then ae becomes 0 on 
a“ 


one or two places on the meltingpoint-line. 
Al . . u - . Oo e . 
From the expression for — (see above) it follows immediately, 


Ow 
ti 
that when A, and consequently @, should be negative, re can never 


d 
become 0, still less positive. The occurrence of unstable conditions on 
the meltingpoint-line may, therefore, only be expected in the case 
of positive a, and only then, as soon as « reaches ov erceeds the 
value, given by (Od). 
The relations («) and (4), when united, give therefore the con- 
dition for stable phases along the entire meltingpoint-line. 
In our example 7 = — 0.74, and (a) gives a, = 0.863. The equa- 
tion (6) further gives with 06 = 0.396 : 
ae 27 >< 0,396 x (0,137)? 
“ < 0,863 <(1,137)"}2<1,137(1 0,396 log 0,137) 3 <0,3965<0,863] 
that is to say 
— 0,180 — 0,180 


| 0,0592. 
ETET Li a < 0,05 


Now, in our case « was 0,0453, so that everywhere we find 
ourselves in the stable region (as may in fact be seen from the 
shape of the observed meltingpoint-line). If @ had been 0,059, 
should have had a point of inflection with horizontal tangent ; and had 
a been 0,059, we should have noticed the occurrence of a horizontal 
tangent in two places of the meltingpoint-line. This last case is, of 
course, not realisable, as the liquid amalgam would break up into 
two heterogenous liquid phases of different composition. *) 


1) It is perhaps not devoid of importance to observe, that when the solid phase 
forms a solid solution of the two components, the presence in the meltingpoint- 
line of a point of inflection with a horizontal tangent points as before to unstable 
conditions. For in the general relation 


a 


Ou 
Another question is, at what values of « and 7' does — first 
U 


become 0, or where does the plait commence, independent of the 
fact whether we find ourselves on the meltingpoint-line or not, which 
had just been investigated. 


Ou Oru 
We have only to combine the relations — =O and ~— () 
wv wv 
2 
a ore 
dil fess Oa,? 
SN —_ 
da (B 
Ihe 
a always becomes O in one place only in consequence of #3—, becoming 0, 
Av 
1e dT 
whilst on account of De becoming 0, i always becomes O in {wo places, or 
ra Ak ‘ 


in the limiting case in two coinciding places in a point of inflection with a hori- 
zontal tangent. De Visser thinks he has found such a point of inflection with 
mixtures of stearic and palmitic acids.}) It is, of course, not impossible, that we 
are dealing here accidentally with a case, in which the quantity z possesses the 
value indicated by (0). That the line of the end-solidifyingpoints also shows in the 
immediate neighbourhood a similar point of inflection, points to the fact, that the 
0°6 ik 
Jet = 0, 5, Sb are fulfilled on both lines at about the same time, 
v i 

which renders it more accidental still, because z would then possess the value 
required for this also in the solid phase. It should be pointed out, that as arule 


conditions 


may ye 08 
the conditions Pe Die =0 for both phases by no means include x, = #3. For 
vu wv 4 
y = 05, : . 
this requires aa = Hee It is there‘ore a new accident, that both points of 
Ly we 


inflection appear to coincide. But for this a reason may be given here. From the 
equation, from which (a) is found, namely rx? —2(1+7r).a2-+1=0, it follows 
that with r=0, «=1/,. De Visser now found both points of inflection to be at 
x about 1/, (= 0.525), so that the quantity 7, both in the solid and liquid phase, 
is about O (bj = bz). And in that case the values of 2 at both points of inflection 
must agree, namely both at x= 1/9. 

The case, studied by pe Visser, may therefore be an accidental coincidence of 


9 9 


2 2 


07g 
= = (0 and — = 0, both 
Oe Òm,? é 


the liquid and solid phases must have broken up into two layers, although of 
identical composition. The smallest delay in solidification would however imme- 
diately have carried the system within the plait, and then both phases would have 
broken up into two layers of a somewhat differing composition. It is however 
more probable, that both lines nearly show a point of inflection with a horizontal 
tangent, and that they approach very near, but not touch each other. 


Ee, 


the two points of inflection. But then, on account of 


1) Rec. Trav. Chim. (2) T. 2, N’. 2 and 4 (1898). 


( 522 ) 


to find the values of x and 7 at the “critical” point. We find as 
above 
lt-r—V1itr4r 
ei een ieee we as. oh 


u 
a Ned: Ou, 
The temperature 7, of this critical point is found from— = 0, 
v 
that is to say from 
a(1l—a,) O Te 
Iro)? 2aT, 


We consequently find: 
2a e(l—e,) 
Ee 


rj ry 


a zl: 
IY, as TL == Eel 
i 2a #&(2—.2,)* 
Rr RL eee STE, 
27 0 (1—z2#,)° 


Ou 
At this, or at lower temperatures, a being then positive, we find 
Or 7 ' 


ourselves therefore in the plait. 
In the case of tin and mercury we find for x, the value 0,863 


(see above), if r=— 0,74. For 7, we find: 
rl. BORE MODE anar 
Ee a 


The “critical” point is therefore situated at 16° C., that is to say 
fully 57° lower than the point of the meltingpoint- ties belonging to 

= 0,863 (13,7 atom-percent tin), namely 83°,2 C. 

There are of course cases, where that distance is smaller, and 
where consequently a trifling supercooling already carries us within 
the region of the plait, which then — in the absence of the solid 
phase — causes a separation into two layers. 

I may observe, that the value z, does not correspond as a rule 
with a point of. inflection (with oblique tangent) on the meltingpoint- 
line, when the critical point is not situated on the meltingpoint-line. 


Ou, Oru ‘eP 
For de 


=—= 0 do not lead to —~ == 0, when these differen- 
DE ” Oa? dx? 


tial-coeffients do not become O on the meltingpoint-line. 


5. The value of g, the heat of fusions of tin in the liquid amal- 


gam, is evidently: 
2 
ge (: +75). 


( 523 ) 


When the value of « is small, and assuming, that mercury dissolved 
in tin is monatomic, we find for q, by calculation 2550 gram-cals. 
Person found experimentally 1690 gram-cals. Should this figure be 
confirmed, it would prove, that the associationfactor of mercury is 
about 1.5. 

Now, it follows from the above formula, that at 25°, where w is 
about 1, g ought to be 


— 2500 to bit 4110 gram-cals., 


whilst van HerEREN, by electromotive measurements, found about 
3000 gram-cals. From this it would follow, that the value, used for 
q,, is about 1.4 times too large, which would be a confirmation of 
the fact, that the mercury in the amalgam is not present as single atoms. 

In order to obtain certainty as regards the molecular condition of 
the tin in the amalgam, it would be necessary to know the melting- 
point-line of the mercury, and to determine the lowering of the 
melting-point in addition to the heat of fusion in the presence of 
very small quantities of tin. There are indeed indications, that the tin 


is also not present as single atoms. Indeed, the quantity 7 = — b, + 4,, 
; b, 

which was found by us to be — 0,74, gives for = the value 0.26, 
) 


1 
from which it would follow, that the molecular volume of tin (b,) 


would be about four times larger than that of mercury (/,). Now, 
the atomic volume of Hg is 14,7, that of Sn = 16,1, so if these tro 


b, 
components were monatomic, — ought to be approximately — 1, 


a 
whilst in reality that relation is */,; this points to the probability, 
that in the case of tin several (may be six) atoms are united to 
one molecule. 

It certainly would be highly desirable if this question were fully 
investigated. For in all our calculations the values of w are only 
then valid, when both mercury and tin are assumed to be monatomic. 
This is also the case with all similar calculations, relating to other 
amalgams. 

May I be allowed to point out, that the molecular condition of 
mercury may be determined from the lowering of the melting-point 
of tin, if this contains a Little dissolved mercury — whilst the molecular 
condition of tin may be ascertained from the lowering of the melting- 
point of mercury in the presence of a little tin. For in the case of 
dilute solutions something is learned only about the condition of the 
dissolved subsiance, but never anything as regards that of the solvent. 
In the limiting formula 


( 524 ) . 
2 
4 Al rj ETT, 
Erna WS ©, 
Jo 


where 7, and g, relate to tin as solvent for example, everything on 
the right hand side will remain unchanged, although tin should not 
be monatomic, but say z-atomie. For «, the concentration of the 
dissolved mercury, would then become j-times greater, but q, would 
also become -times greater, because the heat of fusion relates to 
1 mol. = n-atoms. On the other hand, if the mercury were m-atomic, 
the value of # alone would change; « would then become m-times 
smaller, and we shall, therefore, observe a m-times smaller lowering 
of the melting-point than that, calculated on the basis of mono-atomicity. 

In this way we might attain to the knowledge of the molecular 
condition at the ends of the curve, « being O (for mereury), and 1 
(for tin). But in order to form further conclusions with other values 
of x, the whole of the meltingpoint-line would have to be accurately 
examined, and this may in many cases become an exceedingly com- 
plicated matter. 


6. There is, however, another way to get to know something 
about the molecular condition of the solid tin, and that is the com- 
position of the so/id phase, which is in equilibrium with the liquid 
one. If we equate the molecular potentials of mercury in the two 
phases, we obtain: 

a’ (1—z2')’ 


= ln El 
cl ) == oe —c, F. +- RT log BH út ' Ne i 
re 


—c, T - RT log « - = 
C5 Cs ji wd ä (14 ra)? 2 


This further gives: 


TRT log” a,(l—2)’ _ a, (1—a)’ 
(e,—e = orn (c,—¢ ES =d are + (1 = re!) Ge (ltre)? ; 


or with e‚—e, = 4q',, and with introduction of the meltingpoint 7", of 
pure mercury : 


7 a! 
q', (1- =) = RT log — did, 
i i £ 


0 


therefore 
cae. z a, (lx)? a’, (1—a’)? 
Go| terne Feb 
T—T', 5 RT (1 + re) RT (1+ 7'2'y? 
Now in the liquid condition 
b, Diens ee ape mame Ae ee, 
Bnn he 50 RIA RTE ae ae ae T ZE 
504,8 50 


This quantity is therefore 0,1144 x 0,45. 


298,2 °° 13 


ke! RN 


Putting a, =a, and 7’ =7 as a first approximation, the value of 
the correction becomes: 


0,012 2 0,99 2 
£20,74>< 0,988) \i—0,74% zo) f 


and, as at 25° the composition of the liquid phase was found 
« = 0,988, and that of the solid phase #'== 0,01 (perhaps 0,06), the 
said value becomes: 

0,745 X (0,0020—0,9950) = — 0,74. 


A change of «' from 0,01 to 0,06 can only cause a slight alteration. 


0,745 


i igh © 
The value of the chief term log — is: 
av 


9 


BF 23026 = 4,59 
0,01 X 2,8026 = 4,59, 


so that we obtain (at 25°): 

| 2X 298,2 x 234,5 

ee 63,7 
whereas PeRSON found q' = 2,82 >_< 200,5 = 565 er. cals. We therefore 
find a value 15 times too great. And a small error in the correction 
term 0,74 cannot upset this result. If, however, the tin in the solid 
amalgam is taken as hexatomic, 2’ becomes six times greater and 
g, comes down to about 4400 gram-cals. If, moreover, +! is origi- 
nally taken not as 0,01, but as 0,06, so that with a hexa-atomicity 
x now becomes 0,32, the value g, begins indeed to get more close 
to the value, obtained experimentally. 

The above, therefore, contains indications enough of the poly- 
atomicity of both mercury and tin. To arrive at a decision, however, 
accurate experiments will have to be made in the direction indicated, 
together with fresh determinations of the two heats of fusion. 


log*® 


X 8,85 = 8450 eram-cals., 


Ethnology. — “Influence of changed conditions of life on the 
physical and psychical development of the population of Central 
Borneo.” By Dr. A. W. NreuwenguIs. 


(Communicated in the meeting of February 28, 1903). 


There is great diversity of opinion among competent authorities 
about the influence exerted by external circumstances of life on the 
development of a person and on that of the peculiarities of a tribe. 

If this difference of opinion already gives evidence of the difficulty, 
of determining this influence for the individual, the difficulty is greatly 


( 526 ) 


increased, as soon as we try to find, between two groups of men, 
characteristic differences, which are to be ascribed to their different 
circumstances of life. Examining the highly cultured nations which 
live in very complicated conditions of life, the difficulties become 
almost insuperable. 

We are not a little hampered in this investigation by the fact that 
among civilized nations mutual intercourse and mixture have a 
disturbing influence on the eventual effect of special conditions of 
existence. 

In Europe some data are furnished by the Israelites, which have 
preserved themselves as such for centuries in different countries 
under the circumstances prevailing there and which have absorbed 
few foreign elements. But here, too, the influencing conditions of 


life are very complicated, and the Israelites of the different countries 


have mixed with each other. 

Chiefly because the relations in the societies of tribes, which have 
not reached so high a degree of civilization, are simpler and the 
conditions of life for all their members do not differ so much as 
elsewhere, it is likely that amongst them eventual changes in those 
conditions of life will stand out more prominently and that much 
becomes clear to the investigator, which was difficult to point out 
under more complicate relationships. 

It is moreover noteworthy, that among them the influences of 
nature, of the surroundings in which they live, have a much greater 
effect than in higher civilized societies, which have learned to shield 
themselves better against this direct dependence. 

We also meet with tribes where the great disturbing factor of 
frequent mutual intercourse and mixture is excluded in examining 
the modifications which two tribes have suffered by different external 
causes. A still simpler case presents itself where two large groups of 
the same race have lived for a long time under different external 
circumstances and have mixed little, if at all. 

Before it has been proved that the people forming these tribes, are 
in their original qualities the same as Europeans, we must not directly 
apply what has been observed in them, to European society. For 
the right understanding of the pre-historic course of the development 
of mankind, however, we may refer to the tribes, which have 
reached as yet but a lower degree of culture; in my opinion we 
are equally justified in drawing certain conclusions as to the corre- 
sponding influences on higher cultured nations from many things, 
which we have observed in the social matters of the former. 

During my second journey through Borneo I had the privilege of 


living among two groups of the same tribe, which have existed for 
a century and longer under very different circumstances. They were 
the Bahaus on the Upper-Mahakam, with whom L lived for two 
years, and the Kenjas on the Upper-Kajan, with whom I spent some 
months. 

The tribe-groups of this name occupy together the upper- and 
middle course of all the rivers, whieh fall into the sea on the 
North coast, beginning with the river Batang-Redjang, and as far as 
the East coast, including the river Mahakam. They are called collec- 
tively the Pari-tribes, and they all consider the region containing 
the sourees of the river Kajan as their original country. Mutual 
quarrels, the result of too dense a population, were the cause, that 
for centuries again and again tribes moved away to neighbouring 


~ 


rivers, as e.g. it happened no more than 25 years ago with the tribe 
Oema Timé, which settled on the Tawang, a tributary on the left 
of the Mahakam. 

The Bahau-tribes on the Upper-Mahakam also originate from this 
native country, which they call Apo Kajan, but they have lived in 
their new home already for more than a hundred years. This was 
curiously confirmed on my arrival in Apo Kajan with my Bahau- 
escort. Their chieftain Kwing Trang then received for the first time 
a full account of the history of his ancestors, which was already 
forgotten in his own tribe. 

How little intercourse the inhabitants of the Upper-Mahakam have 
with those of the Upper-Kajan may be derived from the fact that 
among all the younger Bahaus only one man had ever been in Apo 
Kajan, and that, when in the company of 60 Bahaus and 20 pseudo- 
Malays [ set out on the expedition thither in August 1900 none of us 
knew the way. The journey lasted a month, and we had to traverse 
uninhabitated land. The way was indicated by sticks put up in 
a special way in the river-mouths by some Kenjas who travelled in 
boats in front of us, the sticks denoting which rivers we had to take. 

We may therefore assume as certain that we have to deal with 
tribes of the same origin, to which moreover their language, dress, 
morals and customs point, which distinguish them clearly from other 
tribes, e.g. from those on the Barito- and Lower-Batang Redjang. 
Their descending from Apo Kajan to the Upper-Mahakam, however, 
brought the Bahaus in peculiar conditions, which exercised a great 
influence on them. On the Upper-Mahakam, namely, the Bahaus 
live at a height of from 250 to 200 metres, the Apo Kajan is 600 
metres and higher. That this difference as regards the climate is 
very considerable especially in Borneo, may be derived from the 

56 

Proceedings Royal Acad. Amsterdam, Vol. V, 


( 528 ) 


fact that in Java the region of moss vegetation does not begin lower 
than at a height of 2500 metres, whereas in Borneo it begins 
at a height of a thousand metres. This is caused by the following 
circumstances. 

The situation of Borneo being under the equator, the middle region 
is but slightly affected by the influence of the trade-winds, which 
e.g. in Java make the difference between the wet- and the dry- 
monsoon so great. Hence it may happen that more rain falls from 
Deeember to March than from May to October, but particularly in 
the highlands really dry times are unknown, and we may find low 
water in the rivers in the rainy period. The regular distribution of 
moisture through the whole year is greatly furthered by the circum- 
stance that the whole island is covered with one large primitive 
forest, which itself retains large quantities of water, and harbours 
mouldering rocks which do the same. The annual rainfall amounting 
from 3000 to 5000 m.m. at different places, the climate is very 
humid all through the year, and the sky is always more or less 
overcast, so that a cloudless sky is a great rarity in the higher 
regions. Soon after sunset a low hanging curtain of clouds is formed 
in the valleys. This does not rise until seven o’clock in the morning 
or later and envelops the summits of the mountains till pretty late 
in the evening. In consequence of this the maximum temperature at 
a height of 250 metres is 30°C. in the shade on the Upper-Mahakam; 
at six o'clock in the morning however it was never lower than 
20° C. Noteworthy is also that strong winds of long duration do 
not occur there, only some blasts of short duration, which are generally 
preceded by heavy showers. 

The climate of Apo Kajan and of the Mahakam differs but little 
in most of its peculiarities, such as humidity, and a cloudy sky, but 
the latter is a good deal colder on account of the greater height, 
and what is particularly striking is the continually prevailing wind. 
This accounts for the fact that though in two months [ never found 
a lower temperature than 17° C. at six o'clock a.m. and though it 
hailed but once, the climate is yet much rougher. The red cheeks, 
specially of the women and children prove this, and also the faet, 
that the different kinds of rice require a month longer to ripen in 
Apo Kajan than on the Mahakam. Yet the method of growing rice 
is the same, and consists in cutting down and drying the wood, 
after which it is burned and the rice sowed in holes, which are made 
by pushing pointed sticks into the soil, which is covered with ashes. 

The geological formation is the same in Apo Kajan as on the 
Upper-Mahakam; we find in both a strongly denuded upland, where 


( 529 ) 


everywhere old slate layers come to the surface. Only here and there 
younger formations, specially free-stone, cover the older. 

If we now take into consideration that only in the last 30 years 
either the Bahaus on the Upper-Mahakam or the Kenjas on the 
Upper-Kajan have come into such close contact with higher civilized 
nations that it induced some of their men to undertake commercial 
enterprises for the purchasing of salt and linen, I think that Tam justified 
in asserting that the two groups of tribes under consideration belong 
to the same race, that they have lived for upwards of a hundred 
years in countries with a different climate, that they have had but 
little mutual intercourse and have not mixed; that they have not 
changed their life as cultivators of the soil and have developed 
without external influences. 

What effect this difference of climate can have on the popu- 
lation, may be derived from the fact, that in my opinion the thin- 
ness of the population in Borneo depends in the first place on the 
influences of the climate, and much more on the customs of the 
people than on the infectious diseases, such as cholera, smallpox, which 
are introduced from the coast. As both Upper-Kajan and Upper- 
Mahakam are so difficult to reach that infectious diseases but very 
seldom extend to them, we have, when trying to determine what 
the result of those changed conditions of life is for the Bahaus, only 
to deal with those factors which are sometimes comprised under the 
name of influences of the climate. 

What is understood by influences of the climate in the highlands 
of Borneo became clear to me for the first time in the sultanate 
of Sambas on the West coast of the island, where I was struck 
by the difference in the spread of malaria among the population 


of the marshy coast regions and that of the highlands. In order to 


— 


get a fuller knowledge of this difference, L made an inquiry into 
the traces of malaria infection on about 8000 children, both in the 
marshy alluvial plain and in the highlands. These children had not 
been offered to me on purpose for this investigation, but for an inquiry 
into the results of the vaccination among the Malay and Dajak 
population. 

Among the population of the alluvial plains IT found among 2103 
children only 6 with a chronic hard splenic tumor, or 2,8 per 1000. 

Among 420 children of the uplands it occurred in 403 children, 
or 959.5 per 1000. 

The remaining 996 children originated from regions, which in 
their formation were the transition between the alluvial plains and 
the uplands, Janus, Deuxieme Année 1898, 


36% 


This inquiry yielded the result, that in the marshy alluvial plains 
which consist entirely of vegetable and animal remains, malaria 
hardly ever occurs, as opposed to the uplands where nearly all 
children suffer from chronic malaria-infection. At the same time | 
saw, that soon after birth the hardened and enlarged milt makes its 
appearance, for it was long before 1 could find a Dajak child of three 
weeks old, whose milt was not to be felt. 

It is impossible to give the morbidity and the mortality caused by 
the malaria-infection among the population of the uplands in figures. 
[ only found the death-rate in Sambas extending over 6 normal vears, 
i.e. years without cholera or smallpox, to be for Dajaks 37 per 1000, 
for Malays 28 per 1000, which however does not represent the influence 
of the malaria, because there are also some Malays who live in the 
uplands and among those, who have chiefly settled in the lower plains, 
diseases of the digestive organs are much more frequent than among 
the hills. 

In order to appreciate fully the influence of the malaria-infeetion 
on the existence of the inhabitants of the higher regions, we must 
dwell for a moment on the phenomenon, which prof. Koc says that 
he observed in New-Guinea, namely, that the native, who went 
through the malaria-process independently i.e. without any aid except 
his constitution, became immune against it. Many are the refutations 
adduced against this statement by physicians, who practised in New- 
Guinea. They all pointed out how frequently also adult Papoeas 
suffered from malaria. 

Judging by my experiences among the Dajaks, the truth lies between 
the two. I also have been struck by the fact that not so many hard 
enlarged milts as symptoms of the malaria-infection are met with 
among adult Dajaks as among children under the age of ten, which 
certainly points to a less strong influence of this infection. Moreover 
there is a great difference between the action of chinine on Dajaks 
and on Europeans, who are not immune. Though we must make 
allowances for other factors than immunity, vet it is remarkable, 
that we obtained much greater results with at most 1 gram sulphas 
chinini a day among the Dajaks than with 2 to 3 gr. murias chinini 
among European soldiers, seized by malaria in Lombok. 

Among the former it was possible to cure not only the acute cases 
of malaria, but also cases which had continued from 4 to 6 months 
and had not been treated before, by administering 1 gram sulphas 
ehinini per day and per dose during 8 days, whereas in the first four 
months after the war in Lombok in a mixed garrison of 1500 men 
more than 500 Europeans had to be removed, most of them by far 


( 501 ) 


being malaria patients, whom | myself had treated with from 2 to 
3 grams per day and per dose, and who had little chance of being 
cured in Lombok itself. 

Among at the least 2000 Dajak malaria patients, whom 1 treated 
specially in Central-Borneo and of whom hardly any died, [ observed 
another telling difference between the reaction of their body against 
the malaria-infection and that of the Europeans. 

Whereas under unfavourable circumstances many of the latter 
perished under rabid and strong symptoms, sometimes so quickly, that 
chinine was of no avail, such acute cases with strone icterus, uncon- 
sciousness and collapse were never found among the Dajaks. | saw, 
however, many cases where the disease had reached an advanced 
stage after protracted illness. 

That this difference was not due to the inferior strength of the 
infection in Borneo, was proved by -my European and native 
fellow-travellers, most of whom suffered badly from malaria; to them 
IT had again to administer from 2 to 3 grams of murias chinini a 
day, and one of them I had to give a strong hypodermic injection 
of 3,25 gram chinine within 96 hours. 

From all this we may assume that the Dajaks become partially 
immune if in youth they are subjected to repeated attacks of malaria. 
Yet even then whatever weakens the constitution may give rise to 
attacks of malaria, so that diseases of the respiratory organs or of 
the digestive organs, wounds, diseases of infection and specially 
evervthing that is comprised under the name of catching cold, get 
complicated with malaria. 

As the mountainous regions on the Upper-Mahakam are among 
those where malaria is of very frequent occurrence, it is clear, that 
the Bahau-population suffer greatly from it and that the individual 
experiences its enfeebling influence from early youth till death. 

Being used for vears in my practice among them to find that 
the great majority of cases were those of malaria, I was greatly 
struck by the change after my arrival among the Kenja population 
of Apo Kajan. L must add that my reputation as a physician 
procured me immediately after my arrival a great number of patients, 
though only few had ever seen a European on the coast before. 

It first struck me, that so many hvdropie old people called in my 
help, which had searcely ever occurred in lower regions, whereas 
the malaria-cases retired to the background and during my stay 
confined themselves to a few acute cases. found then, that the 
change in the siek-rate of the population was chiefly due to the 
prevalence of bronchitis with emphysema and heart-disease, bronchitis 


( 9320) 


being caused by the rough climate and inereased by the smoking 
of badly prepared tobacco, which even very young children begin 
and which is held to be a remedy against coughing. 

Though more acute malaria cases occurred, when the rough, cold 
weather set in with violent showers, there was not any question 
of a chronic infection of the population, manifesting itself in an 
enlarged, hardened milt in the children. This agrees with the well- 
known fact, that in a rougher colder climate malaria generally 
decreases in violence. 

As bronchitis and its consequences do not make their enfeebling 
influence felt on the constitution before a more mature age is reached 
and are not to be compared in this respeet with strong malaria- 
infection, 1 believe to have found the chief factor of the present 
difference of the two groups of the same tribe as to their consti- 
tution and their character in the difference of the occurrence of malaria 
as a consequence of the difference in height of the country of the 
Bahaus and that of the Kenjas. 

Moreover IT must take into account that syphilis is found ina less 
violent degree among the Kenjas than among the Bahaus. Among 
some Bahau tribes it was so universal, that 1 thought the fact 
that only tertiary forms were found could be explained by assuming 
exclusively hereditary transmission. Among the Kenjas, however, 
syphilis was also met with only in that form, but the cases were 
so isolated that we could not possibly ascribe them to hereditary in- 
fluences. The eases observed seemed to have a less injurious influence 
on the general condition of the Kenjas than on that of the Bahaus. 
That this endemic form = of syphilis is so much less common and 
that its symptoms are so much less dangerous among the Kenjas 
than among the Bahaus is due to a great extent to their stronger 
constitution. 

If we now take into consideration, that among all these tribes 
every family, even that of the chiefs is dependent for its daily 
food and = sustenance on the continual labour of all its members, 
Which is not the case in more highly civilized societies, we feel, how 
great the influence must be which the more or less frequent oecur- 
rence of these diseases must have on the prosperity of the tribe. 

A striking example of the better conditions of existence offered by 
Apo Kajan which is of equal extent to the Upper-Mahakam, com- 
pared with the lower river-basins, is furnished by the fact that for 
centuries many tribes have been leaving this country for other parts 
of the world and that nevertheless the population there is at present 
much denser than in other Dajak regions. 


( dda) 


Instead of 300 to 800 inhabitants as on the Upper-Mahakam, the 
villages count there 1500——2500 inhabitants, though they certainly 
do not le farther apart. Moreover the general appearance of the 
Kenjas makes a much better impression because of their stronger 
build and the less frequent occurrence of deforming diseases among 
the scantily dressed figures, which is enhanced by the absence of the 
cacheetie persons so numerous elsewhere. 

The difference between the Bahaus and the Kenjas is even more 
marked in their psychical qualities than in their physical indivi- 
duality. The enfeebling moments which on the Mahakam affect 
them in a so much larger degree seem to have had a strong 
degenerating effect on the psyche of the Bahaus. 

This is proved by their history: in the beginning of the 19% cen- 
tury they made themselves known not only by head hunting but 
also by raids undertaken on a larger scale till far into the river-basin 
of the Kapoewas, the Barito and the Mahakam, in which regions no tribe 
could resist them; at present smaller forays rarely occur, larger expe- 
ditions are quite out of the question and in a fight with other tribes 
the wounding or death of one man may put his tribe to flight. 

The greatest difficulties which confronted the European stranger 
in his intercourse with the Bahaus, arose in his continual struggle 
with their timidity, fear and suspicion even after a long intercourse 
and in the fact that his movements were continually hampered by 
the peculiar religious and other convictions of these tribes. The 
strong contrast in these respects between them and the Kenjas is 
therefore very striking. 

After my arrival in Apo Kajan | was at once struck by the fact, 
that the 150 men, who had come under their principal chieftain to 
assist me by bringing boats and improving roads, were much freer 
and noisier in their behaviour than my Bahau escort, that the chief- 
tains gave their commands with much greater energy and that they 
were also better obeyed. During my stay in their villages this 
impression was greatly strengthened by the want of shyness on the 
part of the women and children. Remarkable was the contrast 
between the behaviour of the young Kenjas and the Bahaus when 
I, as | usually did, distributed small presents, such as beads, finger- 
rings, needles and pieces of cloth among them. Among the Bahaus 
I could quietly keep in my chair, and though occasionally a little 
hand may have been stretched out too quickly towards the coveted 
object, yet all the little ones waited patiently for their turn and 
never became boisterous. When I distributed things among the Bahaus, 
the proceedings were quite different: [ had to begin with taking a 


firm footing, for boys and girls pressed in upon me with loud shouts 
and extended hands; every one was afraid to be behind hand and 
they scuffled among each other, to get nearer. It soon proved that 
they are less sensible to the bad smells of their fellow-men than the 
Bahaus among whom one can sit for hours with impunity even 
in large companies; therefore they also prefer to go a long way 
round rather than pass a dead body, and who protest to a disagree- 
able smell by violent gestures and spitting. 

Remarkable also is the greater perseverance of the Kenjas at 
labour, which 1 specially observed when making long expeditions 
in rowing-boats on the Mahakam in the great heat to which they 
were not used. Though they are more used to walking than to rowing 
in their highlands, where the roads are better and the rivers smaller 
than in the country of the Bahaus, vet they kept on rowing for days 
together much more persistently than the latter, and always arrived 
earlier. 

These few examples already give evidence of a greater vivacity, 
less sensibility and also of a greater power of resistance of the ner- 
vous system; moreover their mental capacities are far superior. 

When telling the Bahaus about some remarkable features of our 
society, [1 got accustomed to meet with an absolute incapacity to 
imagine these things, which gave rise to disbelief, and induced them, 
but often after a long interval, to try and catch me at an untruth. 
Among the Kenjas, however, [ soon concluded from their questions, 
that they at least tried to imagine railroads and similar inventions, 
and that they really understood other things. A very good criterion 
is furnished by the explanation of the motion of the sun, the earth 
and the stars with the origin of might and day, and the causes of a 
solar- and lunar eclipse. Of course the Kenjas also did not immedi- 
ately believe that the earth is round and moves, nor that it is not 
a monster that eats sun and moon in case of an eclipse, but they 
understood at least my explanation. 

Of practical use to us was the greater interest and the more 
extensive knowledge of their surroundings shown by the Kenjas. 

In the course of our topographical survey of the Mahakam and 
When inquiring into the names of the principal mountains and rivers 
we met among the Bahaus with such utter ignorance, that we were 
for a long time convinced they were unwilling to tell them to us. It 
proved however later on, that it was not unwillingness on their part, 
but that only few among them knew anything about rivers and moun- 
tains outside their immediate neighbourhood, and that e.g. high 
mountains, Which, though they stood at some distance on the territory 


of another tribe, but commanded the landscape, had no name among 
them, and that in order to find out its name, we had to apply to 
tribes living nearer the mountain. It was, of course, quite out of the 
question to avail ourselves of their help in determining the different 
places from such a mountain top. 

I was therefore greatly struck, when among the Kénjas I ascended 
a mountain, for the purpose of getting a survey of their country 
and Boei Djalong, the chief of the country, who accompanied me 
pointed out all the mountains as far as the horizon with their names, 
also those we could verify in the Mahakam territory; he also 
indicated the roads leading to the different adjoining countries as 
accurately as a European could have done. 

Not only we, but also the Bahaus who accompanied me, were 
astonished at the knowledge of the history of times long past, which the 
Kenjas displayed. It is a wellknown fact that tribes, who cannot write 
and who possess a low degree of civilization, lose quickly the memory 
of past events, and the knowledge of the Bahaus about their ances- 
tors was therefore very inaccurate. Great was therefore the asto- 
nishment of Kwing Trang, when the Kenjas told him the traditions 
of his own ancestors during the time of their stay in Apo Kajan. 

This greater development of their psyche keeps pace with pheno- 
mena, which evidence a stronger personality as regards their sur- 
roundings. They are braver, which appears clearly from their 
way of conducting warfare. The tribes in Borneo are notorious 
on account of their headhunting, a method of taking revenge and of 
fighting, which is justly looked upon as being rather cunning and 
cowardly than brave, as it consists in the laying of ambushes and the 
sudden attack of superior forces on but a few individuals. An open fight 
is rare among the Bahaus, and as has been said before, if two tribes 
are confronted, the death or wounding of one man suffices to put 
his party to flight. Quite different is the warfare among the 
Kenjas: hand-to-hand fights are frequent, in which chiefly the 
sword is used, and in which many are killed before the battle is 


‘decided. Though headhunting occurs also among them, yet it recedes 


more into the background, and when it occurs more personal 
valour is displayed. A few years ago e.g. a young Kenja chieftain, 
when performing a war-dance during a visit on the Mahakam, sud- 
denly cut off the head of one of the spectators, and took it with 
him in his flight. This was certainly treacherous, but it requires courage 
to do such a thing in a large gallery with a great many lookers-on. 

It is irritating to see, how the Bahaus submit to be illtreated by 
the Malays, who live at their expense by deceit, theft and grave- 


(199064) 


robbery ete. Only rarily do they take revenge on these unwelcome 
guests, who live among them either because they gather the forest 
products, or because they had to fly from the coasts on account of 
crimes. ‘ 

The Kenja-tribes are less long-suffering: two gangs of Malays, one 
consisting of five members from the Mahakam and one of eight from 
Sérawak, who tried to live upon them in a similar way, were all 
murdered. 

As soon as we come in contact with the Kenjas, this bold perso- 
nality impresses us favourably. Among the Bahaus we could not 
establish for years the frankness of intercourse between them and 
ourselves, which was brought about with the Kenjas in as many 
months. Only incidentally and by indirect means could I get to know 
among the Bahaus what they thought of a plan and what they 
intended to do. When alone with one of them I occasionally suc- 
ceeded in getting him to express his thoughts freely, because he 
had no reason to be afraid of his fellow tribes-men, but they never 
quite relinquished their fear and distrust. 

In our intercourse with the Kénjas the last trace of suspicion had 
soon vanished, and never shall I forget the impression made by their 
political meetings on us Europeans, used to the uncertain, hesitating 
and insincere behaviour of the Bahaus, even when discussing affairs 
of great importance. In the meeting of the Kenjas all the chiefs 
present freely expressed their opinions with peculiar ceremonies on 
subjects as e.g. whether it was advisable to adhere to the rajah of 
Serawak or to the Dutch-Indian government, and the advantages and 
disadvantages were openly discussed. 

If on account of these peculiar qualities the behaviour of the Kenjas 
is noisier, coarser, braver and less sensitive than that of the Bahaus, 
it is interesting to see what influence this has had on their society. 
Among the Bahaus on the Mahakam we find a number of perfectly 
unconnected tribes, in which every individual considers himself quite 
independent of all the others, and perfectly free to look upon his 
own interest as of chief importance, which renders the chiefs powerless 
to exert any influence over their subjects for more general interests 
and enterprises. Everybody entertains the greatest fear for unexpected 
sudden attacks from far or near, and while in the day-time the men 
always go to their rice-fields strongly armed, in the evening they 
dare not even be under their houses without a naked sword. Of 
course women and children are still more afraid. 

Among the Kénjas, on the contrary, we find a somewhat loosely 
constructed, but yet connected whole of all the tribes under the 


acknowledged supremacy of the tribe of the Oemo Tow and its chief 
Boet Djalong. The country is so safe, that the population goes to the 
fields only armed with a light spear as support, and that women 
unarmed and unaccompanied dared to come and visit me from neigh- 
bouring settlements at many hours’ distance through the primitive 
forest or in boats. 

In this better regulated society the higher moral qualities of the 
Kénjas also stood out to advantage. If among the Bahaus the want of 
interest in the public welfare was strongly felt, among the Kenjas 
this was different. In the character of the Kenja chiefs a sense of 
responsibility and disinterestedness came to the front accompanied 
With more moral courage and influence on their subjects. When 
questions arose as to wages, the payment of which always consisted 
in goods chosen by the party concerned, the Bahau chiefs always 
retired for fear of quarrels with their people. Among the Kénjas 
the chiefs calculated, how much was due to each of their people, 
took it home and distributed it there. 

When it had been resolved in the political meetings, that repre- 
sentatives of several tribes should go with me to the Mahakam, hundreds 
of Kenjas prepared to go. Bad omens for the journey, however, caused 
more than 400 to draw back, and though the principal chiefs might 
have done so too, they only sent back their followers and went on 
themselves, because they felt the great importance of carrying on 
the negotiations. 

Among the Bahaus no chief would easily have gone to look after 
the general interests, and certainly not against bad omens. 

Also the conduct of their inferiors during the journey was quite 
different. Eighty Kenjas succeeded in deriving the required favourable 
omens from the flight of birds, the eries of does and the appearance 
of certain snakes, and accompanied us. Though from different villages, 
they formed one company, having their victuals in common, and when 
the Bahaus and ourselves had not enough they shared their stock 
with us, which was then soon exhausted. They had, however, full 
confidence in my assurance that L would buy them fresh provisions 
on the Mahakam. 

The different groups in a Bahau escort never voluntarily share 
their rice with each other, and when I and my Malays were in 
want of rice on the journey, we could only get some from them 
at very high prices. At last a young man had the assurance to ask 
me three times that exorbitant price for his rice, though as a physician 
[ had saved his life, and had treated all of them without asking 
any reward. 


( 538 ) 


In spite of the great advantages, which the Bahaus derived from 
our stay, L never met with any direct proofs of gratitude; they only 
put somewhat greater confidence in me than in other strangers. When 
however | left a Kénja tribe after a six days’ stay, the family of the chief 
came personally to thank me for everything | had given to them 
either by way of exchange, presents or medicine ; the first expres- 
sion of gratitude for many years. 

All this proves that the Kenjas of Apo Kajan are far superior to the 
Bahaus also as regards those traits of character, which are considered as 
higher ones among Europeans. 

Another striking example of their stronger personality is furnished 
by the way, in which thei religious ideas influence their existence. 

From their standpoint as agricultural tribes of fairly low deve- 
lopment, with whom the influence of nature on their principal 
means of subsistence, agriculture, and on their persons in diseases 
and disasters is strongly felt, these peoples contemplate their surroundings 
with ereat fear. Their thoughts about these surroundings and the 
place they occupy in them, which represent their religious conviction, 
are not of a very elevated nature. 

They think that their lives are ruled by one chief god, whom they 
call Tamei Tingei, our high father, and who punishes already on 
earth all crimes with adversity, disaster, disease and death. For the 
execution of his will he makes use of a host of evil spirits, who 
people all nature around. 

All calamities and diseases, therefore, even death on the battlefield or 
at a confinement, are to these tribes the manifestations of anger of their 
chief god with regard to the sufferer, who has incurred this anger by 
the conscious or unconscious violation of human usages or divine laws. 

When the attempts, to guard themselves against the manifestations 
of the anger of their god by observing these laws and usages scrupulously, 
proved fruitless, they tried to reach their aim by extending the prescribed 
laws to the minutest details, so that they have definite precepts as to 
the course to be followed not only in all emergencies of every day 
life, but also in agriculture, the chase and fishery. 

All these precepts are called pémali, and they render certain actions 
in certain cases lali, pantang or taboe. 

If the observation of the pemali is to shield them from the evil 
spirits, they enjoy the assistance of a whole multitude of good spirits, 
indirectly through the mediation of the priests and priestesses or directly 
by warning omens, which are communicated by certain birds, snakes 
and does, and also by certain events. These omens are very numerous, 
and are strictly followed, especially by the Bahaus. 


( 539 ) 

As hawever these pemali and omens have risen, independent of 
the true requirements of the existence of these tribes, they have 
constantly a disturbing influence. To give an example: the Bahaus, 
when growing rice, do not regulate their work according to dry or 
wet weather, or to the condition of their fields, but all the families of 
a tribe have to conform to what the chieftain does, and he sees that 
the necessary religious rites before the special successive agricul- 
tural proceedings are duly performed. When the preliminary rites 
for the sowing have commenced, no one is any longer allowed to 
burn dead wood on his field; if the chief is weeding, every one must 
cease his sowing, ete. 

In the same way they begin all important enterprises, such as 
travelling, the building of a house, ete. not according to the demands 
of the moment, but according to whether a bird flies up to the right 
or to the left, and whether a doe is heard or not. 

Of course, stronger races do not so meekly submit to the galling 
restraints of these pemali and omens, as more timid natures. Thad an 
opportunity of observing this as a characteristic difference between 
Bahaus and Kenjas. It is true that both have the same religion and 
that their pemali and omens are essentially the same, but the pemali 
are more developed among the Bahaus and go more into details, than 
among the Kenjas. Among the former all the adults in a tribe are obliged 
to observe the pemali closely; among the Kenjas the priests are specially 
charged with this, so that the mass of the people have more liberty. 

Among the Bahaus e.g. nobody eats the flesh of the stag; among 
the Kenjas the priests only do not take it. 

The Kenjas have not introduced the above-mentioned very injurious 
precepts for the growth of rice with the same restrictions. It is true 
that also among them the chief causes the necessary ceremonies to be 
performed, but still, every one is free afterwards to do in his field, 
what will prove necessary, and this is of the greatest importance for 
the success of the harvest. 

The Bahaus cling much more scrupulously to the existing pemali 
and omens than the Kénjas. In spite of my having lived for years 
among the Bahaus, I was forced, to observe their precepts as serupu- 
lously as they themselves did. Only in case of urgent necessity [dared set 
out on a journey or receive a patient during the time prohibited by their 
laws, and I was therefore as much shut out from the outer world 
as they were. Once they made the inhabitants of their own village 
on their return from an eight months’ expedition remain in the forest, 
starving, rather than violate the lali of their village by admitting 
them or bringing them provisions, 


( 540 ) 


When L arrived with my companions among the Kénjas, the prin- 
cipal chief and his family happened to be in the condition of lali, 
but in order to be able to receive us he quickly had a new house 
built in another. place for the priest family in his house, who were 
the principal bearers of the pemali. By this means it was permis- 
sible for him to receive us in his house. 

Later on we proceeded to another village, where the house of the 
principal chieftain was also lali, For our reception he divided his 
house, which was very long, into two parts by means of a gate, 
so that we strangers could not enter the one part. In the other he 
received us. 

The Kenjas watch the omens before every enterprise as earnestly 
as the Bahaus, but as soon as they are in conflict with the require- 
ments of the moment, they dare take their own course to a much 
greater extent. 

I have already mentioned that the Kenja chiefs ventured to 
accompany me to the Mahakam in spite of the bad omens of their 
birds. 

In case of imminent danger, e.g. if an enemy is thought to be 
hidden in the neighbourhood, the Kenjas disregard omens. 


So we see among the Bahaus the more serupulous observance of a 
more developed system of religious usages keep pace with the deterio- 
ration of many of their physical and psychical qualities. In these the 
Bahau is inferior to the Kenja, which can originally not have been the 
case, but which is owing to the change of abode of the Bahaus more 
than a hundred years ago, because through this change they were 
exposed to the more injurious influences of their new surroundings, 
the principal of which is a greater prevalence of malaria. 


Mathematics. — Prof. P. H. Scnourr discusses : “ Pe/ations between 
diagonals of parallelotopes” with a view to show by a simple example 
how it is possible that investigations of more-dimensional figures lead 
to new theorems on figures of our ‘hree-dimensional space. This 
example relates, as the title indicates, to those figures which continue 
in the spaces with more than three dimensions the well-known series 


of line-segment, parallelogram, parallelepipedon .... and can there- 
fore be called by the name of parallelotopes. Here diagonal always 
denotes a line connecting — across the inner part of the enclosed 
space — two opposite vertices. /’rsf our attention may be drawn 


fo the fact that the number of diagonals of the parallelotope is doubled 


line-segment, parallelogram, parallelepipedon,. .. 
wigs L. 

every time a new dimension is added, whilst the number of constants 
determining the figure, though at first larger than the number of 
diagonals, increases less strongly than the latter; this is illustrated by 
the following little table, where under each other the corresponding 
values of the number of the dimensions, the number dof the dia- 
gonals and the number y of the determining constants are indicated, 
whilst the meaning of A is explained further on. 


na nale om (ele Oe a |” LO |t me 

d\|2)4| 8 |16/32|64/ 128 | 256/512}... . 221 

gela le ol15|21/28| 36) 45 | 55 |... . Anni) 
es 6149) 99° 1919 | 466 | WEEER @ 1) 


From this is evident in the second place that when constructing 
parallelogram and parallelepipedon all diagonals can be used as 
determining lines, but that this is not possible for the parallelotope 
P, with five and for the following parallelotopes ?,, P?,... with 
still more dimensions; and from this ensues in the third place, what 
becomes the principal thing here, that between the 16 diagonals of 
P, at least one relation must exist and that this number of relations 
for P,, P,.... must increase consecutively to 32—21 or 11, 64—28 
or 36,... If in the fourth place we wish to trace those relations 
and try to do so under the condition that the length ofall the edges 
must figure amongst the determining data, then we find that the 
sum of the squares of all the diagonals — always equal to the sum of 
the squares of all the edges — is known at the same time, and that 
the other relations, between the diagonals only, always present them- 
selves in the form of homogeneous equations, the number / of which 
is indicated above. This includes that already for the parallelotope 
P, we come across a relation between the diagonals. This simple 
relation can be expressed as follows: If we divide (lig. 2) the eight 
vertices of one of the eight parallelepipeda forming the boundary of 


Kd 


the four-dimensional figure into two groups (4,, A,, A,, A,) and 
(B. B, B. B) of non-adjacent vertices, the sum of the squares of the 
diagonals terminating in the four points .f is equal to the sum of 
the squares of the four remaining ones, terminating in the points £. 
And from this ensues, the common centre of the eight diagonals being 
indicated by O, the equation 


OA,’ ali OA, Ei OA,” a OA? 5 Ob + OB,? a OB, ai ob, 


or in words: If we divide the eight angular points of a parallelepipedon 
into two groups of four non-adjacent points, the sum of the squares 


of the distances from an arbitrary point © to the points of each of 


Fig. 3. 


the two quadruples is the same. Tf we now suppose in the fifth place 
that this point © lies with the parallelepipedon in the same three- 
dimensional space, our space I may say, we finally find the following 
theorem belonging to our solid geometry : 

“If we connect (Fig. 3) an arbitrary point O of space with the 
two quadruples of non-adjacent vertices of a parallelepipedon, we 
obtain two quadruples of line-segments for which the sum of the 
squares has the same value.” 

This simple theorem which up till now TI never came across in 
any handbook is of course easily proved; we have but to know the 
formula for the median line in a triangle. With the help of this 
formula we find that, disregarding quantities not depending on the 
place of 0, the sum of O A,* and OA,’ can be replaced by two 
times O C°,, the sum of O A,’ and A O,? by two times OC;, and 


El > 


twice the sum of OC), and OC), by four times OM from which 


is evident that for the two sums named in the theorem, disregarding 
the same quantities not depending on QO, the same value is found, 
namely four times OM, ete, 


Ad 


( 045 


Finally this observation: it is not our purpose to emphasize even 
in the slightest degree the above-mentioned theorem, up till now acci- 
dentally remained unnoticed. Neither have we in view to point out 
that for each parallelotope 7, the diagonals and the sides furnish 
equal sums of squares and that all possible relations between dia- 
gonals mutually can be represented in the above mentioned form. 
Whilst referring for this to a paper, to appear shortly in the “Archives 
Teyler”, we repeat here, that this short communication was given to 
satisfy the wish to show also to non-professional mathematicians by 
means of a simple example how the study of polydimensional geo- 
metry may lead ta. to the discovery of new theorems of plane or 
solid geometry. 


Chemistry. — “On the atomic weight of Antimony.’ By Prof. 
Ernst Conrn and Mr. Tu. SrRENGERS. (Communicated by Prof, 
Well eJuLmws). 


(CGommunicated in the meeting of February 28, 1903.) 


I. In connection with a physico-chemical study on the nature 
of so-called evplosive antimony conducted by one of us (C.) conjointly 
with Dr. W. E. Rixeer, the question of the exact atomic weight of 
antimony became a very important one. 

Notwithstanding a number of investigators ') have attempted to 
determine this atomic weight, it is not as yet known with sufficient 
certainty. 

CLARKE”) sums up his criticism on the determinations made up 
to the present with these words: “..... This result, therefore, should 
be adopted until new determinations of a more conclusive nature, 
have been made.” 


1) Berzeuvs, Poaeenp. Annalen 8, | (1826); Kessrer, ibid. 95, 215 (1855); 
SCHNEIDER, ibid. 98, 293 (1856); Rose und Weser, 98, 455 (1856); Dexrer, ibid. 
100, 363 (1857); Dumas, Annales de chimie et de physique (3), 55, 175 (1859); 
Kesster, Pogg. Ann. 113, 145 (1861); Unger, Archiv der Pharmacie 19%, 194 (1871): 
Cooke, Proc. Amer. Acad. 5, 13 (1877); Kesster, Ber. deutsche chem. Gesellschaft, 
12, 1044 (1879): Scunemer, Ueber das Atomgewicht des Antimons, Berlin 1880. 
Journal f. prakt. Chemie (2) 22, 131 (1880); Cooke, Amer. Journ. Sciences and 
Arts, May 1880; B. B. 13, 951 (1880); Premrer, Lies. Ann. 209, 161 (1881); 
Popper, ibid. 233, 153 (1886); Boxcartz, B.B. 16, 1942 (1883); G. Cl. Friend 
and Kpeéar 1, Sarra, Journal Americ. Chemical Soc. 23, 502 (1901). 

2) The constants of nature, Smithonian Miscellaneous Collections Part V, 
Washington 1897, 


Proceedings Royal Acad. Amsterdam. Vol, Y, 
5 ) 


( 544 ) 


2. Popprr'), under von PrsBats guidance has tried to make a 
determination of the atomic weight by an electrical method. 

He connected in the same circuit a silver coulometer and a cell 
containing a hydrochloric acid solution of antimony trichloride. A 
rod of pure antimony (wrapped in linen) suspended in the liquid 
constituted the positive electrode, whilst the negative electrode con- 
sisted of a weighed platinum wire. 

During the electrolysis the electrolyte was kept in continual motion 
by means of a stirrer so as to exclude local changes in the concen- 
tration of the liquid. 

Under these circumstances explosive antimony is deposited on the 
negative electrode *). Popper fused the substance formed in a tube 
made of hard glass in an atmosphere of nitrogen; in this way 
the antimony trichloride present in the metallic mass was expelled. 
As soon as all the chloride had volatilized the antimony regulus was 
washed first with solution of tartaric acid, then with water, dried 
at 120° and weighed. . Additional experiments had proved that the 
glass tube did not suffer any alteration in weight on heating and 
melting the metal contained therein. 

The silver electrode in the coulometer was wrapped in a piece 
of linen. After the electrolysis was completed, the silver which had 
deposited in the platinum dishes employed was boiled and washed 
with water until this no longer gave a reaction with hydrochloric 
acid and it was then dried at 120°. 

Porper’s results obtained in the electrolysis of solutions containing 
respectively 7 and 22 per cent of SbCl, are given in the subjoined 
table. We have, however, recalculated the data as Poppsr still uses 
the atomic weight 107.66 for silver whereas more accurate investiga- 
tions have shown this to be 107.95. 

In a second series of experiments in which a few more improve- 
ments had been made as regards the insulation of the silver coulo- 
meter, Poreprr found for 7 per cent solutions as equivalent weight 
the value 40.33, therefore as atomic weight the value 120.99. 

As he could not discover any sources of error in his process and 
still believed in the accuracy of the results obtained by Cooke, who, 
by purely chemical means, had found the atomic weight of antimony 
to be 119.9 he concludes his paper with the words: “Sollte nicht 
die Entdeckung des Elements “Germanium” durch Winkrer den 


1) Compare 1. 

?) Such was the case with solutions containing 22 per cent of Sb Cls. In solu- 
tions containing 7 per cent. Popper obtained crystalline non-explosive antimony. 
I will fully refer to this particularity later on in my paper with Dr, Ringer. (CGOHEN.) 


( 545 ) 


: ae Weight of the metal Electrolytic | Atomic 
Grams of deposited in the same time quivalent reloht 
Sb Cl. in 400 (deposited same time — equivalen weight. 
Gr ; circuit in the same time. 
rams ; ; zi 
ED TE EREN of Antimony (Silver 
| Antimony | Silver == 107.93) 
7 1.4788 3.9655 402% | 190.75 
yi 2,0074 5.38649 40.39 Th Temes PV 
Zi | he 18903. |) 44 A847 | 10.45 | 121.99 
i 4.1885 44.4847 | 1042 121.26 
7 5.6869 15.1786 10.43 | 491 .29 
7 | 5.6994 | 45.4786 LO. AG 121.38 
2 | 1.4856 3.9655 40.43 121,29 
22, | 20120 5. 3649 A) 47 AOA AA 
29 | 3.8882 | 10.3740 4. AD 191.35 
22, | 3.8903 10.3740 AO AT 424.44 
22 | SO ENO =" | 14.3868 40.48 | 12 44 
22, 4 W752 11 


3868 40.52 | 121.56 


Wee andeuten, auf welchem die Lösung des vorliegenden Rätsels zu 
te) (a! oo 
suchen sei?” 


3. We have not only repeated the research of Porper but also 
extended the same by using hydrochloric acid solutions of SbCI,, 
whose concentration varied between 2.3 and 83.3 percents of SbCI, by 
weight. 

It was necessary to pay particular attention to the purity of the 
materials employed. The antimony trichloride was obtained from 
Merck; 20 grams were dissolved in solution of pure tartaric acid 
and then digested on the waterbath for some hours with excess of 
clear sodium sulphide. The liquid remained perfectly clear *). 

Some kilos of this antimony chloride were precipitated with sodium 
carbonate free from foreign metals, the precipitated Sb, O, was washed, 
dried and reduced to metal by fusion with pure potassium cyanide 
in a Perror’s furnace. The crucibles used were previously tested to 
see whether they would yield any foreign metal to potassium cyanide 
but we could not prove the presence of any impurity in the melt. 

1) As commercial antimony generally contains lead whose atomie weight exceeds 
that of antimony it was absolutely necessary to prevent the possibility of any lead 
being present in the materials employed, 


ik 


vi 


ee 


( 546 ) 


The fused metallic antimony was poured into cylinders of asbestos 
paper tied round with copper wire: the rods of antimony thus formed 
were cleansed with hydrochloric acid and washed. 

sy way of control we dissolved a piece weighing 20 grams in 
pure strong nitric acid with addition of 75 grams of crystals of 
tartaric acid. The clear acid solution so obtained was rendered alkaline 
by adding small lumps of sodium hydroxide prepared from metallic 
sodium (the lye was free from foreign metals) and digested on the 
waterbath with a clear solution of sodium sulphide but gave no 
precipitate. 

The solutions were prepared by weighing the pure antimony 
trichloride roughly and dissolving the same in pure hydrochloric acid 
of 1.12 sp. gr. at 15°. The exact composition of the solutions was 
determined by electrolysis of the liquid in presence of sodium sul- 
phide according to NeuMANN’s directions '). 


4. In each experiment two silver coulometers were put into the 
circuit; one in front and one behind the series of antimony solutions 
which took part in the electrolysis. The coulometers consisted of 
200 ce. platinum dishes with rough inner surfaces. We will not 
omit to point out that such dishes are particularly suited for coulo- 
metric determinations as it is possible to precipitate in them a large 
amount of silver with little chance of any traces being detached on 
washing the precipitates ©). The amount of silver deposited in our 
experiments varied from 25 to 50 grams whilst when using the smooth 
dishes usually employed it is difficult to handle a few grams without loss. 

As electrolyte we used a LO or 15 per cent neutral solution of 
silver nitrate; no difference was noticed with these solutions. The 
positive silver plates were cast of silver which we received from 
Dr. Horrsema, Comptroller-general at the local Government Mint. 
On analysis, we could not trace foreign metals in LOO grams of this 
silver. The plates were 6.5 ¢.m. in diameter and 4 min. thick. 
They were surrounded by a covering of filter paper (SCHLEICHER and 
Seneur). Each silver plate was suspended by a thick platinum wire. 
The coulometer dishes after being filled with the silver solution were 
covered with a glass plate with a hole in the centre through which 


a platinum wire was introduced. 


2) Analytical Electrolysis of Metals, Halle 1897, S. 145. 

Here, we provisionally took the atomic weight of antimony to be 120; as will be 
seen from what follows, the uncertainty of the atomic weight is of no consequence here. 

2) Compare Kanre. Wiep. Ann. 67, N.F. 1 (1899); Ricnarps, Coins and Hemrop, 
Proc. American Acad. of Arts and Sciences XXXV, 123 (1899), Ricwarps and 
Hemrop, Zeitschr. f. physikalische Chemie 41, 302 (1902), 


(547) 


Great care was bestowed on the insulation of all the apparatus. 
The conducting wires were strongly insulated and were, as far as 
possible, in contact with air only. Each platinum dish was placed 
on a copper plate which stood on a glass plate; the latter was 
carried by porcelain insulators which acted as feet. 

For a rough orientation a technical ammeter was included in the 
circuit; the current was taken from 1 to 3 storage cells. 


5. The antimony solutions which were subjected to electrolysis 
were contained in spacious beakers (1 litre) (B in fig. 1) in which 
constant stirring could take place by means of Wirt’s centrifugal 
stirrers. A Herricr hot-air motor kept all the stirrers in motion. 
The rods of antimony which served as positive electrodes were sur- 
rounded by a piece of linen which was fixed to the rod with platinum 
wire, or by glass tubes closed at the lower end containing a large 
number of not too small perforations (0, O, 0...) (8 or 4 m.m.). 
The object of surrounding the rods was to prevent any loose particles 
of antimony from getting into the liquid. 

As negative electrodes we used platinum wires (/?) about 10 em. 
in length and 0.8—0.4 mm. thick; they were provided at the upper 
end with the capillar glass pieces (C), on which a number was 


engraved. 

Both antimony rods and platinum wires were attached to copper 
binding screws which moved along glass standards (GS). In order to 
prevent contamination of the liquids by contact with copper, a piece 
of platinum wire (1) was placed between the binding screws and 
the rods of antimony or platinum suspended thereby. 


6. The experiments were now conducted as follows: After the 
platinum wires had been weighed they were put in their places; 
the silver coulometers were connected up and the current closed. 
At the commencement the strength of the current may only amount 
to a few hundredths of an ampere; if this is exceeded, evolution of 
hydrogen instead of separation of antimony takes place. When the 
precipitate on the platinum wires had reached a certain quantity, 
when in other words, the surface had become enlarged the strength 
of the current was increased and gradually raised to about 0.3 ampere. 

At the end of the electrolyses the rods were rinsed with a 12 per 
cent solution of tartaric acid’), then washed with water, alcohol and 
ether and dried over sulphuric acid in a desiccator. 


4) By a special experiment we had convinced ourselves that this did not cause 
any perceptible diminution in weight. 


( 548 ) 


To determine the amount of antimony separated by the current 
the following method was adopted *). 

The rod was placed in a tube of hard Jena glass closed at one 
end (length of the tube 30 em, diameter 1 em). This tube had 
been previously cleaned, strongly heated in a current of dry air 
(dried over H, SO, and P,O) and then weighed. The antimony 
rod was now weighed and by way of control the tube and rod 
were again weighed together. 

The air from the tube was now expelled by means of a continual 
stream of carbon dioxide which had been dried over sulphuric acid 
and phosphoric anhydride. The tube (explosion-tube) was then closed 
with a properly fitting india-rubber cork and put into a metal cooling 
vessel made of composition tube in the manner represented in fig. 2. 
This tube was connected with the water tap. 

If now the explosion tube is shaken for a moment the explosive anti- 
mony explodes. The tube is then strongly heated with a triple burner 
on the spot containing the rod ; the Sb Cl, evolved condenses on the cold 
wall of the tube to a clear white mass. The heating is continued 
until the antimony is perfectly fused and this is then allowed to cool 
slowly. The tube is then opened, the SbCl, is removed by rinsing 
with a mixture of alcohol and ether (3:1) the tube is then rinsed 
with ether and dried by heating in a current of dry air as described 
above. 

The tube with the antimony regulus is now weighed. 

A previous experiment had proved that the explosion tube suffers 
no alteration in weight by the heating and subsequent treatment. 
It was found for instance that an explosion tube weighed 29.6614 
gram before the experiment and 29.6610 gram after the experiment 
the contents having been removed by means of nitric and tartaric 
acids. 

By way of illustration one of the experiments is reproduced in 
detail whilst the results of the other measurements are united in 
a table. 


Electrolysis of a 15.6 proc. SbCl, solution. 
Silver coulometer N°. 1. 
weight of platinum dish + silver 73.1920 grams 
" " " 36.7310 fe 


weight of silver 36.4610 grams 
*) Further particulars about this method will be found in the paper of Coney 
and Dr, Ringer. 


oP Bet SAO Nee 

ERD birtd 
AVISIW AAT IMA 
PAO ALT IANA Dg 


ANS 


f 

g rH . 

| i 
| ) 


\ 


8 
A 
4 1 
a 
i 
Bo 
‘ ; 
4 
. 
‘7 | 


ERNST COHEN and Th. STRENGERS. On the atomic weight of Antimony.” 


Proceedings Royal Acad, Amsterdam, Vol. V 


( 549 ) 


Silver coulometer N°. 2. 
weight of platinum dish + silver 71.4580 grams 
" I" I 34.9902 


weight of silver 36.4628 grams 


weight of explosiontube + regulus + platinum wire 55.0281 grams 
" " 41.0780 


weight of regulus + platinum wire 13.9501 grams 


weight of platinum wire 0.2696 — » 


weight of regulus 13.6805 grams 


From this result the equivalent weight of the antimony is calculated 
as follows: 
107.93 


ES 49 6805 — 40.49. 
36.4608 °° 19-6805 


The results so obtained are collected in the following table. (p. 550). 

From this table we see that the atomic weight obtained increases 
with the concentration of the Sb Cl, solutions and varies between 
120.87 and 121.89 within the concentrations 2.3 and 83.3 per cent. 

From this it is quite plain that we cannot arrive at the determination 
of the atomic weight of antimony by the electrolysis of solutions of 
antimony trichloride and that the values found by Popprr, to which 
in the calculation of the atomic weight is attached the same value as 
to those of SCHNEIDER, COOKE and BoNnGArtz'), are quite accidental, being 
dependent on the concentration of the solutions employed. 

It further appears from the above that unknown electrolytic or 
chemical changes play a part here which require further investigation 
and which may be expected to add to our knowledge of the formation 
and composition of the remarkable explosive antimony. 

We hope, shortly, to investigate these changes. 


1) Compare Osrwarp. Lehrbuch der allgemeinen Chemie I, 53 (1891). 


) 


z3 a katy Se * es ae > 
ee en 8 pes 
(5505) = WEET 
Er 


Grams of | Weight of Weight of the silver in the. nivalis | Atomic 


Sb Cl, in 100, the antimony | Coulometer in grams. | weight | weight 
grams regulus in | of the of the 
solution. | grams. | 04. | No 9. Net | Nea | Antimony. ne e 
23 | 16.8747 | 45-2069 45-2019 108 | 
| | | 120.87 
9.3 | 414.5014 39.C805 39.0816 | 4029 | 
—* Hs Sige ae EREA 
3.4 18.36 18.7961 Ee 50.3791 50.3860 40.26 190.781) 
—|——— AS eed =) Soe 
5.0 | 416.9175 | 45.2019 4. 2069 40 38 
| | 421.47 
5.0 | 14.6298 | 30.0805 39.0816 40,39 
En | nd _— rn 
3 | | | 
5.3 | 48.8627 | 50.3791 50.3860 40,40: 
5.3 | 12.6206 | 33.7224 33.7203 40.38 | 124.90 
5.3 | 45.0054 | 40.0810 | 40.0794 | 40. | 
a KE ke EE 
144 | 43129 | 3 9633 | 34.9680 | 40.29 | 
14.4 | 48.8881 50.3791 50. 3860 40.46 124A 
14.4 | 12.6470 33.7994 33.7208 40.47 
a IRE EEE EN 
15:6 | 9.5049 | 25.3M6 2 3407 40.48 
/ 
15.6 13.6805 36.4640 36.4698 | 40 49 121.47 
„45.6 | 13.6803 | 36 4610 364628 | 40.49 
18.8 13.5984 | 36.2088 36.209 40.53 
| | 121.59 
18.8 | 43.8618 | 36.9531 36.9566 | 40 53 
| 3 : 
52.2 | 44.6212 | 38.9046 38 9098 40.56 
| | | 121.71 
522 | “45.0689 | 40-0810 400704 | 40.58” 
55.7 | 413.7192 36.4610 36.4628 40.58 8 
| 194219 
55.7 | 44.7014 39.0805 39.0816 40.59 
83.3. | 43.6305 36.2088 36 209% 40.63 
83.3 | 14.9494 — | 39.6998 40.61 521,59 
83.3 | 13.8998 36.9531 | 36 „9566 40.64 


| 
' 


1) This sent is decidedly loo low, as a trace of antimony got ‘ost during the 
washing. 


(551) 


Chemistry. — “The conductive power of hydrazine and of substances 
dissolved therein.” By Prof. Erxst Cone and Prof. C. A. Losry 
DE BRUYN. (Communicated by Prof. C. A. Lopry pr Bruyy). 


(Communicated in the meeting of February 28, 1903). 


The investigation of the conductive power of non-aqueous solutions 
has of late years been known to have an increasing significance and 
particularly so on account of the important result that the laws and 
rules applying to aqueous solutions do not appear to apply in the 
case of other solvents. Apart from methyl and ethyl aleohol (the 
constitution of which does not differ much from the type water) 
sulphurdioxide, ammonia (NH,), formic acid, hydroeyanie acid, pyri- 
dine, some nitriles, hydrogen peroxide and others have been studied 
as such’). | 

The physical properties of free hydrazine ®) N,H, although still 
incompletely known, might lead us to suppose that this liquid would 
manifest a strong ionising power. In the first place, like water, the 
lower alcohols and acids, it possesses an abnormally high boiling 
point. This is obvious if this point (about 113° at 760 m.m.) is 
compared with of ammonia (— 34°), difference of 147°, and if one 
considers that the difference between the boiling pomts of CH, and 
C,H, is decidedly less (80°); this fact as well as the high critical 
temperature of (at least) 880° point to an association of the NH, 
molecules. The solubility of several alkali salts in hydrazine has also 
been shown to be very considerable although less than in water. 
Another existing observation points to the fact that hydrazine may, 
like ammonie take the place of water of crystallisation *). And finally, 
the dielectric constant of hydrazine, which Prof. P. Drepr (Giessen) 
had the kindness to determine at our request, has turned out to be 
rather high, namely, 53 at 22°. It is now a known fact that there 
exists a certain although sometimes remote parallelism between the 
dissociating power of a liquid on the one hand and the association 
of its molecules, the solvent power and the dielectric constant on 
the other hand. As according to the experiments of FRANKLIN and 
Kraus and of Capy liquefied ammonia is an ionising solvent, this 
might also be expected in the case of hydrazine. From the experiments’) 
presently to be described it will be seen that such is the case. 


1) Compare Joxes, Am. Ch. J. 25. 232. Kantenpere, J. Phys. Chem. 5. 339. 
Wapex and Cenrverszwer, Z. phys. Ch. 39. 514, 557 e. by J. Traupe, Chem. 
Zt. 26. 1071. (1902). 

2) Lopry pe Bruyn, Recueil des Travaux Chimiques des Pays-Bas. 15. 174. 

3) Ibid. 179. 


3 A: sos ee Wan: Rr at : i476 
4) Some preliminary determinations were already m ide in 1896, 1. e. 179, 


Let us first observe that the dielectric constant of hydrazine is 
only surpassed by those of five other liquids and is decidedly larger 
than that of NH,. We have namely: 


hydroeyanie acid = 95 acetonitrile 40 

hydrogen peroxide 93 nitrobenzene 36.5 

water 82 methylaleohol 32.5 

formic acid 57 ammonia 22 (at —34°) 
nitromethane 56.5 pyridin 20 

hydrazine 53 


The peculiar properties of hydrazine (its very hygroscopic nature 
and liability to oxidation by atmospheric oxygen) demand great 
precautions in its preparation. It took place, according to the method 
already deseribed *), by treatment of the so-called hydrate with 
barium oxide and distillation in an atmosphere of hydrogen. 

The heating with barium oxide and subsequent distillation were 
thrice repeated and the base was finally collected in six different 
fractions in pipette-shaped tubes in the manner previously described. 
During the last distillation the base had been only in contact with 
purified, dry hydrogen. 

Apart from the properties of hydrazine mentioned, the high cost 
of the material was a factor which in our experiments had to be 
taken into account. A special apparatus (see illustration) was, therefore 
constructed which admitted of working with a small quantity of the base 
(about 5.5 ee.) and through 
Which pure, dry nitrogen *) 
could be passed, whilst 
through the exit tube for 
the gas the weighed portions 
of the different salts could 
be introduced. 

On account of the some- 
What limited quantity of 
the base at disposal we 


could not, as is customary 
in the determination of the 
conductive power of solu- 
tions, start with the largest 
concentration and succes- 
sively dilute this by adding 
the solvent, but the reverse 
was to be done. 


1) alsem 
*) We take the opportunity to call attention to the fact that platinised electrodes 


(oane 


Weighed quantities of a salt were, therefore, successively dissolved; 
on account of the unavoidable errors in weighing it was difficult to 
experiment with very dilute solutions of accurately known composition, 
but by evaporating a measured quantity of a very dilute aqueous 
solution in a pipette which was then rinsed with the hydrazine we 
have reached for KCl a concentration of V = + 900. 

In view of the above we wish to remark generally that our 
results cannot lay claim to very great accuracy, although they quite 
suffice even from a quantitative point of view, to prove that free 
hydrazine has a strong ionising power comparable with that of water. 

We have worked with solutions of H,O, KCl, KBr, and KJ and 
made a few experiments with a solution of Na and H,N in N, H,. 

In the first experiment the six different fractions of the hydrazine 
had not been kept separate; as we had previously found?) that the 
meltingpoints of the second and fourth fractions were the same we 
thought we might conelude that at least the middle fractions were 
similar. It then appeared, however, that the conductive power of 
the bases taken from different tubes often showed appreciable 
differences. 

For this reason a second preparation was made and the hydrazine 
of each fraction (each time collected in several tubes) was examined 
separately as to its conductive power. From the following figures it 
appears that the conductive power gradually decreases and is smallest 
for the last fraction. 


fraction n°. 2 Wat AS tAO 
3 12.8 „ 
4 12, 
5 10.0 , 
6 6:52 


We do not know what impurity (in any case very small) is the 
cause of this; possibly we are dealing here with a minute quantity 
of ammonia which is present in largest amount in the first fractions 

The smallest conductive power observed by us in any fraction 
prepared previously was 4.10. 


Our experiments have been mostly conducted with fraction N°. 6 
of the above-mentioned quantity. 


dried in the air may occlude such an appreciable amount of oxygen that this 
must make its influence felt when working with readily oxidisable liquids. Such 
appeared to be the case when filling our apparatus with hydrogen when a spont- 
aneous deposit of visible drops of water was formed. 

*) Prepared from air and phosphorus. 

a Cea De 17. 


(BDE 


The apparatus was put into a glass vessel containing paraffin oil 
which was placed in an Ostwald thermostat; the temperature was 259, 


Hydrazine and water (¢ = 25°) 


5e fraction. Gono: Ge fraction. G = 4.249. 

N. X N x 
0 10.0 .40—° 0 6.04.10 — 
0.93 9.79 » 41.1 AET Wie 
7.94 8.95 » 49.5 45 » 

Ay TOS) 58.4 AO) 

{dre Neve) 69.5 4.55 » 

d5:6 6/04» oO elas gree 
82.4 6.09 » 124.7 ees D 

101.8 7.85 » 

156 10751 > 

Daa leen es 


Potassiumehloride. 


== ee ees 
NH, 
G (as V Kx a\ 5) 
5.369 0,0272 14.7 0D 402.9 
) 0,0157 254 4.2» 103.7 
» 0,0080 10.7 DF B 109.3 
[5.4 0,00045 + 900 143.407 st A07 ZN 


Potassiumbromide. 


LD x — 6,5.10—° 
Nol, 
G g V % A 
5.350 0,0617 10.3 10.05.103 103.8 
» 0,0329 19.3 5.66 » 109.2 
) 0,021% 29.9 oth 142,7 
» 0,0105 60.7 1.965 » 118.9 


1) A could not be determined, so that the degree of dissociation of the salts 
is not known. The a’s, however, agree in magnitude with those of the aqueous 
solutions of the same salts. 

2) This value, obtained in the manner described on p. 553, is as a matter of 
fact uncertain. It proves that a very minute quantity of a dissolved substance may 
increase the conductive power considerably. 


( 500 ) 


Potassiumiodide. 


p25. x= 5,6.10 —° 
Na Hi 
G g Vv % A 
5.600 0,072 12.9 8.19.10 9 105.6 
» 0,049 18.8 oe 108.8 
» 0,0280 830 3.40 » 112.8 
> 0,0129 72 1.64 » 18 
G = weight of hydrazine in grams. A = aequivalent conductive power. 
g = weight of the salt in grams. V = number of Liters, in which is dis- 
; solved one mol. of the substance. 
x = specifie conductive power « for the water used = 0,28.10~° 


Without committing a grave error the sp. gr. of hydrazine at 25° may be taken 
to) te) to) A, 
as 1.00. 


It is already known that sodium dissolves in hydrazine with 


evolution of hydrogen ). Pure hydrazine (9, 1.102) was introduced 
into the apparatus and two particles of sodium (weighing about 10 
milligrams) were added. 

The metal slowly dissolved with evolution of hydrogen and after 
solution was complete the specific conductive power appeared to have 
increased to 131.10. 

It seemed very peculiar that a powerful evolution of gas still went 
on after the sodium had dissolved, showing a decomposition of the 
hydrazine with formation of ammonia. This decomposition ceased as 
soon as the liquid was poured out of the apparatus; apparently it 
only takes place by contact with the platinum black present on the 
electrodes and is, therefore, quite comparable to the spontaneous 
decomposition of an alkaline solution of hydrogen peroxide exposed 
to the same influence. 

Finally a few experiments were made with a solution of ammonia 
in hydrazine. The solubility of that gas at the ordinary temperature 
did not seem to be large; about 4.8 per cent of N H, is present in 
the saturated solution. After a few bubbles of ammonia had been 


absorbed in the hydrazine (with * = 5.2.10~) the conductive power 


appeared to be but slightly increased (% = 6.9.10-5); this was also 
still the case after the liquid had been saturated with ammonia (about 


1) Le. p. 183. Dr. J. W. Drro has found that an atom of hydrogen is replaced 
here; the NaH, N, formed is a substance which on being exposed to the air 
causes a violent spontaneous explosion, 


( 556 ) 


220 “mer; Of H‚N in 45920: prof ON Av aes a ee 
is known that on dissolving ammonia in water the conductive power 
is but very slightly increased. 


From the foregoing we may draw the conclusion that, with regard 
to its ionising power, hydrazine is comparable to water. 

As regards mixtures of hydrazine and water it may be observed that 
on addition of water the conductive power at first decreases reaching 
a minimum with a mixture of 60 mols. of H,O to 100 mols. NH, 
(about 25 per cent of H,O and 75 per cent of N,H,) then increasing 
again. This minimum, therefore, does not correspond with the com- 
position N,H, + H,O, or the so-called hydrate. 

Utrecht— Amsterdam, January 1905. 


Chemistry. — “The velocity of transformation of tribromophenol- 
bromine into tetrabromophenol.” By Mr. A. H. J. Berzer *). (4t 
Communication on intramolecular rearrangement, presented by 
Prof. C. A. Lospry DE Bruyn). 

(Communicated in the meeting of February 28, 1903). 


JENEDIKT ?) found in 1879 that tribromophenol brought into contact 
with bromine water is capable of exchanging a fourth hydrogen 
atom for bromine with formation of a tetrabromo-derivative. The 
study of this substance led him to the conclusion that one Br-atom 
occupies a peculiar position in the molecule; it is, in fact, the cause 
of a certain number of reactions in which that Br-atom is readily 
displaced. As moreover the new substance seemed to have lost 
the character of a phenol as shown by its insolubility in alkalis, 
BENEDIKT gave it the formula C,H, Br,.OBr and the name of tribro- 
mophenolbromine. Brenepixr also noticed that, when melted under 
sulphuric acid, it passes into the already known isomeric tetrabromo- 
phenol, a true phenol which no longer contains a loosely bound 
Br-atom. 

In his first publication BexepiKT looked upon this transformation 
into tetrabromophenol not as an intramolecular displacement of atoms 
but as a process taking place between two mol.s of tribomophenol- 
bromine; in a later communication however he does so, without 
Stating any reasons. 

When a few years ago, Jon. Tuimre®) found that BeNEDIKT's 


1) Proc. 31 May, 28 June and 25 Oct. 1902. 
2) Annalen 199. 127, Monatshefte 1. 361, 
5) Ber. 33. 673 (1900), 


tribromophenolbromine by means of leadacetate passed into 2.6 
dibromoquinone, with substitution of 2 Br by O, he looked upon it 
as a dibromoquinone in which one O is replaced by 2 Br | therefore 
as a tetrabromoketodihydrobenzene 


; he is of opinion that its forma- 
tion from tribromophenol can only be explained by assuming that 
the latter can react in the tautomeric form of a p-quinoid ketone 
as follows: 


i Ne AN 
a Ve H BEN ve _—>- aN ee 


In a paper which appeared a year ago, Kasten’) has come to the 
same conclusion as THIELE, as the result of investigations conducted 
conjointly with LORVENHART, Rosa SprijnR and Ginpurt. Kasrun has 
also established the fact that it is only sulphurie acid which, even at 
the ordinary temperature, is capable of causing the transformation 
into tetrabromophenol; a dozen other reagents gave a negative result. 
In order to explain this specific action of sulphuric acid, Kasrrn 
assumes the intermediate formation of an additive product of this 
acid with tribromophenolbromine ; this at first would lose HBr, which 
would then again react at once with reformation of sulphuric acid 
and cause the migration of Br into the benzene nucleus. This inter- 
pretation of the transformation requires the appearance of two non- 
isolated and therefore hypothetical intermediate products and of three 
successive reactions. 

Mr. Brerzer has now studied the velocity of transformation of tri- 
bromophenolbromine. The circumstance that the first substance readily 
parts with an atom of bromine would lead to expect that its 
quantitative estimation would be possible in the presence of tetra- 
bromophenol. It now appeared that the elimination of free iodine 
from hydriodie acid, also observed by Kasrrn, takes place quantita- 
tively; tribromophenolbromine may therefore be estimated in the 
presence of tetrabromophenol by titration. 

At the commencement of the investigation the behaviour of the 
solid substance towards sulphuric acid was ascertained. If the crystals 
are covered with the ordinary 96 per cent acid it is noticed that 
they lose their yellow colour and become opaque and white; of 
solution in the acid taking place nothing can be perceived even by 
the aid of the microscope. No formation of striae can be observed; 
the whole phenomenon seems to be enacted within the solid substance 
commencing on the surface where the substance is in contact with 


( 558 ) 


the acid. If the velocity of transformation is measured under these 
circumstances it is no matter for surprise first/y that no reaction 
constant is found, second/y that the reaction coefficient constantly 
diminishes as the inner parts of the crystals get more and more 
inaccessible to the acid. As expected beforehand the experiment has 
shown that very small crystals or the powdered substance are, on 
account of the larger free surface, more rapidly transformed than 
the larger crystals. The continuation of the research will show that 


the transformation is monomolecular and must, therefore, be taken as 


a real displacement of atoms (perhaps of two displacements one of 
which takes place with very great velocity). It is a remarkable fact 
that there should take place inside the molecule of a solid substance 
a displacement of atoms, an internal change of equilibrium leaving 
the molecule intact, by mere contact with sulphuric acid, without 
there being any question of solution. 

Although we could not expect to get reaction-constants for a 
heterogenous mixture of a solid substance and sulphuric acid, this 
should be duly the case when we worked in a solvent. Here however 
a difficulty occurred which at first threatened to put a stop to the 
further prosecution of the research. A solvent was wanted which 
had no action either on tribromophenolbromine or sulphuric acid. 
Acetic acid scarcely dissolved the first substance and chloroform 
appeared to dissolve only traces of 96 per cent sulphuric acid. It 
was finally decided to choose the latter solvent and to thoroughly 
shake the solution with sulphuric acid‘). The experiment proved 
that on applying the formula of the first order, constant reaction- 
coefficients made their appearance. A first result was thus obtained; 
the transformation does not proceed bimolecularly. 

Mr. Brizer has now studied the influence of the concentration of 
the sulphurie acid and the temperature. 

In most of the experiments, 3 grams of the substance were 
dissolved in 150 ce. of pure chloroform *), the solution strongly 
shaken with the acid and after definite times 25 cc. were titrated. 

Use has been made of: 

a. H,SO, with about 36°/, SO,, 6. H,SO, with about 1°/, 5O, 

c. equal volumes of 6 and d. d. 96 per cent H,SO,. 

In the following tables the results obtained are not given in the 

form of reaction-constants, but to make the matter more plain, the 


1) A uniform emulsion is very soon obtained. 

2) The chloroform was agitated a few times with water, dried over calcium- 
chloride, shaken with strong sulphuric acid and redistilled; it was preserved in 
the dark, 


( 559 ) 


times (T) are mentioned at which the transformation has proceeded 
halfway. 


A. Influence of the Concentration of Sulphurie Acid 


t = 25°. 0,5 ec. sulphurie acid. 
acid a | b | c d 
Te | 9 min. 49 sec. | 2 hours 57 m. | 13 h. 40.5 m very slowly 


= 25°. 1 ec. sulphuric acid. 


acid a b 
ig too rapid 25 m. 44 s, 


% d 
2h. 38.5 m. Zh. 45 m. 


B. Influence of the Quantity of Sulphurie Acid 


= a vac van 


1 ec. | 0.6 ce. 
ree 


too rapid too rapid 5 


0.5 ce. | 0.3 cc. 


5 m. 49 s, oh. Our: 
14 acid Ty 
2 ce. pre ) | 1.25 ec. 1 ce. 0.5 ce. | 0.25 ce. 2) 
T. | too rapid | too rapid | 25 m. 44 s. | 55 m. 20s 


de 2E D7 mA. | 


2. ACG 

1.5 ec. 1 ce. 0.5 cc. 
Ii de he oem. Ei SH So. Am. drh. 40:5, m: 
Dh 38m, 


C. Influence of the Temperature. 


Acid a. 
0560. 0.3 ec. | 0.2 ce. 
T. at t = 35° eames 6m. 12.58) 4 99| 32m. Bs 
» 25° 5 m. 49 .) + 10 (9 hi, Sm: | times —— 
» 159 [58 m. 45 s. J times | 


Acid b. 


1 cc. 0.5 ee. 
DA eone — 33. m, 56 s. | 
» 5 (B m. Ms.) 49 |2h. 57 m,) times 


» 1500 doch 165 m.) times 


) Transformation almost completed after 20 minutes. 
*) Not yet decomposed to the extent of 15 °/, after 21 hours. 


38 
Proceedings Royal Acad. Amsterdam. Vol. V 


( 560 ) 
Acid ¢, Acid d. 
LNG, A ce. 
Ts bh 58 m. 10 s. 1 h- 53:6 m. 
» 25° 2 h. 35 m. 7h. 45 m. 
» 15 3 h. 27 m. | 


From the results obtained it appears in the first place that the 
transformation is a monomolecular one and, taking into consideration 
the circumstances under which it takes place, must be considered 
as an intramolecular rearrangement of atoms. 

To this conclusion the following observations may be added. 

A. The influence of the concentration of the acid, the other circum- 
stances being the same, is very great. The course of the figures leads 
to the idea that the active agent, the catalyser is not H,SO, but SO, 
Experiments were therefore made to ascertain how chloroform 
behaves towards the four acids employed. Whilst from ordinary 
96 °/, acid (d) but very minute traces were dissolved, this amount 
was perceptibly larger with acid c and still larger with acid 4, 
whilst acid « appeared to yield very much SO, to the chloroform *). 

The idea that SO, is the catalysing substance is consequently 
confirmed. The rapid decrease of the concentration of the acid is 
also in agreement with this idea; this velocity is therefore as it 
were a measure of the concentration of the SO, still present in a 
sulphuric acid of given concentration. 

B. It is now also very plain that the quantity of the acid must 
have a great influence. As shown by its behaviour to acid a, chloro- 
form may dissolve considerable quantities of SO,. On shaking with 
sulphuric acid of a lesser concentration, the amount of SO, which 
passes into the chloroform will consequently depend on the quantity 
of the acid. The equilibrium for the SO, which distributes itself 
between the chloroform and the sulphuric acid changes, as is known, 
with the relative quantities of the two liquids and with the 
temperature. 

As a consequence of the view taken here, it must be assumed 
that ordinary 96 °/, sulphuric acid still contains a minute quantity, 
of free SO,-molecules. This view is admissible *) since it is known 


1) The ratio in which different acids yield SO3 to chloroform will be further 
determined. 

2) KyretscH, in his well-known research on sulphuric acid, has shown that an 
acid of 97—98 0/, absorbs SO; much more readily than acids of smaller or 
larger concentration. From the results obtained up to the present it does not 
appear that, in the transformation of tribromophenolbromine, the 98 °/, acid c 
behaves in a particular manner; an extension of the research will elucidate this 
question, 


that 100 °/, sulphuric acid contains a little SO, and consequently 
free H,O. 

C. The temperature-coefficient for sulphuric acid a is particularly 
large and increases rapidly with the temperature; for acid 5 it is 
decidedly smaller and very small for the 96 °/, acid. It will be 
readily understood that in the case of the acid « the dissociation of 
H,SO, into SO, and H,O and the distribution of SO, between chloro- 
form and sulphuric acid are modified in a large degree when a 
change of temperature takes place. 


The rearrangement of atoms may now be represented by the following 
schemes which respectively correspond with Benuprkr’s formula (1) 
and Trrmere’s formula (ID): 

LEE Gro Br Be br 
aC I Som = ng on pals mu Do 


Hire Br Ho, Br HBr 

Against the acceptance of Turenn’s formule (IL) it may be pointed 
out that in the displacement a Br atom must first remove an H 
atom; this then proceeds to the O atom with migration of the double 
bonds, a rather intricate process practically consisting of three succeeding 
displacements. As it has been proved that the reaction is one of 
the first order, two of those displacements must take place with 
immeasurable velocity. Against BeNepiKT’s formula (I) may be remarked 
that, according to experience, the meta-position is hardly ever selected 
in the migration of an atom or of groups from the side chain into 
the nucleus. 

The hypothesis proposed by Kasrrp, which assumes the inter- 
mediate formation and decomposition of non-isolated products, is not 
at all supported by the observations communicated here. 

The investigation as to the transformation of tribromophenolbromine 
will be completed and also extended to other analogous compounds. 


Geology. — “Some New Under-Cambrian Erratic-blocks from the 
Dutch Diluvium?. By J. H. Bonnema. (Communicated by 
Biota. VW. Morr). 


I. In the Geological-Mineralogic Institute at Groningen is found 
a piece of sandstone which a few years ago I found at Odoorn, in 
the province of Drente. With muriatic acid applied to it, there is 
no effervescence; consequently it does not contain any calcium- 
carbonate. The grains of sand are small, but with a magnifying 
glass they may be well distinguished. They are peculiarly lustrous. 

The colour of this erratic-block is chiefly dark-grey. Im some 

38* 


places it is brownish. Moreover there are light-grey worm-shaped 
parts, varying in length and having a breadth of about 6 millimetres. 
This erratic-block is most probably a piece of Under-Cambrian sand- 
stone, in which is found one of those problematical things that are 
sometimes called worm-passages. As they are not straight and do not 
run parallel to each other, they are different from those described as 
Scolithus linearis Hall. They show more resemblance with those tubes 
that were described by Torrent’) as Scolithus errans of Hardeberga 
and Andrarum. According to Horst’), however, there are various 
kinds of these worm-passages differing from Scolithus linearis Hall, 
whilst they also occur in different layers. This geologist makes men- 
tion of them as being found both in many places in the neighbour- 
hood of Simrishamn and near Kalmar. 

The Odoorn erratic-block bears no resemblance to the Hardeberga 
sandstone, in which Scolithus errans TorELL is found. Mosere *) writes 
that this sandstone shows a greyish-green colour, and that the worm- 
passages are dark-coloured. Nor does it resemble the Andrarum (For- 
semölla) sandstone. According to TurrBerG *) the latter is a white, 
quartziferous sandstone with yellow worm-passages. 

The erratic-bloek also differs from the “Kraksten’, which Horst 
mentions, as being found near Kalmar, and which is greenish grey. From 
the kinds of sandstone with worm-passages which according to Horst 
are met with in the neighbourhood of Simrishamm, differs that which 
occurs to the West of Raskarum in being whitish ; and that whieh 
is found close by Ljuuglyckorna is different because its worm-pas- 
sages possess a dark colour. The sandstone which, according to this 
geologist, occurs’ to the North-West of Raskarum, may resemble, in 
colour, the Odoorn erratic-block : he says that its colour is sometimes 
a dirty-grey one. Unfortunately he does not tell his readers what is 
the colour of the worm-passages. 

Consequently we cannot with certainty conclude whether this 
kind of sandstone still exists as firm rock, or not. 

Nor have I been able to find anything whatever concerning the 
presence of suchlike erratic-blocks in the German and the Dutch diluvium. 


1) Torett, Petrificata Suecana formationis cambricae. Lunds Univ. Arsskrift. 
1869: Tom Vip. 12. 

2) Horsr. Beskrifning till kartbladet Simrishamn-Sveriges geologiska Undersökning. 
1399 Ser Aa. N). 109,p.st3: 

Hotsr. Bidrag till kännedomen om lagerföljden inom den kambriska sandstenen. 
Sveriges geologiska Undersökning, 1893. Ser. C. NO. 130, p. 6, 13, 14. 

3) Mogera. Geologisk vägvisare inom Fogelsingstrakten. 1896. p. 30. 

4) TurrBerG. Om Agnostus-arterna i de kambriska aflagringarne vid Andrarum. 
Sveriges geologiska Undersökning. 1880. Ser. G. N°. 42, p. 3. 


"Ook ee 


( 563. ) 


Il. Some years ago I made an excursion in the surroundings of 
Murmerwoude in company with Mr. Borkn, at the time a teacher 
at Murmerwoude, now a teacher at a secondary school at Nimeguen. 
To the West of this village, situated in the north-eastern part of the 
province of Frisia, we found in the sand that lay by the side of a 
freshly-dug canal two slab-shaped pieces of sandstone that fit each 
other exactly and must have formed one whole. The dimensions of 
the bigger piece are about 20, 10 and 4,5 centimetres. The other 
piece also possesses the two first-mentioned dimensions, but the third 
is 3 centimetres. 

These pieces drew my attention as containing many more or less 
complete stone-kernels and off-prints of pyramidal Hyolithus-shells. 
The pointed ends of all these lie in the same direction, which must 
certainly be attributed to the influence of streaming water. 

These erratic-blocks consist of hard, grey, very fine-grained sand- 
stone. With muriatic acid applied to them there is no effervescence. 
Here and there they show small, yellow-brown spots. Some of the 
stone-kernels and that which lies close around them show the same 
colour. 

The stone-kernels are straight and slowly increase in breadth. 
The dorsal side is flat or somewhat concave; at the mouth it is more 
or less convex. This side is not lengthened towards the front, so that 
we have here a specimen of the subgenus Orthotheca. With the 
exception of the dorsal side the surface of the stone-kernels is regu- 
larly. vaulted. Consequently the transverse section is about circle- 
shaped, with only one segment cut off. Towards the pointed end 
they become more or less triangular. In one stone-kernel, which is 
not exposed to view in its full length, the visible part points to a 
length of about 35 millimetres and to a breadth, at the mouth, of 
7 millimetres. 

It appears from these properties that these stone-kernels originate 
from the Hyolithus (Orthotheca)-species, which has been described and 
pictured by Hotm’) as Hyolithus (Orthotheca) de Geeri. 

Horm tells us already that sandstone with Hyolithus de Geeri is 
Under-Cambrian. I have, however, not been able to find in his work, 
on what grounds this assertion is founded. Most problably he came 
to this conclusion because the nature of the stone points to it. At 
the time sandstone with Hyolithus de Geeri was not yet known as 
firm rock. Even now I have not been able to find in the books at 
my disposal, that sandstone with Hyolithus de Geeri should be known 


1) Horm. Sveriges Kambrisk-Siluriska Hyolithidae och Conulariidae. Sveriges 
geologiska Undersöknung. Ser. CG. No. 112. p. 54. 


( 564. ) 


as such. As far as I can see this species of Hyolithus, when Holm 
described it, had not been discovered in company with a fossil from 
which its age might be determined. Mopere’) afterward found many 
specimens in a few big blocks of sandstone, which furnished him 
the material for the description of the new species of Trilobites called 
Holmia Lundgreni. The latter lay in the neighbourhood of lake Tun- 
byholm in the eastern part of the province of Schonen; according 
to Mosrre suchlike stone with remains of Trilobites occurs as firm 
rock not far from this place. As Mopere informs us that sandstone 
with Holmia Lundereni is older than that with Holmia Kjerulfi Linrs, 
this was probably also the case with the sandstone-layers of which 
the Murmerwoude erratic-blocks formerly formed part. 

It appears from Mosere’s description of the stone of the erratic- 
blocks with Holmia Lundgreni, that this stone in some respects 
resembles the material of which the Murmerwoude erratic-blocks 
consist. Both are very fine-grained and contain no calcium-carbonate. 
There does not seem to be much difference in colour either, at least 
as far as some parts of the Swedish erratic-blocks are concerned: 
Mosere tells us that the sandstone deseribed by him is chiefly of a 
bright light-grey colour, though sometimes showing small brown 
spots of ferrihydroxide. My erratic blocks, however, contain no pieces 
of phosphorite, which those from the neighbourhood of lake Tunby- 
holm do. | 

Besides the erractic-blocks spoken of just now, others of sandstone 
with Hyolithus de Geeri-remains were also found, as Holm tells us, 
in the province of Schonen, near Simrishamn and Köpinge. 

The same author makes mention of suchlike stones having been 
gathered near Rüdersdorf not far from Berlin, and near Bützow in 
Mecklenburg. It follows from the descriptions he gives of these 
pieces, that petrographically they bear no resemblance to those found 
at Murmerwoude. The latter are least different from the erratic-block 
found by Prof. pr Grrr at Rüdersdorf. My pieces, however, contain 
no particles of glimmer. 

No more have corresponding erratic-blocks of Hyolithus-sandstone 
been found in any part of the Netherlands. The first of this kind of 
stone were made mention of by vaN CALKER*). They originate from 
Steenbergen in the northern part of Drente; they are three stones 


1) Mopere. Sveriges älsta kända Trilobiter. Geol. Foren. in Stockholm för- 
handlingar 1899. Bd. 21. Haft 4. p. 324. 

2) VAN CALKER. Ueber ein Vorkommen von Kantengeschieben und von Hyoli- 
thus- und Scolithus-Sandstein in Holland. Zeitschr. d. Deutsch. geol. Gesellschaft. 
Jahrg. 1890. p. 581. 


ps 


( 565 ) 


resembling each other. From the description van CALKER gives of the 
stonekernels occurring in them, Hor already drew the conclusion that 
they originate from Hyolithus de Geeri. These erratic-blocks consist, 
however, of dark asch-grey sandstone, so that they differ in colour 
from the Murmerwoude ones. 

Afterward two more pieces of Hyolithus-sandstone were mentioned 
by me’). One was found at Kloosterholt (Heiligerlee), the other 
at Roden, in the North of the province of Drente. The former is a 
small piece of fine-grained sand-stone, yellow-grey on the inside and 
brownish on the outside, in which are found some fragments of 
stone-kernels of Hyolithus-shells. A few of these fragments are enti- 
rely dark-brown, others have a light-grey surface. One of the stone- 
kernels shows the transverse section characteristic of Hyolithus de 
Geeri. The Roden erratic-block is rather a large slab of sandstone, 
containing especially off-prints of pyramidal Hyolithus-shells. This 
one is reddish on the inside and light-grey on the outside. 

Where the sandstone-layers of which the Murmerwoude erratic- 
blocks in former times formed part, were originally found as firm 
rock, cannot be said with certainty, as appears from what was 
written above. Most probably it was near the western coast of the 
southern part of Sweden. 


HI. That the knowledge of our sendimentary erratics still leaves 
so much to be desired, must certainly be partly attributed to the 
fact that so few of them have been gathered up to this time. Non- 
geologists, too, by their researches, may deserve well of this branch 
of knowledge, as was proved once more by Prof. Dr. J. C. Kaprnyn, 
filling a chair at the Groningen University. 

This well-known Astronomer, who in summer lives at Vries, in 
the northern part of Drente, last summer searched the surroundings 
of this village for sedimentary erratic-blocks. To his researches we 
owe a piece that is certainly the most interesting of the erratics 
described here. 

Just outside this village, by the road leading to Donderen, was 
found a small, slab-shaped erratic-block three centimetres thick, the 
largest dimension of which is 14 centimetres. It consists of sandstone 
coloured yellow-grey by ferrihydroxide. At the surface it is brownish. 
With muriatie acid there is no effervescence. The grains of sand 


1) BONNEMA. De sedimentaire zwerfblokken van Kloosterholt (Heiligerlee). Versl, 
v. d. Koninkl. Akad. v. Wetenschappen 1898. p. 450. 

VAN CaLKER, Ueber eine Sammlung von Geschieben von Kloosterholt. Zeitschr. d. 
Deutsch. geol. Gesellsch. Jahrg. 1898. p. 234. 


( 566 ) 


are for the greater part very small; they are not easily distin- 
guished. Among them are bigger transparent ones. The diameter of 
these latter grains is at most '/, millimetre; they are mostly arranged 
in parallel planes, in consequence of which an indistinct layer-like 
construction becomes visible on the vertical sides. On one of the 
horizontal sides there are still parts of a few thin layers. In the 
stone are a great many small cavities, which were formerly evidently 
filled with organic remains. 

On both of the horizontal sides we find remains of Tribolites. On 
one of them the most important are an off-print of a mid-shell about 
8 millimetres long, and a stone-kernel 10 millimetres long, part of the 
shell of which, turned into iron-hydroxide, is still present. On the 
other horizontal side is found the front part of an off-print of a much 
larger mid-shell, which once had a length of about 15 millimetres. 

Undoubtedly these remains, which in many respects resemble each 
other, have come from the same kind of Tribolites. The two first 
mentioned are remains of younger individuals ; the other belonged 
to a more or less full-grown specimen. 

With the younger individuals the glabella was convex, its length 
surpassed its breadth a little, its breadth diminishing towards the front. 
On the front side the glabella is somewhat rounded. On the plaster- 
cast I made of the off-print of the small mid-shell, it is clearly visible 
that the glabella possessed at least 2 side-furrows on either side. The 
stone-kernel shows that the neck-ring was broadened in the middle. 
The cheeks were vaulted, which is very clear in the stone-kernel 
especially. Very characteristic is a deep furrow enclosing the glabella 
in front and being continued on either side on the cheeks, where it 
broadens and becomes less deep. Before this furrow is a vaulted part, 
which does not turn down. The front-edge of this part is on about 
the same level with the back-edge, whilst its height is equal to that 
of the glabeila. In the off-print of the little mid-shell the glabella is 
4°/, millimetres in length, and the part in front of it nearly 3 milli- 
metres in breadth. > 

It is apparent from the off-print of the mid-shell of the more or 
less full-grown animal, which mid-shell is only partly exposed to 
view, that the glabella and that part of the mid-shell which is in 
front of it, which does not turn down here either, are less vaulted, 
and that the furrow separating the two, is less deep. Here are no 
side-furrows to be distinguished on the glabella. 

With the assistance of the scientific works I dispose of, I found 
that these remains are most like those of Arionellus primaevus BRÖGGER, 
of which up to this time only mid-shells have been pictured and 


2 


(phe) 


described. The first pictures were given by Kaervrr *, after remains 
of the “er¢n skifer” from Tomten (TOmten?) in Norway. He informed 
us already that they came from an Arionellus-species. Later on they 
were described by BRÖGGER*), who by them was induced to assume the 
new species Arionellus Primaevus. Under this head he also ranged the 
mid-shell that had been pictured by Kaervrr in fig. 6. Afterward 
LaNNARSSON *) pictured and deseribed remains of this Tribolite. He 
moreover tells us that the mid-shell pictured by KJerunr as fig. 6 
rather seems to belong to a new species called Ellipsocephalus Nordens- 
kiöldi, instituted by him in the same essay. His material had been 
got from the “egrivacke-skiffern” of Forsemölla near Andrarum. He 
dared with certainty to range under the head Arionellus Primaevus 
a small mid-shell 5 millimetres long, which had been found in a 
sandstone-like variety of the stone mentioned above. This was not 
the case with mid-shells from the ordinary stone, which are about 
15 millimetres long. He gives as his reasons for not daring to range 
these latter among Arionellus Primaevus BRÖGGER: first that they are 
much flatter, secondly that the furrows are much shallower, thirdly 
that the glabella has no side-furrows, fourthly that the glabella 
towards the front considerably diminishes in breadth. Why, notwith- 
standing all this, he at first ranged them under this head, though he 
had never heard of transition-forms, he explains by saying that 
BARRANDE had found exactly the same difference between the old 
and the young specimens of the Bohemian species’ Arionellus Cetice- 
phalus Barr., of which transition-forms are known. 

The very same points of difference occur in the Trilobites-remains 
of the erratic-block found at Vries. Here, however, the glabella of 
the older specimen does not diminish in breadth more considerably 
than that of the younger individuals. 

_ As I wished to be as certain as possible in my determination, I 
wrote to Prof. Mosrre, director of the Geological Institute at Lund, 
to ask whether there was any material for comparison at my disposal 
there. Remains of this species of Trilobites seem to be very rare at 
Forsemölla, however, so that my request could not be complied with. 
I received as a present, however, a mid-shell of the Ellipsoeephalus 
Nordenskiöldi, which seem to occur more frequently there, Prof. 


1) Kserutr „Sparagmitfjeldet”. Universitetsprogram Kristiania. 1872. p. 81. Vig. 
7—9. 

2) Bröeerr, Om Paradoxidesskifrene ved Krekling. Nyt Magazin for Naturviden- 
skab. 1878. Bd. 24. p. 58. 

5) Linnarsson, De undre Paradoxideslagren vid Andrarum. Sveriges geologiska 
Undersökning 1882. Ser. C. NO, 54. p. 21. Taf. IV. fig. 3, 4. 


( 568 ) 


Mosere supposing that my Trilobites-remains would prove to belong 
to this species, which is not always to be distinguished from Arionellus 
Primaevus. 

Indeed, I had been thinking of this species, but as Linnarsson declares 
that here the vaulted part of the mid-shell before the glabella towards 
the outside slopes strongly down, I thought I could not range my 
remains under this head. The mid-shell I received from Lund con- 
firmed my opinion. | informed Prof. Moprre of this and sent him a 
few plaster-casts of the Trilobites-remains occurring in the erratic- 
block found at Vries. I was answered that Prof. Mosrra shared my 
opinion and considered them as having come from Arionellus Pri- 
maevus. At the same time he was so kind as to send me a plaster- 
cast of the best of the mid-shells of this species of Trilobites, found in 
the collection at Lund. Now I could ascertain that in Arionellus 
Primaevus the part of the cephalon in front of the glabella does 
not turn down, which is not specially mentioned by Bröcerr and 
LINNARSSON. 

Also in the mid-shell of which MoBrre sent me a plaster-cast, the 
breadth of the glabella diminishes but little towards the front, though 
its length is about 14 millimetres. 

I think, then, that we now may with certainty conclude, that in 
the Vries erratic-bloek we find remains of Arionellus Primaevus 
Bröecerr. As this Trilobite occurs only in layers that contain remains 
of Holmia (Olenellus) Kjerulfi Linrs, and as these are taken to be 
the youngest of the Under-Cambrian ones, the age of the layer of 
which this erratic-block in former times formed part, may be easily 
determined. 

Besides occurring at Tömten in Norway and at Forsemölla near 
Andrarum in Schonen, which places I mentioned already, Arionellus 
Primaevus is probably found in two more places in firm rock, viz. 
at Kiviks Esperöd to the North and at Gislöfs Hammar to the South 
of Simrishamn in Schonen. The former place was first made mention 
of by Narnorsr *), who told that he had found there an off-print of 
an Arionellus? That in Gislöfs Hammar remains of an Arionellus 
occur, was first communicated to us by Luynarsson, in his description 
of the Arionellus-remains of Forsemölla. According to this writer, 
many of the mid-shells found there by von SCHMALENSEE much 
resembled the larger shells of Forsemölla, which he dared not with 
certainty call Arionellus Primaevus. 


1) Narnorst. Om de kambriska och siluriska lagren vid Kiviks Esperöd etc. Geol. 


Föreningens 1 Stockholm Förhandlingar. Bd. 3. 1877. p. 264. 


As for two kinds occurring in the same place, Horst *) mentions 
that the “grivackeskiffer” may also contain a species of Arionellus 
(Arionellus Primaevus BRÖGGER °). 

From communications made by TerrBere ®) and Hennig *) the 
conclusion might be drawn that Arionellus Primaevus Broee occurring 
at Kiviks Esperöd and Gislöfs Hammar, had been sufficiently indi- 
eated. I think, however, that this should not be done. The list of 
fossils which these two authors have drawn up with regard to 
the “eravackeskiffer” of the two places mentioned just now and of 
Andrarum, must refer, in my opinion, to these places taken collec- 
tively and not to each separately. L am confirmed in this opinion 
by the fact that remains of Holmia Kjerulfi Linrs (or of a kindred 
species) are not mentioned by Moere *) as being found at Kiviks 
Esperöd, whereas they are mentioned by them. 

The origin of this erratic-block must most probably be looked for 
in the eastern part of Schonen or in the Baltic Sea-region bordering 
on it. That petrographically it ‘differs from the ordinary “gravackes- 
kiffer”, does not clash with this opinion, several writers informing 
us that the latter often changes into sandstone. The thin layers on 
the lower side indicate that something of the kind has been the 
case here. 

It is not likely to have come from Norway, for never was a 
sedimentary erratic-bloek found in these parts, of which this may 
be said. 

As was mentioned above, I take this erratic-bloek to be the most 
interesting one of the pieces that are described in this paper. | 
do this because it is the first piece coming from layers with 
Holmia Kjerulfi Linrs that has ever been made mention of. Nowhere 
in literature did I find anything about an erratic-block of that age. 


IV. Shortly before the summer-holidays of last year | found, when 
visiting the loam-pit close by Hemelum, a slab-shaped piece of fine- 
grained sandstone three centimetres thick, whilst its largest dimension 
is a little more than 20 centimetres. It is layered and contains 
calcium-carbonate, so that with muriatie acid it gives effervescence 
of dioxide-carbonate. 

Owing to the large number of Glauconite-grains it contains, the 

1) Horst. Beskrifning till kartbladet Simrishamn, p. 17. 

*) TuttBere, Skanes Graptoliter. I. Allmän öfversigt öfver de siluriska bildingarne 
i Skane och jemförelse med öfriga kinda samtidiga aflagringar. Sveriges geologiska 
Undersökning. 1882. Ser. G No. 50. p. 26. 

5) Hennie, Geologischer Führer durch Schonen. 1900. p. 26. 

4) Mopere, Sveriges älsta kinda Trilobiter. 


( 570 ) 


stone of which this erratic-block consists is coloured a strong green. 
This is the case with some layers especially. Some particles of a 
light-coloured kind of glimmer are found in it. 

My attention was drawn to this kind of sandstone, because, when 
splitting this erratic-block into two parts, I found that it contains 
Hyolithus-remains, viz. grey-coloured stone-kernels. The lower part 
of one of them is brown. 

When visiting the Natural History-Museum at Hamburg last sum- 
mer, and admiring its collection of sedimentary erratic-blocks, I asked 
Prof. Gorrscne whether he knew of suchlike erratics. Prof. GOTTSCHE 
thought he remembered such pieces to have been found in the sur- 
roundings of Hamburg. Owing to want of exposing-room, however, 
they lay packed up among other pieces, in consequence of which 
they could not be shown me. He drew my attention to the fact that 
in this kind of erratic-blocks sometimes occur small conical valves 
of horn-shelled Brachiopodes. These valves were shown to me in a 
brown-coloured erratic-block. 

A short time after I found on the beach at Borgholm in Oeland 
not only an erratic-block with Hyolithus-rests entirely corresponding 
with my Hemelum piece, but also a brown piece of sandstone with 
a valve of a small horn-shelled Brachiopode. 

I searched my books for anything on the subject of this kind of 
erraties or stone, but at first without any result. 

As Prof. MoBrrG at Lund in the summer of 1901, when I had 
requested him to be so kind as to give me some information con- 
cerning Oeland, had noted down on my map of this island that on 
its coast, to the North of Färjestaden, occur erratic-blocks with Dis- 
cinella Holsti (then unknown to me), and the valves of Brachiopodes 
I had found were, like those of Discina, horny and flat-conical, but 
much smaller, I supposed that Prof. MoBerG could give me some 
information about this stone. For this reason I intended to write to 
him concerning this subject, and, was going to do so, when acci- 
dentally I discovered in the essay of Hora *) on the Swedish Hyoli- 
thidae and Conulariidae, that by Moprre *) a greenish kind of sand- 
stone, rich in Glauconites, with Discinella Holsti Mosrre and Hyoli- 
thes, occurring as erratic-blocks in Oeland, had been described. 

Having studied Mogrre’s essay, ‘I find that the stone of which my 


1) Hor. Sveriges Kambrisk-Siluriska Hyolithidae och Conulariidae. Sveriges 
Geologiska Undersökning. Ser. CG. No. 112. 

2) Moperc. Om en nyupptäckt fauna i block of kambrisk sandsten, insammlade 
of dr. N. O. Hotsr. Geologiska Föreningens i Stockholm Férhandlingar 1902. 
No. 142. Bd. 14. Haft 2. p. 103. 


(OL 9 


erratic-blocks with Hyolithus-remains consist, has been described bv 
this author as type a. The piece of brown sandstone with the valve 
of a small Brachiopode I found at Borgholm, belongs to his type d. 
The fossil occurring in it has been determined by me as a vaulted 
valve of Discinella Holsti MoBrera. The erratic-bloek that was shown 
me by Gorrscur probably belongs to the same type; the organic 
remains occurring in it are likely to have come from the same 
species of Brachiopodes. 

The Hyolithus-remains in the Hemelum erratic-block have been very 
imperfectly preserved, which, according to Horm, *) is usually the 
case with this stone. A longitudinal section possesses a length of 10 
millimetres and at the mouth a breadth of 4 millimetres, so the 
dimensions of this shell remind of the one pictured and described 
by Mosrre’) under the name of Hyolithus Insularis nov. spec., 
whereas Horm afterward called it Hyolithus Confusus nov, spec. 

The relative age of this kind of erratic-blocks does not seem to be 
with certainty known yet, as up to this time no corresponding stone 
has been met with as firm rock, and the organic remains found in 
them have not yet been discovered in company with such as might 
contribute to the solution of this question. MoBrere, however, thinks 
he may conclude from the general character of the fossils oecur- 
ring in them, from their petrographical nature and from the way 
in which they are spread, that they come from Under-Cambrian 
layers. 

Horst *) draws the same conclusion, after tracing the manner in 
which they are spread. I think I may infer from his essay, that in 
his opinion they come from the youngest Under-Cambrian layers. 
In accordance with this is the presence of Discinella-remains, this 
genus of Brachiopodes occurring, according to Mosrre, in North- 
America, in layers containing Olenellus. 

As was said just now, a corresponding kind of stone was not yet 
met with as firm rock. Most probably it formerly occurred west- 
ward of Oeland; it may be found there even now at the bottom of 
the sea, because this kind of erratic-blocks is found in large num- 
bers only on the western coast of this island, between Halltorp and 
Mörbylânga, and on the little isles and cliffs in the neighbourhood. 
Less numerous they are in the other parts of the eastern and western 
coasts of the Kalmarsund. 


1) Hou loc cit. p. 74. 

2) Mopera. Om en nyupptäckt fauna i block of kambrisk sandsten ete. p. 117. 

5) Horsr. Bidrag till kännedomen om lagerféljden inom den kambriska sand 
stenen, p. 9. 


( 3725 


MosrerG says that these erratices were found by Dr. Horst on 
Bornholm, too. Neither in German nor in Dutch literature have [| 
been able to find anything concerning suchlike erratic-blocks. It is 
almost doubtless, however, that they are mentioned by Gorrscam *) 
as “Cambrische Grauwackeschiefer’”. Only those erratic-blocks which, 
according to him, resemble the Swedish “Gravackeskifer”, must be 
taken into consideration then. The description of the latter entirely 
corresponds with that of type a by Mosrre. The small, round, 
horny-lustrous Brachiopodes-valves with a diameter of 2 millimetres, 
mentioned by Gorrscue, which may come from Discinella Holsti 
Mosere, also cause us to conclude that we have the same kind of 
stone here. Gorrscur does not inform us of Hyolithus-remains occurring 
in suchlike erratic-blocks. No erraties containing them had perhaps 
been found at the time. It follows from what he orally communi- 
cated to me, that now they have most probably been found. 

The same author says that according to LINNARSSON a kind of 
stone entirely corresponding with the one deseribed by him, has 
been met with by Hummer near Tereskov (wich HumMet calls Torekov), 
on the coast of N. W.-Schonen, as firm rock. Judging from the 
description Hummer *) gives of it, it much resembles, petrographically, 
type « of the Discinella Holsti-sandstone. Hummer does not say, 
however, that fossils are found in it. Perhaps we have here 
the same case as with the Glauconitic sandstone from the neigh- 
bourhood of Simrishamn, of which Horsr®) writes that a corre- 
sponding kind frequently occurs in the “sandstone-region” of the 
Kalmarsund. Here, too, the resemblance seems to be petrographic 
at best, for Mopere, in his essay, speaks about this sandstone no 
more than about that of Torekoy. | 

Most probably the thin-layered, greenish stone which resembles 
the “Grauwacken-Schiefer” of the Olenellus Kjerulfi-region, and 
whieh petrographically keeps the medium between the Olenellus- 
stone of Hardeberga in Schonen and the equally old “grén skiffer” 
of Bornholm, with stone-kernels of a Brachiopode probably belonging 
to Acrothele, and with Hyolithus-remains bearing the greatest resem- 
blance to Hyolithus Lenticularis Holm, as SroLLry *) writes, — is 
also Discinella Holsti-sandstone. 


1) Gorrscue. Die Sedimentiir-Geschiebe der Provinz Schleswig-Holstein. 1883. p. 8. 

2) Hummer. Beskrifning till kartbladet ,Bastad”. (No. 60). Sveriees geologiska 
Undersökning. 1877. p. 10. 

3) Horst. Beskrifning till kartbladet Simrishamn. p. Lo. 

4) Srorrey. Die cambrischen und silurischen Geschiebe Schleswig-Holsteins. Archiv 
fiir Anthropologie und Geologie Schleswig-Holsteins und der benachbarten Gebiete. 
1895. Bel. Hett. asp. 130: 


‘ied 
7 . 


(573) 


Finally I must mention that, on the occasion of a later visit to 
the loam-pit near Hemelum, I found two more erratic-bloeks, which 
must probably also be counted among pieces of Discinella Holsti- 
sandstone. Neither contains any fossils. One corresponds petrogra- 
phically with what was described; the other is for the greater 
part white, but possesses green layers. If I am not mistaken, 1 
sometimes saw suchlike stones on the beach of Borgholm. 


Physics. — “On the course of the values of b for hydrogen, in 
connection with a recent formula of Prof. vaN pur Waars.” 
By Dr. J. J. van LAAR. (Communicated by Prof. J. D. vAN DER 
WAALS). 


1. Making use of the theory of cycle motions, Prof. vaN DER 
Waats has given a new deduction of the equation of state of a 
simple substance, in which the size of the molecule appeared to be 
variable, and to be a function of the volume *). 

For a bi-atomic gas the following formula has been found: 


b--b, bb, \? 
—=—1— ES ee ENE EE ey 
v—b bod, 

Here }, denotes the smallest value of 6, corresponding to the case 
that the two atoms of a molecule touch each other; 4, represents 
the greatest value i.e. the value for very great (infinitely great) 
volume. The above equation may be easily derived from the so 
called “equation of state of the molecule” 


vti te et) |b) = FEISS ASS: ways ke aT 
yt 


when we take »—=o, in which case / assumes the value 4, and 


a P 
jae De may be neglected with respect to a (b—b,)- So we get: 
t 


a (6,—6,)’ =A. 


If we substitute this value into equation («), paying regard to 


we get the equation 


1 sf b—b, (ne 
—__—— I — 0s) ==, 
(ea b (bg—,)? 0, , 


which yields immediately equation (1). 


1) These Proceedings of the meetings of February, March and April 1901, 
See also “Livre jubilaire dédié à J. Bosscua” of the Arch, Néerl., p. 47, (The 
first communication and part of the second discuss principally the specific heat 
for very large volume). 


The quantity « in the equation of state («) depends on the forces, 
which keep fhe atoms together in the molecule. These forces are 
supposed to be proportionai to the linear deviation from the position 
of equilibrium 7—7,. 

The equation of state («) for a tri-atomie gas, e.g. CO, — which 
in this case is the combination of two similar equations — will con- 
tain besides RT still a factor f, whose value will vary from 1 to 2 
according as the different cases occur, which we may distinguish in the 
motion of the atoms. For CO, a value of nearly 2 is found for /. 
As, however, this quantity f for a certain substance is, strictly speaking, 
variable (see the paper in the “Livre déedié à Bosscra”, quoted above) 
and as the accurate equation is therefore very complicate, I have 
chosen a bi-atomic gas, namely hydrogen, in order to test the new 
equation of van DER Waats. In this case f= 1 and the relation 
between 4 and v is represented by the simple equation (1). I hope 
later to test the equations for oxygen and nitrogen, in order to 
examine whether the results found for hydrogen also hold for these 
gases. 

Il. An accurate knowledge of a is required for the exact calcu- 
lation of 5. This is still a great difficulty. Absolute certainty as to 
this value cannot be obtained as yet, but still it appears to me that 
the value a=30010~-6') has a high degree of probability. Assu- 
ming another value for a, I found namely that the values calculated 
for 6 decrease much too rapidly, — much more rapidly than agrees 
with formula (1); this is principally the case in the beginning, 1. e. 
for large values of v. Only the values of 5, calculated for a=30010~6 
varied in such a way, that their course was represented by equation 
(1) with nearly perfect accuracy. SCHALKWIJK *) also calculated from 
his last experiments 10° a = 300 (10° 4, = 910). I therefore thought 
myself justified in assuming 300 for 10° a. In the following table 
we find the values for 4 at 0° Centigrade, calculated from the equation 


(0 + 5) (v—b) = (1 + a) (AB) (Lat). 


For (1+a) (1—+) we put 0,9994. All values have been multiplied 
by 10°; the same will be the case with all values of 6 which we 
give in what follows. 

At 0° C. we have: 


0,9994 


a 
p+ ae 
1) All values of v, b, etc. have been expressed in the usual practical units. 
2) These Proceedings, June 1901, p. 124. 


n= 


a b b 
p pl) p2 - v—b calculated A 
oF found. — from (1) | 
100 | 40690 | 414.3 9.6* | 9739 | 951 907 | 444 
150 | 7353 54 07 5.5 6425 | 998 901 | 427 
200-5690 32.38 gor.) ar. | ois" | 396 >} HAT 
250 | 4692 | . 22.01 PFGE mt ad oI Sots ny =i 
300 | 4030 16 24 18.47 3138 892 | 886 Je 
350 3560 12.67 23.65 Dei sist Sho, RE: UM EEn 
400 3207 10.28 929.48 9329 SAS si 075 aE 
450 2933 8.602 | 34.87 2061 SUL, aes «(Und PS ae 
500 2713 7.360 40.8 1S4S 865 | 865 + 0 
550 9533 6.416 16.8 1675 858 | 860 = 
GOO IBR6° 5.695 apel | 153 855 855 td, 
650 9959 |. ~ 5:408 58.8 1410 Gay | Sa bP 
700 | 2149 | 4.60 | 64.9 1307 | 843 om | = 9 
750 | 2053 | 4.215 74.2 1217 836 | 840 ed 
800 1971 3.885 17.2 1139 832 | 835 8 
850 1897 3.599 83.4 1071 826 830 4 
900 18335 3.362 89 2 1010 823 826 9 
950 1774 3.147 95.3 956 818 | 82a 8 
1009 17225 9.967 | 101.4 | 908 815 817 i 
1100 1637 2.680) 414.9 | ~ 825 812 809 + 3 
1200 15575 9465 123 7 757 SO 801 Ee! 
1300 1491 93995") 135.0 696 795 793 +2 
1400 1432 24051 463 646 786 785 +4 
1520 1380 4.904 | 156.3 603 777 777 +0 
1600 | 1334 1.781 | 168.4 565 769 770 | 
1700: je 429% 1.681 1785 532 762 763 — Á 
1800 | 4958 1.583 4189.5 ‚02 756 756 + 0 
1900 1225 1.501 | 499.9 476 749 749 0 
2000 11945 1.497 | 40.2 152 742 743 = 4 
2100 1166% | 1.361 | 290.4 431 736 736 +0 
2200 Mal 1.302 | 230.4 “11 730 730 ae 0 
2300 1148 {4.250 | 240.0 393 ip a EE an de 
2400 10972 1.205 249.0 377 720 149 A4 
2500 1078 4.462 | 258.2 362 716 714 hy 
2600 1059° 1.423 | 267.4 | 349 714 710 4 
2700 1042 1.086 | 276.2 S36 fst 706 705 + 4 
2200 102° 1.050 |. 285.7 324 701 700 | +4 


1) Up to 1000 atmospheres the values of ¢ have been borrowed from the results 
of the “second method” of Amacar (méthode des regards); from GOO atm. to 
og 


Proceedings Royal Acad. Amsterdam. Vol. Y, 


The values of v have been borrowed from the well known expe- 
riments of AMAGAT *). 

The too large values of 5 in the beginning — here only to about 
300 atm. 
a = 300 is still slightly too great. But from 300 atm. upwards the 


are still present. This indicates probably that the value 


agreement is quite satisfactory. Small inaccuracies in the determina- 
tion of the value of r have for large volumes a great influence on 
the values of 4. To this circumstance also it may be ascribed that 
the values of 5 are in the beginning not reliable. So the value 
v= 10690 at p= 100 cannot be accurate to a higher degree than 
to ten units at the utmost. So it might also have been 10680 or 
10670 and 6 or r — (v—+) might have been 10 or 20 units smaller. 
The values of 4 “calculated” have been determined with the aid 
of equation (1) in the assumption 


by 917 ; 0, = 463. 


4, may be determined in the following way. If we substitute 
into (1) 


bb, 
— — — WwW, 
bg—b, 
dl 
and pay regard to b—b, = aes (4,—b), then we get for (1): 
— . 
Pen 
Sr nb : 
and therefore : 
b,—b 12 
fe eg) 
rb a 


For an assumed value of 4, this equation enables us to determine 
the corresponding value of . from v and 5 at e.g. 500, 1000, 1600, 
2200, 2800 atm. The value of 4, may then be calculated from 


b, = b — (1 —a’) wv —b), 


which follows immediately from (1). So I found with 6, = 917 at 
1000, 1600, 2200, 2800 atm. respectively the values 4,= 455, 463, 
462, 466. If we put a—400 instead of a—300, then we find with 
6b, = 1000 at p= 2800 atm. in the same way b,— 468. With 
1000 atm. the values of v at 600, 700, 800, 900 and 1000 atm. represent the 
mean values of the results of the first method (that of the electrical contacts) 
and those of the second method. From 1100 atm. upwards the values of v have 
been determined by the first method. 

1) Mémoires sur l’élasticité et la dilatabilité des fluides jusqu’aux très hautes 


pressions, p. 32—33 and 38, 


( 577) 


a= 500, 6, = 1100 we find at 2800 atm. again 6, = 464. So we 
may assume with perfect certainty 4, to differ very little from 463. 

With this value of 4, in the first place 4, was again calculated. 
From (1) follows: | 


(Lb) bb (v—b) poe (4—b,) 
OB ay y—b Pee kek: 


SO 


En ee ee (ee 
Ee eat LO ECN 


In this way I found at p==500, 600, 700,-800, 900, 1000, 1200, 
1400, 1600, 1800, 2000 atm. respectively Gj =— 919: Toe Opa 
912, 913, 919, 917, 917, 917 917. From these values I concluded 
that b, = 917. 

After that the values of 4 (calculated) were determined as follows. 
We derive from equation (1): 


b—b, (bb) 
a a en ae a 
If we put bb, = y, then we get for 6,—b, = 454: 
y y 
el) y ABP 


from which follows: 


DE ea 
RE pe iel 
‘ (v—b,) ee 


We know the values of 4 already in approximation from / (found). 


These values, substituted into the second member of the above 
equation, yield the accurate value of y, and so also of 5. 


HI. Let us begin with assuming that the values of 4, and 5, 
are independent of the temperature, which follows from the supposition 
of Prof. var per Waars, that the quantity «‚ which depends on the 
forces between the atoms, is proportional to the absolute temperature. 
Then we may calculate the critica’ quantities in the following way. 
Equation (1) in connection with the following equation : 


==> a= a or 0 -— 0 pa em ). 
+2(8,+8,) 3 Shai 
where 


39% 


yields after some reductions *): 


{a 1—w\' 
3 Pan ee 


en 5 — (1 —)? 2 


2 b 
Here is 7 = (=) and u Sar . We may write for the 


Jg — 9% 


bo | 


second member: 
2(143 a?) 
(1 +2) (2—a-+ 2)? 


Therefore we get also: 


5 L WW 3(1+.w)(2—a+a’) 
Dl HU = — —_ eae ees Pare oe ) 
Ve 4 1434" ”) 
The value of « may be derived from this equation. As 6,=917=1,986,, 
1 : een : 
u gets the value = 1,02, and we find in approximation for « 
the value 0,709. 
Therefore 
by—b, - 
—— — )Y JV,/ 09 = 0.842. 
pry 


from which we may easily derive: 
by ZOZ = 845. 


Now we have: 
3 vb 2(14 3.7) 
Rn Ree 
from which we find: 
. OE == dot bkr Be + B, — 0,0837. 
The critical volume is therefore: 


TNB De Deg END Vie 2172. 


— 0,9163, 


At 0° C. this volume is (comp. the table) already reached at a 
pressure of about 700 atm. The values of v at O° range in the 
experiments of AmaGat to 1025; the verification of equation (1) of 
VAN DER WAALS may therefore be extended over volumes which have 
the size of liquid volumes; this fact compensates the want of experi- 
ments below the critical temperature. 

We may also calculate the quantities 8, and 8, separately. From’) 

1) See v. p. Waats, l.c. ILL, p. 652. 

1) van DER Waats, Lc. III, p. 651, 


| (lx)? 
Br Ite Arda? 
1+ —— 
(lx)? 
follows: 
S= 030472. ; B, = 0,0365. 


We find for £7}: 5) 
8 a (L—8,—B,)'\1+2(8,+8,)) 


Re 


AAT by 18, 
or 
8 a 0.8396 «1,1674 Al 8 a a @ 
lg DE e000, 805 =. 
re acy 2 0,9528 27 by by. 
With a = 300, bj, = 845 we find therefore: 
ee Tr 
AT — (7.9994 —— = 0.108. 
273 


which gives: 
LG — 29°.5 ; 
Dewar found 7), = 30° 4.32°*). 
The critical pressure is represented by *) 


Eel ada ae 


= 
ie 27 bj? 1—8, ; 
or 
js) 0,8068 & 1,363 3 i ays: Sa Gf 
en Pe = 1,154 X — — = 0,0427 —. 
PW A) Pa 0,9528 BO by? 


Introducing into this expression the values of @ and bj, we find: 
pe = 18,0atm. 
Dewar found 15,4 atm.; Onzewski *) 20 atm. 
We find for the so called critical coefficient Y: *) 


, pv 3 Les 
ee ee Cr EE 
RT}; 8 (ll) 


x 2 ee En 0.961 0.360 
A = — K ——— ZZ Oe == UNE 
8 x 0.8396 5 x —_ 


Finally the quantity } may be calculated from *) 


or 


1") Id. II, p. 583. 

2) Proc. Royal Inst. 16 (2), N°. 94 (1901), p. 477. 

5) ven. Waars, l.c. II, p. 583. 

+) Wied. Ann., 56, p. 133 (1895). See also Verscuarrert, These Proceedings, 
Febr., 1899, p. 327. 

5) v. p. Waats, l.c. II, p. 584. 

6) Id. III, p. 648. 


( 580 } 


Pd 13 —8, 0,9165 . 
VE (5 7) == 4 SS Ax ——_ = 4 1,136 = 4,945. 
bat de 0.8068 


Just as VY comes again very close to the normal value 0,375, so VY 
for hydrogen approaches again close to the theoretical value 4. The 
expressions for 7, and py, differ only little from those, found for 
these quantities for tri-atomic gases, such as CO,; the expression for 
vy, on the other hand deviates strongly from it. This is to be ascribed 
to the fact, that 4, has here not the value of nearly four-times 4,, but 
amounts to only twice that value. The quantities >, and 3, are there- 
fore much smaller than in the case of tri-atomic gases. 

VAN DER Waats found for CO, e.g. B, —= 0,138 and 6, = 0,1, the 
values we found above amounting to only about one third of these 
values. bj is also in this case not 0,86 6, but 0,92 6,, and for vo we 
find 2,57 by, instead of 2,03 6;,, or 2,376, instead of 1,75 dy. 

It is certainly of the highest importance to know whether the 
result for vj agrees with the experiments. At the same time the value 
of the critical coéfficient will then agree, for the values of 77 and 
pe agree very well. But with the investigation of this question, and 
with the verification of }, we will wait till we have investigated 
the behaviour of 5 at higher temperature, which will be done in the 
next chapter. 


IV. In the first place we will repeat the calculations of § 2 at 
99°,25 C. We derive the following table (p. 581) from the expe- 
riments of AMAGAT') at that temperature. 

rh has here been calculated from 


0,9994 (1 + 99,25 x 0,0036627) 


(bl == 


For the “calculated” values of 4 I determined quite in the same 
wav as is indicated above for O° 


by SN A b, =S eed) 


Again the initial values of 6 “found” (up to about 400 atm.) are 


too great. But afterwards the agreement is sufficient, though the 
verification was only possible up to 1000 atm, as, alas, no further 
experiments were available. We come to the remarkable result, that 
the value of 5, has considerably decreased though the limiting value 
of 6 has remained unchanged. It seems that at higher temperature 
the atoms in the molecule may approach one another closer than at 
lower temperature. 


1) Le. p. 38 (2nd method). 


p | r | v? | 5 el | ; Bd | A 
| | | | | found from (1) | 
150 9846 | 96.94 | DROS | 8902 | O44 | | 
: Qs |  96.§ | ae | &902 QA. 902 | +42 
200 7567- | 57.26 | 5.27 | 6640 27 | 897 | +30 
250” | 6200 | 38.44 | 7 g0 | 5286 14 | 8 | 499 
300 | 5286 | 27.94 Mene | AA8ne PC 001” | - 887 | 4414 
350 | 4636 241.49 | 13.99 | 3744 | 802 | ga | 441 
A00 | 4447 17.20 Ee 889 — |)! 876 |, At g 
450 | 3766 | 14.48 | 91.4% | 9899 | 7) ee ay eel 
500 3462 | 11.99 25.0? | 2596 | 866 | 866 | 0 
550 | 3214 | 10.33 29.0 985307] Bals IN ‘ger ol er 6 
600 | 3006 | 9.036 | 33.99 | 9150 854 Bete ie 6 
650 | 284 | 8.015 | 37.0 | 1983 | ss | em | —3 
700 | 2680 | 7,182 | 41.8 ABT Se es 273 
ue aaneen che. WE: | 4710 [---839 | - 84 Mees 
800 | 2436 | 5.934 | 50.6 | 1602 | 834 | 836 ae 
850 | 2336 | 5,407 Eken dsc, ERD | 831 Kad 
900 one | 5036 | 59.6 |“ 1490 | son | gar | sets 
1950 | (2174) | 4.796 | 63.5 1345 IBD gaa | — 
1000 | 2093 | 4381 | 68.5 | 1975 | BI ie len 


| I 
From equation («) follows that for great volumes: 


« (bg—b,)? = RT. 
Now we find: 
OP by—b, = 454 (6,-— 5, )? ==.20,61, x10" 
1000 | tl == Oe EP 

(bb)? has therefore increased in the ratio 1 :1,368. But 7’ has 
increased in the ratio 1 : 1,364, from which would follow that « is 
independent of 7. 

In order to investigate whether this also applies to still higher 
temperatures, I have also performed the calculation for 200°.25. 

rh may then be calculated from: 

0,9994 (1 +200,25X0,0036627) _1,7324 


Di 0 Maree 


a 


') The value given for ¢ at p=950 atm. appears to be erronious; probably 


(Se) 


With the aid of the following table we may survey the results. 


200° EC. 


2 L y 


p p r | eb 
| found calculated 
en | 
150 | 19390 | 451.78 | 1.98 | 11399 921 894 +97 
200 0420 88.74 | _ 3.38 | 8518 902 ji 889 | HZ 
950 | 7680 58.98 5.09 | 6791 8x0 884 | 45 
| 
300 | 6520 42.51 7.06 5642 878 BO 
350 5694 SN) 9.95 1829 872 873 | —1 
A00 5075 TS) 4165 4208 867 SGS — 4 
450 1503 21.10 14 22 3732 861 863 |. —2 
500 | 4210 17.72 16.93 3351 859 858 ze 
550 | 3891 15.44 19.82 3040 851 GENE 
600 | 3627 | 13.46 | 922.80 2782 845 OE Nae 
650 3403 | 41.58 25.91 9563 840 843 ag 
700 | 3211 -| 410 31 29 10 2376 835 838 Zee 
750 | 3045 | 9272.) AAG We S914 831 833 ee 
800 | 9900 | “8.410 | 35.61 2073 827 828 nee 
850, | 2772 | 7.684 | 39:20 1949 823 823 Jt 
0900 9657 7.060 12.5 1838 819 819 +0 
| 


Only at 150 and 200 atm. the values for 4 “found” are somewhat 
foo high: furtheron the agreement is satisfactory. The experiments 
ranged ouly to 900 atm. The values of 4 “calculated” have been 
determined from (1) with the aid of: 

h, in 6. = 306. 


by appears to be slightly smaller than at O° and 100°, but 4, has 
again strongly decreased. It is a remarkable fact that the decrease 
of 6, between O° and 99° amounts to 77, and that between 99° and 
200° to 80; so for each degree the same amount namely 0,8. 

As to b,—b,; we have now: 


0° by — br A (b,—6,)° =-20,61 
200° ren he Fe = BO sae 
The ratio of the values of (6,—6,) is 1,77. For 1+ at we find 


1,73. Taking for b,— 6, at 200° a value which is only 6 units 


( 583 ) 


smaller, namely 598, the ratio of the values of (b,—b,) would also 
have been found equal to 1,738. We may therefore safely assume 
that (b,—6)? is found to be accurately proportional to the tempera- 
ture within so large an interval of temperature as that between 0° 
and 200°, in consequence of which the quantity @ must be quite 
independent of the temperature. 

It is not astonishing that @ is independent of the temperature: 
the contrary would rather seem to be remarkable. Being induced 
to make this contrary supposition for the better agreement of the 

; Lf dp . e : 4 : : 
quantity ( ) for CO, with the experiments, Prof. v. p. WaAats?) 
p \dT)y 
immediately pointed out its astonishing character. 

We shall just draw attention to the following consequence of the 
fact, that b,—6, is proportional to V7. 

If we put: 

b,—b, = VyT, 
then equation (1) may be written as follows: 
b—bg+ V4 ie SE fad (b—b, + VyT) ae bg—b (b,—b)? 
Ln DIT 
With small value of 6,—6 and great value of v, we get approxi- 


mately : 
Vyl by—b 
(bj = Vyl 
therefore 
YT 
b,—b En 
2v 
et tert RT 
r being in this case approximately equal to „wesen: 
: 4 5 
en 
2R 
or 


tS by—y' Pa 
i.e. the value of 4 depends only on p and no more on 7 or 7, the 
value of 6, being nearly constant. The values of 4, calculated for 
the same pressures, have therefore the same difference whether the 
temperature be 0° or 200°. For we have: 
biel 55 jd (P.—P)- 
We found this fact affirmed in the above tables*). For the purpose 


DE es UL,» pe 646. 

2) L pointed this out already before in a paper in the Archives Teyler („Sur 
influence des corrections, etc.” (2) VIL, Bme partie, p. 26—27.) I tested there the 
b-values for hydrogen to an empirical formula of KAMeRLINGH ONNeEs. 


( 584 ) 


of a more direet comparison we collect the values of 5 for pressures 
differing each time LOO atm. in another table. 


L | b | U 
p | 
0e | 100° 200° 
= SE eee eee 
| | 
100 | 907 | ee pen 
| Ad) 
20 | 896 | 897 S89 
10 10 10 
300 R86 887 879 
| lf 44—| 11 
400 | 875 876 868 
10 10 10 
HOO S65 | R66 S58 
10 10 10 
600 855 | 856 848 
10 40 10 
700 845 S46 838 
AD 40 10 
800 835 | 836 828 
0) q 9 
900 826 827 819 
{) 9) 
1000 817 S18 = 


We see that the differences are the same. All the values of 6 at 
200° are 8 units less than the corresponding values at O° and at 
100”, because the value of 6, at 200° is 7 units less. But the course 
is always just the same. And as at a given value of p we always 
find decreasing values of v at increasing temperature, so the value 
of 6, must of course always decrease. 

From the above follows also, that we may determine 4, immediately, 
eg. adding 52 units to the values of 4 found at 500 atm., or 32 
units to that at 400 atm., ete. 

On the preceding reasoning we may base the following short 
calculation. 

At p,—p, — 100 the initial value of b,—b, amounts to circa 10 
a 11; we have therefore: 

u ee shia O,10a 3 dee 

2R 100 ne 

Therefore 

bb, VT = 10 VOT REED AE 


or 


De er eee 
So we have at 0° 10°(4,—6,) = 458 (found 454). 
At 100° we find 10°(,—,) = V 21><10'S<1,38627—=535 (found 531). 
At 200° we find 10°(4,—0,) = V 215<10*<1,7324=603 (found 604). 


(“ode 


V. A slight correction must of course be applied to the calcula- 
tions of § 3 in consequence of the variability of 6,—6, with the tem- 
perature. For the assumption that 4, remains constant pleads also 
the circumstance, that according to an observation of D. Brrrignor 
the experiment yields the value 2,93 a 2,98 for the ratio between 
the temperature at which a gas in extreme rarefaction follows the 
law of Borrr, and the eritical temperature; for which ratio the sup- 
position that 4, is constant over this large temperature interval *) leads 
to the value 2,9. If we assume this same supposition, we shall 
find 5, to be equal to. circa 920 also for the critical isothermal. 
But 6, will be found to be considerably higher than at 0°. We saw 
above that the difference amounts to 77 units for 99° difference in 
temperature. We shall therefore find 6, at — 242° C. from the equation : 

249 


b, = 463 + = X 77 = 463 + 188 — 651. 


If therefore we put 6, = 920 and 4, = 650, then in the first place 


by is no longer equal to 26,, but to: 


b, = 1,415 b,. 


The variability of 6 is therefore much smaller than at 0°, and in 
consequence of this the quantities B, and 8, will also be found to be 
much smaller, and the critical quantities will approach still more 
closely to the normal values. 


) i! 
rhe quantity « ——-— is here —_~= 2,41, and the value of 
6 Jo ),415 
b.—b,\ sf 
nj — of equation 4 ceases accordinglv to be 0,709, but becomes 
by —b, 2 we 
0,852. In consequence of this we find: 
brb, 


——==/ 0,852 = 0,928, 
bg 8; 


from which follows: 
bir = 0.977 hy = oo) 


For +, and for @, + 8, we find (comp. § 3): 
vy, = 2,87 be ; B, + B, = 0,0228. 
So we find: 
Ua, Of brl ==, 80 bo -— 5,9 bere 


a volume which is reached at 0° C. at a pressure of + 550 atm. 
The values of 8, and 8, taken separately are: 
Pi Pa | € 
(le) 5 
B, — a a 0,0117 ; B. en 0,01 EG 
dag OO ne 


1) Zie vaN peR Waats, l.c. III, p. 647. 


( 586 ) | 


Now we return to the experimental verification of vp. 
1 Gr. H, at 0° C. and 1 atm. occupying a space of 11127 cM°., 
S19 <K 10-* > 4112) hence she 


re is expressed in ccM°. equal to 257% 


x 


critical density is: 


tt = 38,70 


According to the theorem of the straight diameter of Marutas we have: 


d,+d, 5 1 si 
et -— = —— mn — f. 
dt. ces 


— 0.0348: 


which quantity g has been found by Youre and Marmas to differ little 
from unity for different non-associating substances. 
Dewar?) found the density of the liquid phase at the melting point 


of H, (16°,5) to be 0,086, so we find, neglecting the density d, of 


the vapour: 


0, 086 16,5 
Se ee == 0,468, 
di. jaye 
which yields for dj: 
0,086 DRE 
di = ——— = 0,0348, 
2,466 —_—- 


in perfect agreement with the value of d, we have calculated above. 


We now proceed to the calculation of the other critical quantities 
fg : B 
kes Dk X and ¥; 
We find for 7: 
8 a 9, 9549 1,0456 8.4 a 
x ; (ps = 02095 


es een — 1,010 x — 
oT hi 0.9883 SOF be be 


With « == 300, 4, = 899 we find therefore 


T;, 
0.9994 — — 0.100. 
273 


sO 


C= ede 


This value is somewhat too low; the experiment has yielded 


e= Be De 
We find for the critical pressure: 
i 0.9439 1,093 1 
akk EN Le == ODSB7 


Rr nen E : 044 X = 
OT bis 0,9883 27 by be 


1) 1. ec. bl. 477. Dewar finds the melting point to be 16° a 17°: the critical 
temperature to be 30? à 32° absolute temperature. [The density of the liquid 
phase at the boilingpoint (20° à 21°) has been estimated to be + 0,07, but then 


the vapour density may no more be neglected. ] 


( 587 


With the values found for « and 5, we get: 
pe = 14,4 atm. 


Dewar found + 15 atm. 
The critical coefficient VY becomes: 
VR ERN EN : 
== a x 0.9549 8 XxX 0,989 — 0,371, 


so nearly the normal value 0,375. 


jn T dp 
For Y={— : we find now another value than before. In the 
pdT/,. 


general expression *) 


ft Be ase dPy 7 Ph | db 
plat), ne les de 


B d db gl N dP, 
the factor of — is now no longer zero. For as on -= a(b—b,), we 
av av 
have: 
ao AAP Ib 
LT — = =a oll 
OT \ db dl 
as we found @ to be independent of 7, 4, on the other hand to 
db 


depend upon 7. We find therefore for the factor of —: 
av 


We have found above: 6,—b, = V7T, so b, =l a Wyt, and as 
6, has been found to be nearly independent of T, we get 


„db, pes 1 
ri ae = 5 Vy! = == 9 (6,—,). 


4 dh 
The factor of = becomes therefore : 


aU 
1 
c (0-1, == 3 nee ; 
and with 


BE Lt ag jet a\fv—b 1) 1 
ey Eh) Tie! (hy hy Tr Dn u? tas ay b— 5. 


1 1 b—d, 

— as according to (1) we have — ll — — =i 
= (by ij ETS v cag 

we get: 


1) v. p. Waats, |. c. III, p. 644, 


( 588 ) 
djb 1 h,—b, 
p+- | ie 
ye li b, : 2) b—b, 
noe : : on dp | ee db 
Phis expression for ( -— | becomes therefore, if we put ==: 
P d k dv 5 


EE) 
aa =( PRU ine or: ze 5 ay wars , 


This yields with the panies calculated above (see § 3) 


ily COLL Lhd ee et EL 1) Ee ay 
"== De 0,0 Wm == 
X 09439 |T i( SG yee ( 2 B49, 


= 4 1,035 4 0,0117 > 


< 0,747 & 0,45781, 
or 
FS 4°120 Ss 105064267 


T dp 
Finally we investigate, whether this value of © a may be 
pc 


brought into agreement with the few experimental data of Dewar. 
Dewar found namely (Le): 
Orle a ge Lait 


P= 30" 238 (apy = baten: 


The two data yield by means of the integral formula 


nep log = LE a 1) 
P di 
for f the value: 


5 nep log 15 ae v 7 
=— 2 == Net yn a tee were 7 . 
Les be FEE alerts 


tO 
ALE | 

according as we take 20° and 32° or 21° and 30°. The lowest 
value is 4,51, so still higher than the calculated value 4,27. We 
must further note that 20° differs comparatively very much from 7%, 
(being */, 7) and that therefore at 20° the factor f will certainly 
be found to be greater than near 7), hence 4,51 is probably too 
great. 

From the above we may in any case conclude, that the large 
extrapolation, by “means of which we have calculated the value of 
b, at — 242° from the values of 6 at 0°, 100° and 200°, really 


0 


yields the critical data with a sufficient degree of accuracy at 
least in so far as we may judge from the few data, that are available. 
Only Mis probably too low. 

We have reason to expeet a priori that the new equation, derived 


by van DER Waars for the variability of 6 with the volume, does 


(OB 


not represent the experimental data with perfect accuracy. For the 
correction, introduced before for the partial coincidence of the distance 
spheres has not been taken into account in the deduction of this 
formula. The quantity 6 in r— b for a monatomic gas, ec. e. 
mercury vapour, argon etc. would according to the new theory of van 
DER WAALS remain invariable; whereas this quantity which according 
to the former considerations would for very large volumes be equal 
to four times the molecular volume, for smaller volumes would 
certainly have a smaller value, and it would approach to about twice 
the molecular volume — at least if the shape of the molecules does 
not exercise any influence on this calculation. 


Physics. — “Peculiarities and changes of Fraunhofer lines interpreted 
as consequences of anomalous dispersion of sunlight in the 
corona’ by Prof. W. H. Junius. 


(Communicated in the meeting of February 28, 1903). 


Especially by Jrewerr’s investigations on the coincidence of solar 
and metallic lines *) attention has been drawn to several variable 
peculiarities of Fraunhofer lines. Here we do not mean the irregu- 
larities occurring in the spectrum of spots or of faculae, which relate 
to disturbances in comparatively small parts of the sun, but abnor- 
malities shown by the average sunlight, as observed when the slit 
is illuminated by a long strip of an imperfectly focused solar image. 
In that case, according to Doppier’s principle we may, of course, 
expect displacements of the lines in consequence of the Sun’s rotation, 
of the rotation of the Earth, and of the change in the distance between 
Sun and Earth caused by the exeentricity of the Earth’s orbit. But 
even when all these influences have been allowed for, some irre- 
gularities still remain. 

Indeed, Jrwerr has observed that some Fraunhofer lines do, others 
do not, exactly coincide with the emission lines in the are spectrum 
of elements, and that the displacements are unequal both for lines 
of. different elements and for the various lines of one and the same 
element. Moreover, the shifting of certain lines on one set of photo- 
graphic plates was sometimes found different from that on a set of 


DL. E. Jewett, “The coincidence of solar and metallic lines. A study of the 
appearance of lines in the spectra of the electric are and the Sun.” Astroph. 
Journ. Il p. 89—113, 1896. The same: “Spectroscopic notes. Absolute wave-lengths, 
spectroscopic delerminations of motions in the line of sight, and other related 
subjects.” Astroph. Journ. XI p. 234—240, 1900, 


( 590 ) 


plates taken at another time. With several lines the intensity too 
appeared to be variable. 

JEWELL explains these phenomena on certain hypotheses on density, 
pressure and temperature of the absorbing and emitting gases in the 


different layers of the solar atmosphere, and by variable ascending 


and descending velocities of matter. 


Harr’s abnormal solar spectrum. 


Much greater than the irregularities mentioned are those, found in 
an “abnormal” solar spectrum, lately described by G. E. Hare. *) 

This highly remarkable spectrum had accidentally been photographed 
as long ago as February 1894 in a series of exposures made with 
the sole intention of investigating the peculiarities of the grating. 
Only a few months later it was discovered that a very extraordinary 
phenomenon had been photographed. Hate hesitated to publish this 
accidental discovery. Copies of the plate were sent to several spectro- 
scopists for examination with the request that an explanation, referring 
the phenomenon to: some origin other than solar, might be supplied, 
if possible. As no such explanation was forthcoming, the spectra 
were very carefully measured and described. 

On one and the same plate 12 exposures had been successively 
made in the third order spectrum of a plane grating. A solar image 
of 51 mm. in diameter was so adjusted that the image of a spot 
fell exactly on the slit. The length of the slit (6.5 m.m.) corresponded 
to about one eighth of the sun’s diameter. 

The first exposures show the normal spectrum without any con- 
siderable changes. Then came the disturbance, which culminated in 
the eighth spectrum and, in the following four, decreased rapidly. 
Hare gives reproductions of four spectra, each of them extending 
from 23812 to 24132. N°. 1 has been taken before the disturbance 
occurred; N°. 2 is the most abnormal spectrum; N°. 3 is called 
by Harr the “intermediate” spectrum, it has been obtained a few 
moments after the abnormal one; N°. 4 shows once more the nor- 
mal solar spectrum, as it was photographed at another time on 
another plate. Nos. 1, 2 and 3 show a dark band throughout the 
whole spectrum, corresponding to the sun-spot which had been 
focused on the slit. 

The most prominent features of the abnormal spectrum awe: 

1°. The band due to the spot appears much fainter than in the 
spectra, photographed before and after the disturbance. 


1) Georce E. Hare. “Solar research at the Yerkes Observatory”. Astroph. Journ. 
XVI p. 211—233, 1902. 


( 594 ) 


2°. With several Fraunhofer lines the intensity or the width is 
greatly diminished. This is most conspicuous with the 
broad, dark calcium bands H and K and with the hydrogen line 
Hd, these being almost totally absent in the abnormal spectrum. 

3°. Other lines, on the contrary, appear uncommonly 
strengthened. 

4°. Many lines are more or less displaced. 

The same peculiarities are noticed, though generally in a smaller 
degree, in the intermediate spectrum, so that the latter, in fact, forms 
a link between the abnormal and the normal spectrum. 

This marvellously complicated disturbance was not confined to 
light coming from a comparatively small part of the solar disk, for 
instance from the immediate surroundings of a spot; on the contrary, 
it extended almost equally over the whole width of the spectrum and 
was therefore nearly the same for all the light which came from a 
very great area of the Sun. 

The moments of the 12 exposures and the exact date had not been 
recorded, but there was sufficient evidence that the whole process 
of the disturbance lasted only a very short time. 

Harre calls the phenomenon: “a remarkable disturbance of the 
reversing layer”. But is it not almost impossible to imagine a rather 
thin layer in the solar atmosphere undergoing suddenly and simul- 
taneously over a great part of the sun such a thorough change, as 
to make its absorbing and radiating power in some parts of the 
spectrum for a while nearly unrecognizable ? 

It occurred to me, therefore, that the origin of the phenomenon 
should be looked for somewhere on the path of the light between 
the Sun and the Earth. If on this path there be media, causing 
anomalous dispersion, the beam must show an altered composition. 


As I formerly indicated 5), the properties of the chromospheric 
light may be derived from the supposition, that this light has been 
scattered out of the photospheric light by anomalous dispersion. 
According to this hypothesis the spectrum of the chromosphere 
informs us, which are the kinds of light, that may follow rather 
strongly curved paths in the solar atmosphere. So the idea suggested 
itself, that the same waves might play a striking part in HaAtp’s 
abnormal spectum. 

In order to investigate the question as impartially as possible, | 
marked (before consulting Hanw’s table or a table of chromosphere 


1) Proc. Roy. Acad. Amst. II, p. 575—588; ILI, p. 195—203; IV, p. 162—171; 
Physikalische Zeitschrift 4, p. 132 —'36. 
40 


Proceedings Royal Acad. Amsterdam. Vol. V. 


(592) 


TABLE I. 


Lines whose intensity is less in the abnormal than in the normal spectrum. 


Intensity 


a 


Chromo- 
sphere 


inter- 
normal | mediate | abnormal 


Wavelength Remarks, 


SPUAU] 


(ROWLAND) (HALE) (HALE) [(LoCKYER) 


3872.6 


in the abnormal spectrum 


4012.50 5 4 
4033 .29 7 42 
4034.64 6 10 


o—b- 171; ete. 
3-4 |Un, Fe 
3—4 |dn, Ve 


4063.76 20 RE ee eee 

4071.91 15 15 15% 

4077 .88 8 10 7e 
H 4102.00 40 7 ze 


3871.4 | | 4 C |)Not mentioned in Hare's 
| | Fe list, but distinctly weakened 
3874.09 Be A Dis Yea 2(?)| Fe on the reproduction. 
3878. 47 ON ND Vos bs te 3 3 | Fe, Fel 2 = 3878.15 and; = 3878.72; 
H, 3889.05 p 15 | = 8 H HALE mentions Ve, Mu. 
” 3895.80] 7 Ce 3 | Ze 
3899 . 30 5 RN = 2, V2 
3903.09 do re — 2—3 le 
3905 . 66 12 | LO a 2 Cr, Si 
3906 70] 14 | — | 4 2 Ve 
3913.63 eat ae eee Mn 6 Ti 
TON ne Mie SCE ed, 1i_|_* These intensities are very 
3016 54 3 LN ht 3 y {probably estimated too high 
J when compared with the 
3920.41 40 10% 105 3 Fe |numbersin the second column. 
3923.05} 12 12e | 19% 5 <4 tie eee OP ores 
K 3933.82 | 10 Ca 
3944.16 15 15% 12% 5, Al 
3948 91 13 15 — } le 
3950.10 3 — 2 "3 fe 
3953 .02 17 1D ol AS Fe, ete. 
3958 35 5 Ek — i Ti 
3961 67 20 DO ci 6 Al 
H 3968.63 | (700) 7 7 10 Ca 
H, 3970.18 7 8 | — 10 iH 
3977 .89 6 RT 2 Fe 
3986.90 6 Bree 
3998.78 | 4 4 | a ewes, 


(593) 


lines) on the reproductions of the spectra in the Astrophysical Jour- 
nal a number of lines, which struck me as being weakened in the 
abnormal spectrum. By means of Grorcr Hiees’ photographie atlas 
of the normal solar spectrum the wave-lengths of the selected lines 
were easily read; they are to be found in the first column of Table I. 

The second, third, and fourth columns show the intensities of 
these lines in the normal, the intermediate, and the abnormal spec- 
trum as given by Harre (for the normal spectrum from Rowraxp’s 
tables, for the other two from estimations by Mr. Abams). Hare 
remarks that the intensities of the lines were estimated independently 
for the two disturbed spectra’). The fifth column indicates the inten- 
sities of corresponding chromosphere lines as found by Lockyer in 


TABLE II. 


Lines whose intensity is greater in the abnormal than in the normal spectrum, 


Intensity. 


2 
Wave- EET TER eee Chromo- = Remarks. 
length normal | mediate | abnormal] sphere = 
cen (HALE) (HALE) f(LOCKYER) 3 
3921 86 Oe ee Zr, Mn 
SHAR — | — 25 P 
3930. 45 Seal 18 28 3=4 Fe 
BOONE If! ee ede 40 2 
GOTE EE Peat, ae eae b> p 
3950.50 Paige MEE y 
3962.29 3 ee 11 Fe? 
3973.77 6 — sy A: Ni, Zr, Ve,Ca 
398 |. 92 4 13 30 6 Ti, Fe * In HuMmPHREYS’ table 
A 3 | & | 40 ge hee Pmt 
3996 . 80 a md 5 p occur. 
4013.90 el dr. eta Ti, Fe 
4O14 67 En | 9 20 Fe 
4923 .38 ae ade Sa 10 
4033.77 pA Sarre ileal Oke Gs Mn 
4040.79 hare 20 4 Ve 
044.09 | 5 | 20 | 45 Fe 


1) In selecting the lines that appeared weakened in the abnormal spectrum I 
did of course compare the three spectra mutually. That is why in my table some 
lines occur, whose intensities, as estimated by Mr. Apams, are not comparatively 


low in the abnormal spectrum. 


=40 


( S59) 


the spectrum, secured at Viziadrug during the 1898 eclipse’); the 
sixth column shows the absorbing substances. 

In a similar way Table IH has been composed; here we find the 
lines, which on the reproduction appeared to be strengthened 
in the abnormal spectrum. 

The result is very striking. Weakened lines correspond 
to chromosphere lines, almost without exception; 
mostotthe strenzthened lines, on the other hans 
are not to be found in the spectrum of the chrome 
Bip be re: 

Lockyer gives the strength of the chromosphere lines on a scale 
such that 10 indicates the strongest and 1 the faintest lines. If we take 
into account that in his list the greater part of the lines bear the 
numbers 1 and 2, our table shows us, that by merely observing the 
abnormal solar spectrum we have been able to pick out strong 
chromosphere lines. This cannot be chance. Undoubtedly both phe- 
nomena — the weakening of Fraunhofer lines in the abnormal spec- 
trum and the origin of the chromosphere spectrum are to be 
explained in close relation with each other. 

The strengthening of lines in the abnormal spectrum does 
not, on the contrary, seem to be so directly connected with the com- 
position of the chromosphere spectrum. 


If our view be correct that the chromospheric light has been se- 
parated by strong ray-curving from the “white” light emitted by 
deeper layers, those special radiations must, as a rule, show reduced 
intensity in the spectrum of the Sun’s disk *). Fraunhofer lines cor- 


1) Lockyer, CurisHotm-Barten and Peprer. “Total Eclipse of the Sun, January 
22, 1898. — Observations at Viziadrug,” Phil. Trans., A, vol. 197, p. 151—227, 1901. 

2) It might be thought that the rays forming the chromosphere light, need to 
be absent only from the spectrum of the edge but not from that of the central 
portions of the Sun’s disk. By a simple consideration, following from a look at 
Fig. 4 of my paper, read in Febr. 1900 (Proc. Roy. Acad. Amst. II, p. 580) we 
see, however, that the chromosphere light visible to us may very well, fora part, 
have its origin even in points of the Sun which lie opposite to the Earth’s direc- 
tion. The chromosphere light, reaching the Earth, may proceed from any point 
of Scuipr’s “critical sphere“. For the greater part it is likely to come from the 
back half of the Sun. But then the half, facing us, furnishes the chromospheric 
hight which travels to other regions of the universe, and this light, of course, is 
wanting in the spectrum of the disk. (There is some reason for supposing that, 
on an average, more chromospheric light is sent forth in directions making great 
angles with the Sun’s equator, than to the equatorial regions, including the 


Earth’s orbit.) 


* oor le 


ETT B, 


er 


responding to chromosphere lines will therefore have a more or less 
darkened background in the ordinary solar spectrum. The rate of 
darkening at various distances from the centre of an absorption line 
is, of course, connected with the shape of the dispersion curve near 
that line; whereas the average shading depends 1st on the quantity of 
matter causing anomalous dispersion and 2°¢ly on the slopes and the 
directions of the density gradients in the gases through which the 
light is transmitted, viz. on the Sun’s “activity” *). 

We distinguish, therefore, a twofold origin of the dark lines in 
the solar spectrum: real absorption of those waves, exactly cor- 
responding to the periods of the media, and dispersion of the 
strongly deviated neighbouring light *). 

The dispersion will be especially evident where extraordinary diffe- 
rences in the density of the medium occur ; in this way the widening 
of most of the Fraunhofer lines in the spectra of spots may be 
accounted for. 

Dispersed light has not, of course, vanished; the absence of certain 
rays in the spectrum of a spot is counterbalanced by the increased 
intensity of the same radiations in the light coming from the neigh- 
bouring faculae. Thus the distribution of the density in the solar 
gases may locally be such, that a limited part of the disk seems to 
emit a considerable amount of rays with abnormally high or abnor- 
mally low refractive indices. In-the spectrum of such parts not only 
will the Fraunhofer lines show narrower and fainter than usually, but 
here we may even meet with lines contrasting brightly with their 
surroundings. These bright lines will not coincide with the corre- 
sponding absorption lines; their average wave-length will in general 
be greater or smaller than that of the absorbed light, for, according 
to the accidental distribution of the density, we shall find either the 
rays with high or those with low refractive indices most prominent 
in the beam. 


The above considerations suggest an explanation of Hare’s abnormal 
spectrum. 

In fact, the lines showing especially faint in this spectrum were 
exactly those, causing strong anomalous dispersion — witness the 


1) The possible influence of the general or regular ray-curving (after Scumpt's 
principle) on the feature of the spectral lines has, in the present paper, been left 
out of consideration. If we were able to observe or to calculate the radii of the 
“critical spheres‘‘ for radiations undergoing anomalous refraction, it would be 
possible to estimate that influence; but as yet sufficient data are wanting. 

2) Proc. Roy. Acad. Amst. If. p. 580. 


a Te we ine 


( 596 j 


chromosphere spectrum. With MH, A, Hy) and some iron lines it 1s 
conspicuous that the abnormal faintness regards mainly the broad 
dark shadings of the lines, i.e. those parts, whose darkness in the 
normal spectrum we attributed not to absorption, but to dispersion. 
Moreover, the dark band due to the spot has nearly disappeared. This 
means that waves, which in normal circumstances are wanting in 
the spot spectrum on account of their strong dispersion, at the time 
of the disturbance had been gathered again into the beam reaching 
the instrument. 

How all this may happen will become evident as soon as we shall 
be able to establish a plausible cause, by which, within an angular 
space great enough to include a considerable part of the solar disk, 
the strongly dispersed rays might be gathered again. 


It is not necessary to introduce a new hypothesis for the purpose. 
The same idea about the Sun’s constitution 1) which enabled us to 
explain the properties of the chromosphere and the prominences, 
furnishes us once more with the required data. 

Indeed, if (according to Scumipt’s theory) the Sun is an unlimited 
mass of gas, surfaces of discontinuity must exist similar to those, 
whose general feature has been determined by Euperx ®) for a sharply 
outlined radiating and rotating sun. These surfaces must extend unto 
the remotest parts of the gaseous body — a conclusion in excellent 
harmony with the visible structure of the corona. For along the 
surfaces of discontinuity waves and whirls are formed; the core-lines 
of the vortices nearly coincide with the generatrices of these surfaces 
of revolution, and in these cores the density is a minimum. This 
may account for the streaky appearance, shown more or less dis- 
tinctly in all good photographs and drawings of the corona. 

This particular appearance may have another cause, though ; for 
what follows, however, this is immaterial. We only assume that the 
density of the coronal matter varies in such a way, as to correspond 
to the striped structure visible at the time ofa total eclipse of the Sun. 

A coronal streamer which, at a given moment, runs exactly in the 
direction of the Earth may be very roughly compared, then, to a 
bundle of glass tubes through which we are looking lengthwise. Such 
a structure will gather and conduct rays of various directions, ente- 
ring it at one end. This takes place also if the parts with the greater 
and those with the smaller optical density do not alternate abruptly, 
like glass and air, but gradually. 


1) Proc, Roy. Acad. Amst. IV, p. 162. 
2) R. Empen, Beiträge zur Sonnentheorie, Ann. d. Phys. [4], 7, p. 176—197. 


In Fig. 1 the optical density of the 
matter may be represented by the com- 
pactness of the streaking. A ray for 
Which the medium has a large positive 
refractionconstant would for instance 


follow the path AA‘, curving round the 


denser parts of the structure; aray BB, 


for which the medium possesses a large 


| negative refractionconstant, would move 


in a similar way through the more rare- 
fied regions. On the other hand, the light 
| CC" for which the constant exactly equals 
zero is not influenced by the fluctuations 
of the density ; and if for some kind of 
light the refractionconstant is very nearly 
zero, the ray would have to travel a long 
way almost parallel to the structure before 


its curving would be perceptible. 

Now the corona sometimes shows exceedingly long, pointed strea- 
mers. We only have to suppose that the Earth was exactly 
inthe direction of sucha streamer at the moment 
the abnormal spectrum was photographed; then 
all the irregularities observed in this spectrum become clear. Light, 
under normal circumstances absent from the solar spectrum through 
strong dispersion, has been collected by the coronal streamer ; hence 
the weakening of the Fraunhofer lines, especially also of those 
in the spectrum of the spot. As the abnormalities were caused by a 
peculiar distribution of matter in the vast regions of the corona, lying 
between the source of light and the Earth (and not by disturbances 
in a relatively thin ‘reversing layer’) they could appear in the 
same way over a great part of the Sun’s disk. The rarity of the 
phenomenon is the result of the slight chance we have to take a 
photograph at the very moment on which an uncommonly long coronal 
streamer is projected exactly on the part of Sun’s disk illuminating 
the slit; the short duration finally is a consequence of the 
difference between the angular velocity of the corona and that of the 
Earth in its orbit. 


As we have mentioned before, #0 chromosphere lines correspond, 
in general, to those lines showing extraordinarily strong in the abnor- 
mal spectrum. How are we to account for the strengthening of 
these lines? 


(598 ) 


We might be tempted to think of absorption in the corona; for 
if it be true that a streamer was turned towards the Earth, the rays 
had to go an uncommonly long way through an absorbing medium. 
But on closer examination this idea is less probable. 

The particles of the extremely rarefied corona gases will hardly 
influence each other; their periods will, therefore, be almost absolutely 
constant, so as to cause very sharp, narrow absorption lines. Thus it 
is difficult to understand, how an absorption line, already present 
in the normal solar spectrum, might be strengthened by the absorbing 
power of the corona. Further, in studying Harr’s table, we observe 
that many lines which are strong in the abnormal spectrum, show 
a much smaller intensity in the intermediate spectrum (taken only 
a few moments later); whilst the reverse happens as well, viz. that 
lines are strong in the intermediate and very weak in the abnormal 
spectrum. This hardly fits in with the absorption hypothesis. Some 
lines showing this peculiarity are given in table III. 


TABLE III. 
Lines whose intensity is very different in the intermediate and the abnormal spectrum. 


Intensity | 
bn | ela eee Pe Remarks. 
RowLAND)| (HALE) (HALE) | (LOCKYER | 
el Ee GE ee EE SSP ee eee eee 
3005.66 2 20 — 2 Cr, ot 
3905.81 21 — 20 Si 
3921.71 9 14 — Ti,La,Zr, Vii 
3921.87 4 -- 20 Zr, Mn 
3950.33 = 10 — P 
3950.51 De 13 Me 
3972.30 2 12 — Ni 
3972.61 FS Yin AL ee 42, ? 
4005.86 3 25 D ? 
4057 .39 4 — any {—2 Cos Fe 
4057 . 66 7 40 aa P 


In the chromosphere spectrum corresponding lines seem to be 
wanting. (At 2 3905.66 and 2 4057.39 the faint chromosphere line 
may SNE belong to another element than the abnormally streng- 
thened absorption line). 

To arrive at a more satisfactory explanation of the strengthening- 
phenomenon we suppose that these absorption lines do indeed cause 
anomalous dispersion of neighbouring waves, but in a very slight 


zi 


, ogous 


degree. Then, the refractive indices of the neighbouring waves differing 
hardly from unity, the direction of those rays will only be percep- 
tibly changed after they have travelled a very long way through 
the corona and almost parallel to its structure-lines. Whereas the 
strongly refracted rays, entering the coronal streamer in various 
directions, were obliged to follow the structure-lines, curving about 
them, and so in a sense were concentrated on the Earth, it may 
happen with the extremely slightly curved rays we are now consi- 
dering, that they have been bent for instance only once over the 
whole length of the streamer and continue their way in a direction 
not meeting the observing station. The divergence of a beam con- 
sisting of these rays will have increased, the intensity diminished. 
Thus, the resultant spreading of neighbouring light causes the 
absorption line to appear somewhat widened and therefore strengthened. 
But obviously it must be possible too, that, after a short time, under 
the influence of another part of the corona, circumstances turn out 
even favourable for that slightly curved light to reach the observer. 
In that case the absorption line is weak again. (Similar alternations, 
of course, also occur with the more strongly refracted rays, and that 
in quicker succession, but this does not alter the fact of their average 
intensity appearing increased as long as the structure lines of the 
coronal streamer are turned towards the spectroscope. For a detailed 
discussion of this case see the Note at the end of this paper). 


In both abnormal spectra a number of absorption lines are more 
or less dispiaced. Perhaps this is partly due to motion in the line 
of sight; but after the foregoing it will not be necessary to explain 
in detail, that also anomalous dispersion can account for this pheno- 
menon. Dissymmetric form of the dispersion-curve as well as a 
peculiar distribution of the density of the coronal matter may une- 
qually affect the intensity of the light on both sides of the absorption 
line, and thus bring about a seeming displacement of the line. 


Certain peculiarities of lines in the normal solar spectrum. 


If we have been right in connecting the uncommonly great abnor- 
malities in Hare's spectrum with a very particular position of the 
Earth with respect to the corona, it is to be expected that similar 
irregularities, though to a smaller degree, will ever be found, as the 
sunlight always reaches us through the corona. 

According to Jewerr’s above mentioned investiga’ ions this supposition 
proves to be well founded. Many solar lines have varying intensities 
and positions, so that Jewerr deems them unfit for standards for 


( 600.) 


very accurate determinations of wavelengths. And these are for the 
greater part the most prominent lines of the spectrum, especially the 
shaded -ones *). 

JuWELL emphasizes the fact that all distinetly shaded lines in the 
solar spectrum show to a greater or less degree the following typical 
feature ®). 

Within a broad, shaded, moderately dark background a much 
darker central absorption line contrasts rather sharply (Fig. 2). 


ed 


Tig. 2 Fig.5. 


Besides, the absorption curve often shows dippings close to the central 
line, as in Fig. 3, sometimes symmetrical, sometimes dissymmetrical. 
Jewett affirms that this is not an optical delusion, due to contrast, 
but a real phenomenon. He assumes, therefore, that the broad absorp- 
tion band is produced in the lower portions of the solar atmosphere 
and under a great range of pressure; that in higher levels radiation 
prevails again, producing a rather wide emission line ; and that finally 
in the highest parts, where the pressure is very much less, the sharp 


absorption line is produced. The position of this central absorption - 


line with respect to the emission line is usually unsymmetrical, which 
is conspicuous in the case of H and A. The central line itself also 
varies somewhat in width upon different plates and its maximum of 
intensity is not always in the middle of the line. The displacement 
of this central line in MZ and A varies in magnitude, but, so far as 
has been observed, always toward the red with respect to the emis- 
sion line and the corresponding metallic line (in the are). 

Jewerr concludes that the absorbing calcium vapour descends all 
over the solar surface with a velocity sometimes amounting to about 
75 miles per minute. 

Upon the same plates showing strong dissymmetry in // and A, 
the shaded lines of other elements (Me, A/, My, Si) have been 
examined. The strongest iron lines and one aluminium line showed 
displacements of the same character as that observed in the case of 

1) Astroph. Journ. XI, p. 236, 1900. 

2) Jewett, “Certain peculiarities in the appearance of lines in the solar spectrum 
and their interpretation”. Astroph. Journ, Ill. p. 99, 1896, 


ore aac ill 


a Je 
zn” 


( 601 ) 


H and kK, but to a much smaller degree and sometimes toward the 
violet, sometimes toward the red. Certain shaded lines of My and Si, 
on the contrary, showed no evidence of a displacement, nor did the 
iron lines without considerable shading, the faint calcium line at 
A 3949,056 and many other lines. 

If we admit no other explanation of line-shifting and -widening 
besides those, based on DorPrer’s principle and on the effect of 
pressure and temperature, we arrive at very strange conclusions 
relative to the condition of the elements in the solar atmosphere. Not 
less surprising is, as noticed by Jrwrrr *), the small amount of the 
absorption in the shaded parts of the lines, when we consider the 
enormous depth of the solar atmosphere and the high pressure which 
must exist in the absorbing layers, for them to produce a broad 
absorptionband. 

By making various suppositions concerning the condition of the 
gases in the solar atmosphere, JrwerL succeeds in finding an inter- 
pretation of most of these astonishing facts. But it must be granted 
that his explanations include a greater number of arbitrary and mu- 
tually independent hypotheses than is the case with our explanations, 
founded as they are on selective ray-curving and readily deduced 
from that principle for each separate phenomenon, without intro- 
ducing new suppositions. 

Only the dark central lines of the Fraunhofer lines are to be 
ascribed, in our theory, to real absorption. Their shaded background 
of varying intensity we consider as an effect of anomalous dispersion 
of the not absorbed neighbouring waves. This selective scattering 
will be strongest in those places where the density-gradients are 
relatively steep, viz. in whirls in the deeper regions of the gaseous 
body. But some of the widely dispersed rays may be gathered by 
the corona owing to its “tubular structure and be conducted along 
its greater or smaller streamers. 

This will especially apply to the most strongly refracted waves, 
Whose position in the spectrum is very close to the real absorption 
lines; thus pseudo emission lines are produced in about the middle 
of the pseudo absorption bands. *) 


1 Astroph. Journ. ILI, p. 106. 

2) A most remarkable fact is that the shading of K, H, the iron-line à 3720.086 
and of some other strong shaded lines is sometimes partially kroken up into a 
series of faint nebulous lines, symmetrically situated about the central line. In 
each case the distance apart of the component lines increased as the distance from 
the center increased (Jewett, Astrophysical Journal 8, p. 51—53). 

It might have been predicted by our theory that we should meet with this 
phenomenon now and then. 


( 602 ) Ek 4 


Most likely Hare's abnormal spectrum has shown us a case, where 
these seeming emissionbands acquired an uncommon extent. We may 
therefore expect that a systematical investigation of solar spectra, 
photographed at different times, will afford all kinds of intermediate 
cases. 

It would be desirable, for the moments when the photographs 
are taken, to know form and position of the coronal streamers ex- 
tending toward the Earth. At all events the actual phase of the sun- 
spot period, with which the shape of the corona seems to be con- 
nected, should be taken into consideration; and perhaps the simul- 
taneous observation of the photospheric reticulation, discovered by 
JANSSEN, may procure some evidence concerning the position of coro- 
nal streamers, and thus contribute to our knowledge of their influence 
on the Fraunhofer spectrum. 


Mineralogy. — “On the refractive index of rock-qlasses,” by P. Trscu: 
(Communicated by Prof. J. L. C. SCHROEDER VAN DER Kork). 


Of the group of the igneous rocks, the origin of which out of 
fluid red-hot condition we accept, the voleanie rocks constitute that q 
subdivision, which includes the rocks, that as lavas have broken 
through the surface of the earth. 

The quick cooling at the atmosphere renders it possible that in 
these rocks part of the magma congeals amorphously, so that next 
to the minerals a rockglass appears, which constitutes either an infe- 
rior part or a prevailing one of the rocks. So in general this glass 


Let us consider a beam of light of an exactly defined wavelength belonging to 
the shaded background of an absorption line. This beam leaves the deeper layers 
of the Sun with a certain divergence. As it passes along a “tube” of the corona, 


q 
| 


its divergence will alternately diminish and increase, and on reaching the Earth 
it shows in the spectrum an intensity, depending on the divergence (or perhaps 
convergence) with which it has left the last traces of the corona. For a beam of 
light whose wavelength is only slightly nearer to that of the absorption line, the 
medium will have a considerably greater refraction constant, so that the rays of 
this beam, on their way through the corona, may make part of a bend more than 
the former ones. The beam may therefore arrive with a quite different degree of 
divergence and, consequently, of intensity. Thus, proceeding towards the absorption 
line from either side, we easily see that we must meet with a periodically changing 
intensity. Rays, corresponding to the middle of one of the so formed fringes, will 
have made one full bend more or less than the rays, belonging to the middle of 
the next fringe. 

If this interpretation be correct, the width and the number of fringes visible 
must prove to be variable, As far as | know, the observations made on this point 
are not numerous. May the proposed views serve to further the investigation of 
this interesting phenomenon. 


( 603 


consists of silica and metal-oxides. We may suppose that the silica, 
which is most likely to be the principal part, will also have a pre- 
valent influence on the physical characters of such natural glass. 

A determination of the specific gravity of the glass is made more 
difficult by the presence of many gas-bubbles. If this obstacle did 
not exist, the specific weight would be a better expedient for a 
quick temporary orientation than the determination of the refractive 
index, for which more instruments are necessary. With respect to the 
specific gravity it could be stated, that with these rocks where the 
value of the index the use of bromoform as liquid of comparison neces- 
sitated and whose exponent proved to be greater than that of bromo- 
form (1,593), the specific gravity of the glass was still higher than 
that of bromoform (2,88). The small air-free, not to be isolated 
grains, still sank in this liquid. Now I have tried to find out in how 
far the refractive index is dependent on the SiO, percentage. For 
that purpose 16 rocks have been examined, forming a series of the 
most acid to the most basic magmas, which occur in nature. 

The result has been eomprised in the following table: 


Name 


| 
| 
| 
| 
| 


Origin sis [tates Index 
| 


Granite Magurka, Hungary 72,65 1,500 
Granite Brocken, Harz Mountains AAG 4,500 
Granite | Auvergne 70,62 1,500 
Granite ‚_ Korinitsch, Hungary 67,31 1,510 
Quartzdiorite | Adamello, Tyrol 66,58 10 
Syenite | Plauensche Grund, Dresden 60 26 1,520 
Klaeolite-syenite | Ditro, 59,88 1,525 
Diorite | Hodritsch, Hungary 59,57 1,525 
| 
Syenite | Ditro, 57,36 1,530 
Augite-syenite | Monzoni, Tyrol 53,79 1,550 
Chrysolitenorite Radau Valley, Harz Mountains 53,64 1,550 
Diorite | Auvergne 50,86 1,570 
Quartzdiorite | Dumkuhlen Valley, Harz 48,89 1,585 
Basalt | Dyrafjord, Iceland 4850 1,540 
Gabbro Radau Valley, Harz 44,08 1,620 
Harzburgite Harzburg, Harz | 42,24 1,630 


( 604 ) 


From this we see that a classification exclusively according to 
decreasing SiO, percentage, coincides with an increasing value of 
the refractive index. 

Apparently the metal oxides present have only little influence on 
that value, at least this influence falls within the limits of the 
errors of observation. 

A chrysolite-norite and an augite syenite with about the same 
SiO, percentage have also the same index, whereas the oxides, 
especially MgO are sure to be there in quite another relation, for 
in the chrysolite-norite the minerals containing Mg come strongly 
to the foreground. 

As regards the colour of the glass it will be almost wholly 
dependent on the iron-percentage. 

With the examined glasses the colour changed from light green 
to dark brown. Just as with isomorphous mineral series, as e. «. the 
enstatite-hypersteneseries, the dark colour most likely points to a 
greater iron percentage than the light one. 

The typical amorphous glassfracture can be easily distinguished 
at the splinters under the microscope. 

The fusion of the roek-powder took place in a gasflame in which 
compressed oxygen was blown. As an underlayer a cupel of chalk 
or bone-ash was used. But care has to be taken that the melted 
magma of the cupel remains isolated, because there is a chance that 
oxides of alealic earths will be absorbed by the cupel and in 
consequence the composition of the magma does not answer any 
more to that of the rock. This can be obtained by directing the 
point of the flame towards the middle; the upperlayer then fuses 
quickly to a little ball, which remains isolated by the underlaying 
rock-powder of the eupel. To control the regularity found in the 
independence of the refractive index of the Si O, percentage, two 
mixtures of the following composition were made: 


L IL 
SiO, 60 °/, 60°/, 
Fe,O, 10 20 
A1,O, 10 5 
Ja0 10 5 
MeO 5 10 


K,0,Na,O 5 En 


Of both the mixtures the fused glass had the index 1.520; here 
we see again the prevalent influence of SiQ,. 
At last some slags and melted minerals were investigated, 


P. TESCH. On the refractive index of rock-glasses. 


Proceedings Royal Acad, Amsterdam. Vol. V, 


( 605 ) 


Composition. Index. 
SiO, 45,5 1,600 
CaO 19,8 

FeO 5,3 

SiO, 27,4 1,750 
FeO 41,7 

Cabr. 0,2 

Pb 4a. 

ALO 0,8 

ZnO 21,8 

MnO 


In this slag the ZnO plays the part of the MgO. When ZnO is 
replaced by MgO, the index remains the same. 
Finally the index of the following minerals was determined: 


Quartz mit. 100-°/, 1,475 
Chrysolite fi 40—45 1,610 
Orthoclase i 65 1,485 


The last mineral, the pure K.Al.silicate consequently does not fit 
into the composed series. After mixing with some grains Fe,O, 
(5—10 ,/°’ and fusing anew the index was raised to 1,510. 

The method described above can be of practical use for a quick 
determination of the SiO, percentage of slags from the refractive 
index with an accuracy of + 2 °/,. 

A word of thanks for the aid and advice to the Professors Dr. J. L. C. 
SCHROEDER VAN DER Kork and 8. J. Vermars Jr. may find a place here. 


Mineralogy. — “On an “Kisenrose” of the St. Gotthard”. By 
G. B. HoGENRAAD. (Communicated by Prof. J. L. C. SCHROEDER 
VAN DER Kork). 


Some time ago I tried to get a Hematite-streak with a so-called 
“Kisenrose.”’ I did not succeed however, for to my astonishment 
the streak was not red but black. Several explanations came to 
my mind : 

1°. that the mineral was somewhat friable, which was the cause 
that the streak could not consist of the very finest particles. But in 
rubbing the black colour remained; only the outlines showed a 
reddish-brown tint. The same was stated with about 25 other pieces 
of the same finding-place. So that the explanation proved to be not 
the right one. 


( 606 ) 


2°. that the mineral contained Mn or Ti, since these elements have 
a great influence on the colour of the streak. But an analysis only 
produced little Ti and no trace of Mn, so that this explanation did 
not hold good either. 

3°. that the mineral was magnetite. In its favour spoke the very 
distinet magnetism, stronger than hematite generally shows. 

I then consulted some literature, to see whether anything had been 
written before on the streak, the magnetism and the chemical com- 
position of “Eisenrose.” 

Dana says‘): 

St. Gotthard affords beautiful specimens, composed of crystrallised 
tables grouped in the forms of rosettes (Eisenrosen), and accompany- 
ing crystals of adularia. 

Dana calls this occurring Hematite, though he neither speaks of the 
chemical composition, nor gives any particulars about streak or 
magnetism. 

In the “Zeitschrift für Krystallographie und Mineralogie von P. 
Grorn”’ I found in Number 13 on p. 301 a report by A. CATHREIN 
from Srriver’s account on “Pseudomorphose von Magnetit nach 
Eisenglimmer von Ogliastra in Sardinién”’, written in tke Atti della 
Reale Accademia Dei Lincei 1886. Volume IL, 2°. Semestre, p. 331. 
The report in question follows here : 

„Die Hauptmasse der Stufe besteht aus einem grobkörnigen Mine- 
ral, dessen unregelmässigen Individuen von mehreren Centimetern 
Durchmesser fest mit einander verwachsen erscheinen. Jedes Korn 
zerfällt nach einer Richtung äusserst leicht in dünnste Lamellen. 
Harte 6, Pulver schwarz, stark magnetisch, schwer schmelzbar, in 
Salzsäure leicht löslich. Diese Eigenschaften kommen dem Magnetit 
zu. Das Gemenge erscheint ganz frisch, unverändert und ursprüng- 
lieher Entstehung. Dass es sich hier nicht um nach {111} blätterig 
abgesonderten Magnetit handelt, folgt aus dem Mangel jeder Spur 
von Spaltbarkeit nach einer anderen Richtung ausser jener einen. 
Die Lamellarstructur als Druekwirkung aufzufassen verbietet die 
Richtungsänderung der Lamellen in jedem einzelnen Korn. Nach 
des Verfassers Ansicht bleibt nur die Annahme einer Pseudomorphose 
von Magnetit nach Eisenglimmer.” 

So this appearance as regards streak and magnetism corresponds with 
the specimen examined by me. Through the absence of a chemical 
analysis it cannot be decided in how far the supposition is right, that 
he had to do here with a pseudomorphosis from Magnetite to Eisen- 
olimmer. 


1) System of Mineralogy p. 216, 


( 607 ) 


In the ‘‘Zeitschrift der Geologischen Gesellschaft” Bd. 22, 1870 I 
found on page 719 in an article by G. vom Rarn the following 
statement *): 

“Pseudomorphische Massen von Magneteisen nach Kisenglanz. Farbe 
und Strich schwarz, schimmernd auf dem Bruch, magnetisch. Das 
rz ist aber weder dicht, noch körnig (wie es sonst dem Magneteisen 
zukommt), sondern schuppig. Man erkennt sogar in einzelnen Drusen 
ganz deutlich die hexagonalen Formen des urspriinglichen Eisenglan- 
zes; doch auch diese letzteren haben einen schwarzen Strich.  Ver- 
mutlich is demnach jene ganze colossale Schichtenmasse bei Vallone 
urspriinglich Eisenglanz gewesen”. 

So to this can be applied what has been remarked on Srriiver’s 
article. 

Finally D. F. Wiser says *): 

Die Eisen-Rosen vom Pomonetto wirken sehr stark auf die Magnet- 
Nadel. Das Strich-Pulver is dunkel-röthlichbraun, beinahe schwarz. 

Die Wirkung auf die Magnet-Nadel is bei den Schweitzerischen 
fisenglanzen gar sehr verschieden, sowie die Nüanzirungen von Kisen- 
schwarz bis Stahlerau in ihrer Färbung. Bemerkenswerth scheint es 
mir, dass die EHisen-Rosen ohne aufliegende Rutil-Krystalle immer 
die schwärzeste Farbe zeigen, und dass dieselbe hingegend immer 
heller wird, je mehr Rutil auf den End-Flächen der Kisenglanz- 
Tafeln, ich möchte sagen, ausgeschieden worden ist. 

Die Mineralien, welche die Eisen-Rosen vom Pomonetto begleiten, 
sind: kleine, graulich-weisse Adular-Krystalle, kleine sechsseitige Tafeln 
von Tombackbraunen Glimmer und eine schmutzig griinlich-gelbe 
Rindenformige Substanz die vielleicht den Chloriten beigezählt wer- 
den darf. 

Mein Freund, Hr Bergrath Srockar hieselbst, hat die Eisen-Rose 
vom Pomonetto analysirt und wird hoffentlich nächstens das Resultat 
seiner Untersuchungen veröffentlichen.” 

However LE could not find this promised analysis anywhere in 
literature, so that I decided to do it myself (1). For a good control 
the same analysis was made by Messrs B. H. van DER LANDEN (II) 
and G. W. Marrúr (HD. The results of our investigations were as 
follows : 


1) Geognostisch-mineralogische Fragmente aus Italién, chapter VIIL: Die Insel 
Elba, Zeitschr. D. G. G. 1870. 
2) Bericht über Mineraliën aus der Schweiz, N. Jahrb. 1854 p. 26. 


r 
. 


Proceedings Royal Acad. Amsterdam. Vol, \ 


Fe 69,94 69,13 69,50 
O 29,97 29,60 30,46 


accompanying mineral 1,2 


99 91 99 93 SE) 
Reckoned for : 
Hematite Magnetite 


Fe 70 72,41 
O 30 27,59. 
So that my conclusion is that we have not to do with Magnetite but 
with Hematite. 
The results of my researches are in consequence the following: 
Tst, That I have had to do with Hematite with very obvious 
magnetism and a black streak, which in rubbing along the outlines 
shows a brown tint (which generally every black streak does) and 
not with a pseudomorphosis from Magnetite to Hematite. 
2ad- That where in literature of this occurrence of Hematite has 
been spoken, no analysis has been added, though the magnetism and 
the black streak have been observed more than once. 
sed, That it is desirable to convince oneself of the chemical com- 
position with every “Eisenrose”, which shows these characteristics. 


Physics. — “Contributions to the theory of electrons.” 1. By Prof. 
H. A. Lorentz. 


Simplification of the fundamental equations by the introduction 
of new units. 


§ 1. If all quantities are expressed in electromagnetic units, as I 
have done in former papers, the relations between the volume-density 
o of the charge of an electron, the velocity » of its points, the 


1) | here by have to mention that first the figure for the oxygen was determined 
by reduction in a hydrogen-current und weighing of the water absorbed by Ca Clo; 
that after that the figure for the iron was determined by dissolving the reduced 
mineral in dilute H,SO, and making a titra'ion ot this solution (after reduction 
in a H,S-current and after removing the H,S by boiling in a CO, atmosphere) 
with a KMnO,-solution, of which 1 cM® corresponded with 8,9 m.G. Fe. 

The presence of Ti was shown as follows: the mineral was melted together 
with KHSO,, the fused mass dissolved in cold water. This solution together with 
H,0, gave the well-known orange colour of TiO;. Moreover after adding a 
little HNO;, the Ti after having been boiled precipitated as white TO). The 
accompanying mineral, which in microscopic examination proved to be adularia, 
was removed as much as possible, 


( 609 ) 


dielectric displacement > in the aether, the current {and the magnetic 
force § are as follows *): 


du} =o, 
dod, 0 
end uw tors, 
onhe Q v) 


(=d ov, 
do'h= 0, 
roth=4Anrl=4r(d dot), 
4 ac? rot d = — bh, 
where ¢ is the velocity of light in the aether. To these equations we 
must add the formula 
F=4actd + fy. b] 
for the electric force, i.e. the force, reckoned per unit charge, which 
the aether exerts on a charged element of volume. 

The equations take a somewhat more regular form if we express 
o, >, Land f in electrostatic units (preserving the electromagnetic unit 
for 6) and a further simplification is obtained, if, instead of the units 
for charge and magnetic pole that are usually taken as the basis of 
the electrostatic and electromagnetic systems, we choose new ones, 
4a times smaller *). Introducing both modifications, we have to 
replace’o, >; l- by — ze = ae a 

we VA Van’ cVAxr 
letter must now represent the force acting on the new unit of charge, 


, f by cV4dar.f, because this 


and likewise § by V 4a. 6. 
This leads to the equations 

QS Obs ok Ar EN (1) 
s Edin (obi 0 ee es ee 
GE bh hd AE ean ee 
ei Bn re ne Es (IV) 

1 ‘he 
rot fh == == — (D+ 00); - 2 . . . (V) 


( 


1) See my Versuch einer Theorie der electrischen und optischen Erscheinungen 
in bewegten Körpern. 1 shall again suppose that all quantities are continuous 
functions of the coordinates, so that e.g. the density p will be regarded as passing 
gradually to the value 0, which it has outside an electron. With the exception of the 
letters, the notations are the same as in the just mentioned treatise. The scalar 
product of two vectors a and b will be denoted by (a.b), the vector product by 
[a.b]. The axes of coordinates are supposed to remain at rest, relatively to 
the aethicr. 

2) This change has been warmly advocated by Heavrsipe. The units [ shall 
how use are those that have been adopted for the Mathematische Encyclopddie. 


41% 


( 610 ) 


eee 
pt De EP es (VI) 


ul 
htss. Di. RDP ARE Oe TE 


In connexion with the last formula it may be remarked that d is 
the electric force that would act on an immovable charge. 
The electric energy per unit-volume is given by 
re 1 9 af 
We ed pi ee Re rt a at yk, 


9 
a 


the magnetic energy per unit-volume by 


ae te 
i mS ae De . . . . . . . . . (LX) 


and Poyntine’s flux of energy by 
TSS Jo . hb] . . . . . . e e (X) 

We shall further write for the total electric and 7’ for the 
total magnetic energy of a system. 

The equations (IV) and (V) suffice for the determination of the 
magnetic force b, as soon as the current [ is given in every point. 
W, is then known by (IX) and 7’ follows by integration. In this 
sense, every motion of electricity may be said to be accompanied 


~~ & 


by a definite amount of magnetic energy. 
Scalar potential and vector-potential. 


§ 2. The equations of § 1 apply to every system in which 
charged matter moves through the aether, whether the charge be 
confined to certain extremely small parts of space (electrons) or 
otherwise distributed. Moreover, the motions may be of any kind ; 
the electrons may have a pure translatory motion, or a rotation 
at the same time, and we may even suppose their form to change 
in the course of time. For the validity of the formulae it is however 
required that each element of volume whose points move with the 
charged matter should preserve its charge, though its form and 
dimensions may change. This is expressed by the equation (IT) and 
it is on this ground that the electric current |, as defined by (IID, 
(the resultant of the displacement-current d and the convection-cur- 
rent ee) may always be said to be solenoidally distributed, so that 

dio == 02 

If now the motion of the charged matter is given, the electro- 

magnetic field in the aether, within and without that matter, has 


( Git} 


to be determined by means of (I)—(VI), a problem that may be 
reduced to equations of the form 
1 Oy 
yc ae 
COE: 


in which @ is a known, and y an unknown function of w,y, zt. 


En Oi Va Un! ay Ae edn See 


Let a be any closed surface and 7 the normal to it, drawn out- 
wards. 

Then, if the equation (1) holds in the whole space JS, enclosed 
by o, we shall have for the value of w in a point P of this space, 
at the time f, 


Ie: vod: Pee Fo any abe 
i —}| — |— — | — 
he eu r bel er = | r 5 | Ly On ( r ) 


Here the first integral extends over the space S and the second 
over the boundary surface 6; 7 is the distance to P, and the square 
brackets serve to indicate the values of the enclosed quantities for 


jp 
the tme. tn 
Cc 

Let us now conceive the surface 6 to recede on all sides to infinite 

distance and let the circumstances be such that the surface-integral 


in (2) has the limit 0. Then, ultimately: 


A NE i 
p= [> leas . . . . . . . (3) 


where the integration must be extended over infinite space. 

§ 3. Equations of the form (1) may be deduced from the formulae 
DVI) in many different wavs; they may e.g. be established for 
each of the components of d and *.') The solution is however ob- 
tained in a simpler form’), if one introduces four auxiliary quantities, 
a scalar potential p and the three components a, a, a. of a vector- 
potential a, These quantities satisfy the equations 


Oe 
Ag — — ae — 0. 
c? Of? Ss 
1 074, 1 1 O%a, 1 
AN DEN [Ge re ae tte, Une 6 rn 
a OF? as ms U, ET . Ly, etc 


so that, with the restrictions that are required if (3) is to be true, 
we may write 


EN A 
ofer 
| 


Am, 


1) Lorentz, La théorie ¢lectromagnétique de Maxwett et son application aux 
corps mouvants, Arch. néerl. T°, 25, p. 476 1892, 

2) See Levi Crvira, Nuovo Cimento, (4), vol. 6, p. 93 , 1897; WrecHERT, 
Arch. néerl., (2), T. 5, p. 549, 1900. 


if Egat ee 1 ] 
Arm I—[om]dS , a,=— |{— [ev] ds, ete. 
Ame ifs c Awe, f- ‘ 


After having found g and «a, we may determine the dielectric 
displacement d and the magnetic force bh by means of the relations *) 


Ley 
betrap ye ee 


C 


AL Nees aten atd andes ye OE 


It is to be remarked that the two potentials are not mutually 
independent; they are connected by the equation 

| i | 

TANN rt ar Nn MEDE Dea 


( 


Theorems corresponding to the principle of vb ALEMBERT 


and that of least action. 


§ 4. The physicists who have endeavoured, by means of certain 
hypotheses on the mecanism of electromagnetic phenomena, to deduce 
the fundamental equations from the principles of dynamics, have 
encountered considerable difficulties, and it is best, perhaps, to leave 
this course, and to adopt the equations (1)—(VII) — or others, 
equivalent to them — as the simplest expression we may find for 
the laws of electromagnetism. Nevertheless, even if we prefer this 
point of view, it deserves notice that the fundamental equations may 
be transformed in such a way that we arrive at theorems of the 
same mathematical form as the general principles of dynamics. This 
has been done especially by ABRAHAM in his important paper 
“Principien der Dynamik des Elektrons’™*). The considerations in 
this and the two next paragraphs agree with those of ABRAHAM, though 
presented in a form differing from his. 

We shall consider a system of electrons moving in the infinitely 
extended aether, and we shall fix our attention on the different 
states of this system, the aether included, that sueceed each other in 
the course of time in any electromagnetic phenomenon. From every 
one of these states we shall pass to another, differing infinitely little 
from it, and which we shall call the varied state. The variation 


or “virtual change” will consist in infinitely small displacements 9 of 


1) 1 shall write grad » („gradient of „”) for the vector whose components 
0p Op Ap 
are <— 


2) Drupe's Annalen, 10, p. 105, 1903. 
} 


( 613 ) 


the points of the electrons, accompanied by infinitesimal changes in 
the dielectric displacement. 

We shall write dd for the difference, in a fixed point of the 
aether, between the dielectric displacement before and after the 
virtual change, the sign of variation d having a similar meaning 
when it precedes other symbols representing the value of some 
quantity in a definite point. If it is affixed to a letter representing 
a quantity belonging to the system as a whole, such as the total 
electric energy U, it will simply serve to indicate the difference 
between these values in the original or real and the varied states. 

The variations to be considered are not wholly arbitrary. We 
shall limit our choice by supposing in the first place that each 
element of volume of an electron preserves its charge during the 
displacements q; this is expressed by the relation 

ase ie" (Oa) tN eke ete one ta oa ey MOE) 
which may be compared to (IL). 

In the second place we shall suppose the variations of ò not to 
violate the condition (1). | 

In virtue of these restrictions the vector 

dd + O4 
will present a solenoidal distribution. Indeed, we see from (I) that 
div dd = do, 
and here we may, according to (7), replace the right-hand member 
by — dw (o 4). 

Let us now conceive q and Jd» to be chosen for every instant f, 
so that they vary continuously with the time. Then, in order com- 
pletely to define the succession of varied states, or what we may 
call the „varied motion” of the system, we shall suppose the varied 
positions of the points of each electron to be reached at the same 
insiants at which these points occupy the corresponding original 
positions in the real motion; we assume likewise that, in every 
pomt of space, the varied dielectric displacement exists at the same 
moments as the original one in the succession of real states. 

By this the varied motion of electricity is entirely determined ; 
indeed, since we know the velocity of matter and the rate at which 
> changes, we are able to state what has become of the convection- 
current, the displacement-current, and also of the total current [. 
The first thing we have to do will be to express d{ in q and Jd, 
Of course we may be sure beforehand that the distribution of both 
the new ! and the variation dt will be solenoidal. This must neces- 
sarily be the case, because we know 1st. that, in the states that 
succeed one another in the varied motion, each volume-element of 


( 614 ) 


an electron retains its charge, and 2°¢. that the condition (D) is con- 
tinually fulfilled. 


§ 5. Let us begin by considering dw. This is the variation in 
a fixed point of space. Therefore, if (dv,) is the variation for a 
definite point of an electron, we shall have 

vx Ov, Ov. 
(Sox) = te den 1 Gy ay den, 
As to (dv), it is easily shown to have the value 
_ dj 
(do) = Er 


& dq. ; ee 
if we understand by fae the rate at which q‚ changes for a definite 


dt 


Ox 


point of an electron. Comparing this to 5, OF os the velocity of 
: : 


change in a fixed point of ae we get 


Oy: r Oja 
(de) = de + t= + Wy Oy + Ve ae 


These equations, combined with (7), lead us to 


dl = 0 (dr + 0 te) = diz + od, + vd = 


= J Da: a 0 Qa -- 0 Vr 
Oy, Ov, Oy 7 


— @ da = — Oy on — ede ya — yr div (a q). 
or, if we add to the second member the first member of (IT), multi- 
plied by q,, after some further transformation, 
Ogu 


dq 2 
vy = = + 0 bz dE div (0 q) — 


0 
Ne Di A es 
S [a a, Odrie Mere: ae en 


i) Vs 0 Dz oe Va i; ke 
— 04x aye 0 Ay iy —o4- au + qa div (v ») = 


0 0 0 
a OL (J De = Q Qa) + Oy lo (Gx Dii 0) | = ae lo (J- On — Oz b,) ]- 


Here we may remark that the two last terms taken together repre- 
sent the first component of the “rotation” of the vector whose com- 
ponents are 

0 (qy ve — Jz vy), 0 (Fz te — Gz vz), O (Az by — qy v2); 
and that this veetor is precisely the vector-product, multiplied by 
0, of q and v. After having calculated dl, and dl. in the same way 
as dl;, we may combine the results in the formula 


SS ee 


eS ae ee PE ee 


( 615 5 


d | =< (ABE eq ratio [Gath ree ee Ge) 

What has already been said about the solenoidal distribution of 

di is confirmed by this equation. The two vectors represented on the 

right hand side both have this property, the first by what we know 

of the vector dd + 04, and the second on account of the mathema- 
tical form in which it appears. 


§ 6. We may next proceed to determine the variation d7’ of the 
magnetic energy. In doing so we shall start from the assumption 
that the varied motion of electricity involves a definite magnetic 
energy '), to be determined as stated at the end of $ 1. 

The formula 


leads immediately to 
dT =|. dh + by dy + he dh-) S= fo . Sh) dS, 


Where the integration covers all space. The same will be the ease 
with the other volume-integrals appearing in the following transform- 
ations. If an integration is performed, or if the process of inte- 
gration by parts is applied, one obtains integrals over the infinite 
surface which we may conceive as the boundary of- the field of inte- 
eration. These surface-integrals however will be supposed to vanish. 
We begin by writing zot « instead of fh, as may be done in virtue 
of (5); and we shall next integrate by parts, keeping in mind that, 
on account of (V), 
: 


1 
ads 


C 


The result is 


1 
dE fee de dh) dS == fos . rot dh) dS = fa sdi sone memes "2 


or, if we substitute for dl its value (8), 


zefls [ot eal Jas + S(« rot | (ela. ely Jas. (10) 


Using (4), we may put for the first term 


') This assumption only means to define the value of 7’ we shall assign to the 
wholly fictitious varied state. 


ah 


( 616 ) 
Lie 
edt 


1 A 
== ale .{dd+09})dS fe {dd+og})dS+ | (gradg.{dd-+-9q})dS. (11) 
| cay 


Now, it appears from (9) that 


1 
— f(a. fod + onpas. ; ere | 
C 


is the change the magnetic energy of the system would undergo, if 
we gave to the current the change Jd + 9q. We shall write d’l for 
this variation of the current, and d'b, dT for the corresponding 
variations of § and 7. As to d’l, it may be defined as the current 
that would exist if the changes represented by q and dd were accom- 
plished in unit of time. 


Ene 
fee ten Hodes (a. {dd + eq) dS = 


On the other hand, fe-amas is the variation of the electric 
energy U and the last integral in (11) is 0, because the vector 
Jd Heg is solenoidally distributed. Thus, the first term in (10) becomes 

ao T 
dt 


+ dU + fe . oq) dS. 


For the last term in that equation we find, integrating by parts, 
1 ee Ghee irr as git Spee 4 
ay (rot Wie tolq : v|i)dS == jew A [ q- v| ) AE Fi 0 (4 [v - fy }) dS, 


so that finally 


dd'T ae; | 1 
dente A tfola- fette dS. 


Now, the equation (VII) shows that the last term is precisely the 
work done, during the displacements 3, by the electric forces exerted 
by the aether on the electrons. 

Writing d/# for this work, we have 


dd'T 
da De 
an equation closely corresponding to D'ALEMBERT's principle in common 


dE = 0 (T—U) — (13) 


dynamics. 


$ 7. The motion of the electrons themselves may be determined 
by ordinary methods; it will be governed by the electric forces 
whose work has been denoted by d#, together with forces of any 
other kind that may come into play. We shall confine ourselves 
to those cases in which these latter forces depend on a potential 
energy U; then the total virtual work of all forces acting on the 


( 617 ) 


electrons will be dE— dU. Moreover we shall aseribe to the 
electrons a certain kinetic energy 7, which they have by virtue of 
their mass in the ordinary sense of the word. Should there be no 
==); 

One of the forms that may be given to the variational equation 


€ . >? rs Vals, 7 . TO T Ay 
such “true” mass, we have only to put 77, 
of motion for a system of material particles is 


dd! T, . 
OA -— dT, 


dT, being the change of 7), if we pass from the real motion to 
some varied motion in which the varied positions are reached at 
the same moments as the original positions in the real motion, dA 
the virtual work of the forces, and d'7, the increment that would 
be acquired by the kinetic energy 7’, if variations, equal to the 
virtual changes of the coordinates, were imparted to the corresponding 
velocities (the coordinates themselves being kept constant). For our 
system of electrons 
JA dE dU; 
hence, if we use for d# the formula (13), 
(mp 
Cire TD zee =o: 
We shall finally multiply this by dé and integrate from f, to ¢,. 
In case both the displacements q and the variations dd vanish at 
the limits, we find 
ty 


| (7 =F 1) = (U -+ U;); di —— 
h 


This is analogous to the principle of least action. 


§ 8. In what precedes there has been question of the variations 
of the energies 7 and U, taken for the system of electrons together 
with the surrounding aether, which extends to infinite distance. 
Similar though somewhat less simple results are obtained, if one 
understands by 7’ and Cl’ the magnetic and the electric energies, in 
so far only as they belong to the space within an immovable closed 
surface 6. In what follows it is to be understood that this surface 
may have, relatively to the system of electrons, any position we 
like; for simplicity’s sake however we shall suppose that it cuts 
none of them, so that, in every point of 5, the density @ = 0. As 
to the virtual variations, determined by q and do, they need not 
at all be confined to the part of the system within the surface. We 
shall denote by # the normal to the surface, drawn towards the 


( 618 ) 


outside, and by à, u. r the angles between this normal and the 
positive axes of coordinates. 

If now we repeat the above calculations, we have to do with 
volume-integrals confined to the space within 6, and every integration 
by parts will give rise to a surface-integral. 

Thus. to the last member of (9) we shall have to add the term 

cos 2, COS U, COSY | 
Amr Ayn Mz | do =| la. Sh], do 


dh, 0). Jf) - | 
and the value of (12) will no longer be d'7’, but 


COS wh COS u. COS TY 


ee ope vedan le | d od || a.d'b]„ do. (14) 
dh dh 09:2 


The last integral of (11) becomes 


» 


of (grad @ . wot J'b}) a5 =< J oe grad g . dh) dS — ‘| [grad gy . dh |, do (15) 


e 

Here the first term on the right-hand side is 0, since vot grad p=0. 
The transformation of the last part of (10) remaining as it was, as 
we have supposed g@=0 in all points of the surface, we finally find 
for the second member of (13) the additional term 


ij i) 
| | — [a. dh], + fa. don +efgrad gp. ORNE 


Ot 


But, on account of (4), 


| 


[a : Sy |n +- c | grad q 5 dl 


a [et (20'D || aie Mente pal otha 
— Lo | : fa. dy ” e [grat pd hl 


\0d'h 
— En — 0 [D db, 


We get therefore, instead of (13), 

Eh doe Wa. (adh ae ee 
dd in —— Sf —e[d. d'b]x; do (LE) 

dt Ji: {08 | = 

§ 9. The following are some examples of the applications that 
may be made of the formulae (13) and (16). 

a. Let the virtual changes in the position of the electrons and 
in the dielectric displacement be proportional to the rates of change 
in the real motion, i.e. let 


== EU Od = ed, 


( 619 ) 


e being a constant infinitely small factor. From these assumptions 
it follows at once that 
ult Ik 05 Zei. 

Now the magnetic energy may be considered as a homogeneous 
quadratic function of the components of the current; it will therefore 
change in ratio of 1 to 1 + 2¢, if the current becomes (1 + <«)'. Thus: 
ESS nk 

We may also infer from our assumptions that the position of the 
electrons and the values of d are, in the varied motion at the time 
t, what they are in the real motion at the time ¢+ ¢, so that the 
only difference between the two motions is that the one is in advance 
of the other by an interval «. 

In this way it is seen that 

ae dU Of 0 d'l 


A eee (WG Ofer ae 1 Ee er tre 
Ae i dt ie Ot Ot ; 


Substituting these values in the equation (16), we get, after division 
by & and multiplication by df, denoting by d the work done by 
the electric forces in the real motion, during the time «4, 


IES AAH Oee f[d-blede. | REE Glug} 


This is the equation of energy. The last term represents the flow 
of energy through the surface. 

6. Applying (17) to a single electron, whose motion is a translation 
with variable velocity along a straight line, one may calculate the 
force with which it is acted on by the aether, and which, under 
certain simplifying assumptions, is found to be proportional to the 
acceleration and directed oppositely to it. The quotient of this force, 
divided by the acceleration, may appropriately be called the e/ectro- 
magnetic mass of the electron. 

c. There will likewise be a force proportional and opposed to 
the acceleration, if the latter is perpendicular to the direction of 
motion. In this case however, of which the uniform motion of an 
electron in a circle furnishes the simplest example, we must recur 
to the equation (16), in order to determine the force. The surface 6 may 
be supposed to lie at infinite distance and the virtual displacement 
must be taken in the direction of the acceleration. The ratio of the 
force and the acceleration may again be called the electromaynetic 
mass, though, except for small velocities, its value is not equal to 
that of the corresponding ratio in the case 5. 

In both cases the result agrees with what has been found by 
ABRAHAM, 


( 620 ) 
Ponderomotive action on a system of electrons. 


§ 10. A virtual change of a very simple kind is an infinitely 
small translation of all the electrons, combined with what we may 
call an equal translation in the same direction of the whole electric 
field. Applying to these variations — which we give as well to the 
part of the system outside the surface 5 as to the part enclosed by 
it — the equation (16), one may calculate the resulting force exerted 
by the aether on the electrons within the surface. This foree may 
be shown to consist of two parts, the first of which is the force with 
which we should have to do, if the surface 6 were subjected to the 
stresses in the aether, whose components have been already determined 
by Maxwern, whereas the second part is determined by the rate 
of change of a certain integral, relating to the space |S within o. 
The latter part will therefore vanish if the state is stationary, and may 
be left out of account if, for periodic states, we wish only to know 
the mean value of the resulting force, taken for a full period. I 
need not here work out the formulae, having formerly deduced the 
result in a more direct way. The components of MAXWELL’Ss stress are 


, 1 1 | 
A ZE > (d, 7 dv, FEE Ò a ) En BY ( Nee ae 7 —— {) ee 2 he etc. 
| (18) 


X, = dy ie ly ‚etc. 


and the just mentioned volume-integral is 


S, being the flux of energy in the direction 4, for which we seek 
the resulting force. 
Thus, the resulting force in the direction of is given by 


ce? dt 


Aen era! “ie 
z= f lee CdS So ee 


mf GEN 
The vector ol Sd S is called by Apranam the electromagnetic 
C t 
a 


momentum. 


$ 11. Similar results would be obtained if we chose for the virtual 
variation, instead of a translation, an infinitely small rotation about 
an axis passing through the origin of coordinates; the equation (16) 
would then serve to determine the resulting couple, arising from 
all the forces exerted by the aether on the electrons within the 
surface 6, The moment of this couple may however be calculated 


in a shorter way, if we start from what we know already about 
the forces. 

Indeed, in virtue of the formula (19) and the two corresponding 
to it, the components of the force acting on an element of volume 
dS may be represented as follows : 


OX, aig... OX» ee \ 
XdS = gh gen SAGs aE, dS] 
(S245 +52) prs 


a rh 48 0 Y, 0 ¥ Y 1 ~ Y 
nae dee Ke NGN 0 


Ou 


u dz c 
En ORN ar Lowe 
LAS = te dS Gyds 
\ Ov dz Ge 
and these formulae give a eee for the components of the 


couple 
iS mp eee kt Z EP fee ; 
[a VIS == fe n= 2 Yo) do — aa [es OSE le GEDE 


$ 12. Another consequence of the equations (20), analogous to 
the well known virial-theorem in ordinary kinetic theory, will perhaps 
be thought of some interest. In order to find it, we have only to 
add the three equations, multiplied by we, y, 2, and to integrate the 
result over the space S, within the surface o. Transforming such 


= 


“ly = 5 3 ‘ J 
terms as | wv dS by means of partial integration, we find 
ó wv 


| (Xe + Yy + Zz) dS = | Kur + Yoy + Ze) do — 


= [G+ % +2 dS — [Eer + Ey + ez) dS. (22) 


For stationary states the last term will vanish, so that, if we 
substitute in the term preceding it the values (18), 


fe + Yy + Ze) dS = fis, ®d Yn y + Zn 2) do + 1 + U. 


Particular cases of ponderomotive action. 


$ 13. In a large variety of cases, in which the system of electrons 
is confined to a space of finite dimensions, the electric and magnetic 
intensities in the surrounding field become so feeble at great distances 
that the surface-integrals in 19) and (21) approach the limit O, if 


the surface 5 moves to infinite en Moreover, the volume- 
integrals will vanish if the state is stationary. We then come to 


the conclusion that the resulting foree and the resulting couple are 
O for the whole system. If the system consists of two parts A and B, 
we may express the same thing by saying that the total pondero- 
motive action on one of these is equal and opposite to the total 
action on the other. 

Of course this will be equally true if, for a system whose state 
changes periodically, we have only in view the mean ponderomotive 
action during a full period. 

These theorems are useful whenever the phenomena in one of the 
parts, say in A, are not well enough known to permit a direct cal- 
culation of the force acting on this part of the system. If the pheno- 
mena in B are less complicated, so that we encounter no difficulty 
in determining the force or the couple acting on this part, the action 
on A will be found at the same time. 

We may apply this in the first place to well-known experiments 
on electromagnetic rotations. 

Let us consider a cylindrical magnet, touched in two points 
of its surface by the ends of a conducting wire JV. Let this wire 
be the seat of an electromotive force, producing a current that 
flows through JV and through part of the magnet. The ponderomotive 
forces acting on the wire are known with certainty and may easily 
be deduced from the formula (VII); they produce a couple, tending 
to turn the wire about the axis of the magnet. Without entering into 
any speculations concerning the motion of the electrons in its interior; 
we may infer that the magnet will be acted on by an equal couple 
in the opposite direction. 

Of course this reasoning must be justified by showing that the 
surface-integral in (21) is really O, if it is taken for a surface at 
infinite distance. This is readily seen to be the case, if we keep in 
mind that, at great distances, the magnetic force produced by the 
system varies inversely as the third power of the distance, and that 
the intensity of the electric field, if it exist at all, will certainly contain 
no terms diminishing more slowly than the square of the distance. 

. 

§ 14. 1 shall choose as a second example some experiments, lately 
made by Wuirrnkap') for the purpose of testing a consequence of 
Maxwerr’s theory that has been admitted by many physicists and is 
unavoidable in the theory of electrons, viz. that a ponderable dielec- 
tric, which is the seat of a variable dielectric displacement, and 
therefore of a displacement-current, when placed in a magnetic 


1) Warregeap, Ueber die magnetische Wirkung elektrischer Verschiebung, Physi- 
kalische Zeitschr., 4, p. 229, 1903, 


( 623 ) 


field, will be acted on by a similar force as a body carrying a con- 
duetion-current. In WHITEHEAD’s apparatus two cylindric metallic 
plates, having the same vertical axis PQ, formed a condenser, 
in which a rapidly alternating electric field was maintained; at 
the same time alternating currents were passed through the horizontal 
windings of a circular coil, surrounding the condenser; the axis of 
the coil, which is at the same time the axis of its magnetic field, 
coincided with PQ. A sensitive torsion-balance was suspended by a 
wire passing along the axis of the instrument; the ends of the beam 
carried each a piece of some solid dielectric, so that these two equal 
pieces hung, diametrically opposite each other, in the air-space 
between the condenser-plates. The two fields, the electric and the 
magnetic, had exactly the same period, being produced by the same 
alternate current-machine; besides, the arrangements were such that 
there was a phase-difference of a quarter period between the two 
fields. Thus, at the instants at which the magnetic force had its 
maximum values, the rate of change of the electric field and conse- 
quently the intensity of the displacement-current was likewise at its 
maximum. Under these circumstances a sensible couple acting on the 
dielectric was expected, but no deviation of the beam, attributable 
to such a couple, could with certainty be observed. 

We may remark in the first place that in Wurreneap’s formula 
for the expected effect, the specific inductive capacity A appears in 
the numerator. If this were right, a couple would act on the aether 
between the plates itself. According to the theory of electrons, as here 
presented, ponderomotive force acts only on the electrons contained 
in ponderable bodies, but in no case on the aether. The theory 
therefore regards every ponderomotive action as due to the difference 
between the properties of the body acted upon and the aether; it 
can lead to a formula containing in the numerator A—1, but never 
to one, containing, instead of this factor, the coefficient A’ itself. 

In the second place Wourrpurap has overlooked a circumstance by 
which the effect he sought for must have been, at least for the greater 
part, compensated. The compensation may be shown to be complete 
if the properties of the dielectric used differ from those of the aether 
to so small extent, that quantities which are in this respect of the 
second order of magnitude, i. e. of the order (A—1)*, may be neglected. 

If this may be done, the ponderomotive action on a ponderable 
dielectric, placed between the condenser-plates, may be considered not 
to be altered by the presence in the field of a second or third piece 
of the same dielectric. Now, the two bodies suspended at the ends of 
WHITEHEAD’s torsion-balance may be taken to have been parts of a 

42 

Proceedings Royal Acad. Amsterdam. Vol. V. 


( 624 ) 


complete dielectric ring, bounded by a surface of revolution with the 
axis PQ. Moreover it will be safe to assume that the action on the 
two bodies which it was sought to observe, did not depend on their 
relative positions with respect to the wires leading to the condenser- 
plates, and remained therefore the same, in whatever position the 
torsion-balance was turned. If this was the case, the action on 
a body that is the #'h part of the ring (being cut out of it by two 
planes passing through the axis) must have been the 2 part of the 
couple, acting on the complete ring. Consequently, it will suffice to 
show that the effect is 0, if the experiment is made with a complete 
dielectric ring. 


$ 15. For simplicity’s sake we shall suppose the condenser-plates 
to be united by a wire W and their alternating electric charges to 
be produced by a periodic electromotive force in this wire. As to the 
currents in the coil, they may be regarded as due to electromotive 
forces of the same period, acting in the windings themselves; indeed, 
the action on the dielectrics can only depend on the magnetic field 
and not on the way in which it is produced. For this same reason 
it is allowable to ascribe to the windings so small a resistance that 
they do not carry any appreciable charges. 

Then no other but electromagnetic forces will act on the windings 
of the coil and these cannot give rise to any couple about the axis 
PQ, because such forces are perpendicular to the elements of the 
windings. By the theorem of § 13 the couple acting on the torsion- 
balance must therefore have been equal and opposite to the moment 
of rotation, acting on the condenser-plates and the wire W. It remains 
to show that this last moment has been 0. 

I shall denote by I the electromotive forces acting in the connecting 
wire JW, by II those existing in the windings of the coil, and I 
shall distinguish by the suffixes 1 and 2 the states arising from these 
two causes. Let us indicate by 4, the charges of the plates and 
the currents in these and the wire W, in so far as they are due to 
I, and let A, have the same meaning with respect to II; also, let 
F, and F, be the electromagnetic fields excited by the two causes. 
In each of these fields there will be an electric force Dd (acting on 
charges that are in rest), as well as a magnetic force bh; in virtue of 
the first, the field will exert a ponderomotive force on the charges 
of the plates and in virtue of the second on the currents, one of 
these actions being determined by the first, and the other by the last 
term in the general equation (VII). If we denote by the symbol (Pf, A) 
the couple acting on the plates and the wire, in so far as it is due 


( 625 ) 


to a field F and a state A of these bodies, the two actions we shall 
have to consider may be represented by 
| (Fil A.) and. (F,; Ay) 

The first of these is readily seen to be 0. Indeed, the magnetic 
field, produced by the forces II, though modified by the presence of 
the dielectric ring, is symmetrical around the axis PQ. Therefore, 
if the periphery of the condenser-plates is nowhere interrupted, the 
state A, will consist in circular currents in these plates, without any 
electric charge. It is impossible that the field #, should, by its 
action on these currents, give rise to a couple, since, whatever be 
the nature of this field, each element of the stream-tubes will only 
be acted on by a force perpendicular to its length. 

In reality the case was somewhat different, each condenser-plate 
being cut by a vertical slit. There must have been equal and 
opposite charges at the edges of each slit and the field #, must 
have acted on these charges, in virtue of the electric force existing 
in it. These forces may however be supposed to have annulled 
each other, because the distance between the charges on the two 
edges was very small. 


§ 16. The action (#, A,) is therefore the only one that remains 
to be considered. Now, in the state A,, the plates of the condenser 
were the seat of charges, whose amount was modified by the 
influence of the dielectric ring, and whose alternations were accom- 
panied by currents in the wire W and in part of the plates them- 
selves. In so far as they are currents of conduction, i. e. in so 
far as they consist in a motion of electrons, these currents are evi- 
dently unclosed. We may decompose the whole system of them into 
infinitely thin stream-tubes, the tubes being all thronged together in 
the connecting wire, and widening out in the plates, at whose sur- 
faces each stream-tube ends in two elements of surface. 

Let S be one of the stream-tubes, G the end of it on the outer, 


and A that on the inner plate, e the charge in G, — e that in H, 
de 93 

(= la 
dt (28) 


the current in the tube in the direction from H towards G, and let 
us consider the action (/’,, A,) only in so far as it depends on this 
current ¢ and on the charges e and — ve. 

In the first place there will be an electromagnetic force on the 
tube S, owing to the current ¢. The couple arising from it depends 
on the course of the magnetic lines of force in the field /’,; it is 
most easily found by remarking that its work during a complete 

J 49% 


( 626 ) 

revolution of S about the axis PQ is numerically equal to the product of 

by the number of lines of force that are cut by JS. These lines 
C 
are precisely those that are intersected by the surface described by 
S in its revolution, a surface which may have different forms, accor- 
ding to the form of the wire IW, but has at all events for its boun- 
daries the circles described by the points G and //. Let MN be the 
number of these lines, taken positive if the middle one of them passes 
upwards along PQ, and let us take as positive directions for the 
rotation and for the couple the direction corresponding to the upward 
direction. Then, for a full revolution in the positive direction, the 


Ne 
work of the couple will be — —4 M, whence we find for the couple 
jd 


itself 
1 


——iwW. ee oe 
22 


. (24) 

If this were all, we should indeed come to an effect such as was 
expected by Wuirrnnap. We must however keep in mind that there 
can never be a variable magnetic field without electric forces. Such 
forces, represented in direction and intensity by the vector >, will 
exist in the field /’,, the lines of electric force being circles around 
the axis PQ. 

We must therefore add to (24) the couple arising from the action 
of the field on the charges e and — e; its moment may again be 
found by considering the work done in a complete revolution in the 
positive direction. 

The force on the charge e being ed, its work is equal to the 
product of e by the line-integral of d along the circle described by 


G. Similarly, the work of the force acting on the charge — e in H 
is the product of — e by the line-integral of 5 along the circle 


described by #H, or, what amounts to the same thing, the product 
of + e by the line-integral for this circle, if it is taken in the 
negative direction. Now, if we follow the circle G in the positive 
and the circle #7 in the negative direction, we shall have gone along 
the whole contour of the surface described by the stream-tube $, 
in a direction corresponding to the positive direction of the magnetic 
force. Hence, by a well known theorem, of which the fundamental 
equation (VI) is the expression, the sum of the two line-integrals by 
which e must be multiplied, will be 


( 627 ) 


and the couple to be added to (24) will be given by 
1 dN 
Que dt 
Taking into account (23), we find for the total couple 


1 IN ‘ N 
Mind (ive ,)=- 5D) 
2e 


dt Once dt 


Since this is the rate of change of a periodic quantity, the mean 
value will be 0, as above asserted. 


The above somewhat complicated reasoning has been used in 
order to avoid the difficulties arising in a closer examination of 
the phenomena going on in the ponderable dielectrics. The result 
may however be verified by making suitable assumptions concerning 
these phenomena. It will suffice for our purpose to replace one of 
the dielectric bodies by a single pair of electrons A and B, the 
first of which is immovable, whereas the second may be displaced 
over an infinitely small distance, in a radial direction, by the electric 
forces of the field #,. We shall denote by —e and + ¢ the charges 
of A and B, by r the distance of A to the axis, by s the infinitely 
small distance A B, and we shall write bh. for the vertical component 
of the magnetic force in the field /, and D for the value of the 
delectric displacement in this field at a distance 7 from the axis. 
We shall take the positive directions as follows: for s outwards, for 
hb, upwards, and for D along the circular line of electric force in 
a direction corresponding to the positive direction of bh, i.e. in the 
direction of a positive rotation about the axis. 


ds 
Now, owing to the velocity 5 of the electron B, there will be, 


„according to the formula (VII), a force 

6.308 

edt 

acting on this electron along a circle about the axis, and producing 


a moment 
2 ds 

th ENT MR a er | 
This is the couple of which Wurrenrap has sought to prove the 
existence. It is however annulled by the moment arising from the 
action of the field /, in virtue of its electrie force D. For the 
particle A this moment is 
—erD 


„and for the particle B it is obtained if we replace —e by +, 


( 628 ) 


taking at the same time the value of 7D at the distance r+s from 
the axis. 
The algebraic sum of the two moments will therefore be 


0 
e a (7 D) 


and for this we may write 


Ee Ob: oi 
mid 1 SN 
since, by the equation (VI) 
1 0b: 
5e (7 ES rea =? 


For the sum of (24’) and (24’’) we may write 
é d (s fy-) 
MEET : 


c dt 
whence it is immediately seen that its mean value is O for a full 


period. 


Physics. — Methods and apparatus used in the eryogemc laboratory. 
ITT. Baths of very uniform and constant temperature in the 
cryostat (continued). A cryostat of modified form for appa- 
ratus of small dimensions. IV. A permanent bath of liquid 
nitrogen at ordinary and at reduced pressure. V. Arrange- 
ment of a BurckHarpt-WEIss vacuum-pump for use in the 
circulations for low temperatures. Communication N°. 83 (con- 
tinued) from the Laboratory at Leiden. By Prof. H. KAMERLINGH 
Onnes. (Read February 28, 19053). 


UI § 6. A cryostat of modified form for apparatus of small 
dimensions. If the cross sections of the apparatus that is to be immersed 
into the bath are small, vacuum glasses may be profitably used in 
the construction of the cryostat. For, vacuum glasses of comparatively 
small diameter can then accommodate the stirrer and the temperature 
indicator in addition to the measuring apparatus. Plate IV shows a 
cryostat of the kind, viz. the one used in the determinations by 
HynpmMan and myself on the critical state of oxygen. | 

Obviously the arrangement could be much simpler, as it was not 
necessary to watch the liquefied gas streaming from the jet or to use 
the generated cold vapour for the cooling and as no particles of dust 
from the leads had to be feared, a filter was not required. (Comp. Comm. 
51, Sept. 99 § 2. Y, p. 12). The principles for obtaining a uniform con- 


~ "ta 


( 629 ) 


stant temperature, laid down in the previous communication have all 
been applied in this arrangement, a vigorous stirring with the ring 
shaped valved-stirrer, the adjustment at the desired temperature to the 
indication of a sensitive indicator by regulating the pressure at which 
the liquid boils while reading a differential oil-manometer made for 
the purpose, and lastly the determination of the temperature of obser- 
vation as corresponding with the mean obtained graphically of the 
readings of the thermometer (as in § 5). 

Plate V shows in detail the differences in the construction between 
this form and the former plates I and II (and also Plate I Comm. 51), 
the parts unaltered remaining are indicated by the same letters as 
before, and the modified parts by letters with accents, while entirely 
different parts have new letters. 

The height of the vacuumglass 5',, is so chosen that the liquefied 
gas cannot be blown out; and the glass itself has been silvered, 
leaving open two opposing windows V',. Through these the pheno- 
mena in the experimental tube may be watched, and from the position 
of an aluminium wire fastened to a cork float the depth of liquefied 
gas may be derived. If the insulating power of the vacuumelass is 
not perfect, condensation of moisture on its outer wall may be avoided 
by placing it into a beaker filled with alcohol, which if necessary 
is renewed when cooled. Thus the same principle is followed which 
was employed when necessary in the case of the cryostat (Comm. 51) 
when the windows had to be kept clear and where hot dry air was 
drawn through the outer spaces of the observing glasses (V,, see 
Pl. I of this Comm. and for the details pl. I Comm. 51). 

The vacuum glass and the auxiliary apparatus are supported by a 
copper cover V',,, with its rim tinned to protect it from the action 
of the india-rubber ring V',, and which, like the cryostat of § 1, has 
been coated with polished nickel-paper. To this cover are fastened the 
exit tube of the gas 7, and the safety tube Y,,, the connection 
A', with the oil manometer (for details see plate I) and a copper 
tube .V’,,, into which the india rubber stopper is placed holding the 
apparatus to be immersed in the bath (in our case the piezometer 
for the critical phenomena X,, and the correction thermometer 6,, 
with its leads 5, (comp. $ 1) while the thermo-element @ may be 
considered as forming an inherent part of the cryostat). There is 
also a tube through which the capillary a, admitting the liquefied 
gas is led and where it is supported by a piece of cork a’, It is 
closed by means of an india-rubber tube a’,, drawn over the tube 
and a thin cap soldered on to a 

Between the cover and the rim of the vacuum glass a wooden 


630.) 


cylindrical jacket N', is placed resting against the latter by means 
of an india-rubber ring N’,. Two cylinders N',, N', of nickel-paper 
serve to diminish radiation, especially in the direction of the delivery 
tube. 

As mentioned the frame which keeps the protecting cylinder in its 
place is fastened to ihe cover. For a complete explanation of the 
letters and parts of both this and the stirrer reference may be made 
to § 4. Further we may note that §, is fastened with silk cords 
to &, and this again with silk cords to the cover W’,,, while §', is 
supported by the glass tube &, fitting onto the pins §',. 

The three threads 4, on which the stirrer hangs are led directly 
through the three india-rubber tubes y',,, connected hermetically to tubes 
soldered onto the cover and fitting hermetically onto the threads at 
x',2, to the brass disc 4’, and rod y',, which is connected by a 
small chain y',; passing over a pulley y',, to the motor by means 
of a steelwire. The arm of the motor may be adjusted to different 
throws, while velocity of rotation can be regulated by means of a 
rheostat. 

The mounting of the apparatus is very simple. The stopper with 
the measuring apparatus is placed into the tube .V’,, of the cover, 
to which all the auxiliary apparatus has been connected, then the 


vacuum glass is slid into the india-rubber ring which is also connected 


to the cover and is fastened there by means of tightening bands. In 
order to secure an airtight fit the india-rubber on the metal and on 
the glass has been coated beforehand with a solution of indiarubber 
in benzine. 

With a view to the description given in III the operations for 
the adjustments at given temperature require amplification only ina 
few points. In the case considered here, the evaporated gas was led 
back through the exit tube to the gasholder or to the large exhausted 
reservoir of the ethylene circulation in the cryogenic laboratory 
(Comm. 14, Dec. ’94) whence the ethylene was further condensed 
into the condenser immersed in methyl chloride. As described in 
Comm. 14 the circulations of the cryogenic laboratory have been so 
arranged that they may be used at any time. Besides the reservoirs 
that have to be exhausted, a permanent part of the circulation consists 
in branched tubes with cocks as shown on plates I and IV. The 
cryostat had only to be connected to the circulation in order to be 
easily brought to the required pressure. In the case considered here the 
experiments. were not made in the cryogenic laboratory but in an 
other room and the length of the lead a’,, was 10 m. Although 
the liquid ethylene had to be conducted over such a distance, yet 


end 


( 631 ) 


the adjustment of the bath to the required temperature (say at — 120°) 
was obtained within one hour after the pumps in the cryogenic 
laboratory had been set working. 

Instead of a resistance thermometer, to regulate the temperature, 
we used the thermoelement ©, the protected junction being placed 
at the side of the piezometer (comp. comm. 27 June ’96); it is visible 
through the window V', (in plate IV). The electro-motive power of 
the thermoelement is compared by means of the zero method with 
that of a thermoelectric control element or a Weston-element. 

For the same difference of temperature the deflections on the seale 
of the sensitive galvanometer were almost as large as in the measure- 
ments made with the resistance thermometer (comp. $ 5). An example 


of the determination of the temperature is not necessary in addition 
to Plate III. 


IV. A permanent bath of liguid nitrogen at ordinary or reduced 
pressure. In Comm. 14 (Dec. ’94) a short description was given of the 
temperature steps obtained by means of circulations of methylchloride, 
ethylene and oxygen. In connection with that description I mentioned 
my intention of adding more circulations to those already existing 
and said that I hoped to replace more and more parts of the existing 
circulations by greater and to insert such technical apparatus as 
should be found advisable so that the existing apparatus could be 
used in the new circulations with pure or costly gases. An example 
of this is the circulation of nitrogen added to the existing temperature 
cascade, of which a description is now required by the completion 
of some of the measurements rendered possible by it. For measure- 
ments at temperature between — 195° C. and — 210° C.a nitrogen 
is much to be preferred to an oxygen-circulation as the tension at 
which the oxygen boils at — 195° is so small that accurate regulation 
at constant temperature becomes very difficult. As the preparation of 
pure nitrogen in such large quantities as a circulation requires 
presents many difficulties, the compressor and the vacuum pump 
must be suitable and efficient. These conditions are fulfilled by the 
mercury and the auxiliary compressors which are generally used for 
the compression of pure gas and which in the originally tempera- 
ture cascade served for the oxygen circulation. However when the 
BroTHERHOODcompressor (comp. Comm. 14 Dee. "94 and 51 Sept. ’99) 
could be used for the oxygen circulation in the cascade they could 
be used for the nitrogen circulation. 

The nitrogen is prepared from sodium nitrite. Besides being passed 
-through ferrous sulphate and sulphuric acid it is led over hot cop- 


( 632 ) 


per and then again through ferrous sulphate and sodium hydroxide, 
because otherwise traces of nitric oxide might be left and this blocks 
the cocks (this gas is recognised at once by a strong smell of higher 
oxides of nitrogen when it mixes with the air). In order to remove 
traces of this oxide, I have sometimes added to the gas a quantity of 
oXygen as nearly as possible equivalent to the NO contained therein 
and have then passed it through sodium hydroxide. The gas is col- 
lected and provisionally kept in galvanised iron vessels holding 1 M*. 
From these it is driven out later by water heated by a steam jet 
and after passing through sodium hydroxide and sulphuric acid it is 
forced into a small gasholder floating on oil and holding 500 L. 
By means of the auxiliary compressor AC lubricated with glycerine 
(see Pl. VI and for details Comm. 54 Sept. *99) and the mercury 
compressor HgC (see Pl. VI and for details Comm. 54) the gas is 
forced over into a metal cylinder of 18 liters capacity after passing 
through the drying tubes D,, D, filled with caustie soda in the form 
of sticks. 

Plate VI shows the scheme of the entire circulation with the 
cryostat Cr, into which the liquid nitrogen is admitted at a and where 
it evaporates under ordinary or reduced pressure at the desired tem- 
perature. The whole arrangement has been used in the comparison 
of the platinum resistance thermometer with the hydrogen thermo- 
meter, which has been mentioned in II. The apparatus themselves 
are drawn diagrammatically but in their true proportions, while the con- 
nections are entirely schematic. A detailed representation of the cryostat 
with the auxiliary apparatus appertaining to it for uniform and constant 
temperatures will be found on plate I where the same letters have 
been used. On the other hand plate VI may be considered as a sup- 
plement to plate I. Nothing is wanting for a complete representation 
of the circulation except the gasholder and the vacuum vessel of 
5 M*. (comp. § 5 for its use) which are too large to be repre- 
sented on the same drawing as the parts given. There is an 
insignificant difference in the coupling of the leads between plate l 
and plate VI, for on plate VI Zeh. 1' indicates the connection of the 
compression side of a BurckHarpt—Welss vacuumpump bu Vac., 
described below into which the exhaust Hvh. 2 terminates, to an 
exhaustpump (which may also be AC of the circulation). Moreover 
next to the lead from Y, to Y,, we have drawn what must be sub- 
stituted for it in comparison with the arrangement on plate IV. 

RN is the cylinder where the nitrogen has been compressed by 
means of AC and HgC through the drying tubes D, and D,, while 
Gaz indicates the 500 liter gas holder floating on oil. The nitrogen may 


—————— en …_- — dd 


( 633 ) 


be admitted at the required pressure into the condensation spiral CS 
from the cylinder RN through a final drying tube D, containing phos- 
phoric anhydride, as well as directly from the compressor. The spiral is 
placed in a vacuumglass B with a protecting cylinder A. Liquid oxygen 
is admitted into B through Oxz./iq from the oxygen circulation of the 
eryogenic laboratory, viz. from the condensation spiral which is cooled 
in the ethythene boiling flask (Comm. 14, Dec. ’94). The oxygen escapes 
through Owv.vap, a wide safety tube S being connected in the ordinary 
way, and is compressed into the spiral by a BROTHERHOOD-COMpressor 
which is lubricated with glycerine and arranged as deseribed in 
Comm. 51. It may be remarked that, with a view to the possibility 
of an explosion of a glycerine mist mixed with oxygen, the pressure 
in this operation is not raised above 80 atmospheres. (Comp. the 
explosion described in the Zeitsch. f. Kohlensäure Industrie 1903). 

The nitrogen condenser itself has been drawn in detail on plate 


VII. In so far as the parts correspond — either with plate V for 
the cover, or with plate I of Comm. 51 for the regulation cock 
described there — the same letters have been used, but as some of 


the parts differ a little the letters have an additional accent. As in 
the case of the small cryostat plate V, the cover is coated internally 
with nickel-paper, while the upper turns of CS are protected again 
by a ring of paste board and nickel-paper. The condensation spiral 
consists in the condenser proper CS, and the regenerator CS,; here 
the same principle has been applied which has been followed in the 
cryogenic laboratory from the first (Comp. Comm. 14 Dec. *94); the 
vapour of the oxygen is forced by the cylinder B, which is closed 
at the bottom with the stopper B",, to pass along the regenerator spiral. 
As in the ethylene boilingflask (see comm. 14 Dec. ’94) the level 
of the liquid oxygen in the glass tube W is indicated by a cork 
float dr, with a steel capillary dr, to which a thin reed d, is 
fastened; the steel capillary passes through a glass tube b’,,. 

Liquid nitrogen flows out through the fine regulatingcoek hh, of 
the same kind as that through which the liquid gas is admitted into 
the cryostat. For the description of this cock compare Comm. 51 
and 54. 

It may be added that Gaz’ shows the connection with the auxiliary 
apparatus described in Comm. 54 for operations where HgC is used, 
which connection make it possible for the gas to stream back to the 
gasholder Gaz. | 


V. Arrangement of a BorcKkHarDt-Weiss vacuumpomp to be used 
with a circulation for low temperature. The well-known excellent 


(26347) 


vacuumpump patented by BurckHarpt and Weiss has been first used, 
I think by Orszewski, for removing the large volumes of gas which 
rise from a bath of liquefied gas at a reduced pressure. We shall 
now speak of some modifications and auxiliary apparatus by means 
of which the perfect purity of a gas is secured in a high vacuum. 
A pump arranged in this way may also be introduced into circula- 
tions of costly gases. In our laboratory it has been worked very 
satisfactorily for many years. A diagrammatic figure of the entire 
BurckHArDT-pump has been given on plate VI Bu. Vac., the pump 
cylinder with its slide valve box, the beginning of the suction- and 
the delivery tubes with the auxiliary apparatus belonging to them 
are shown on plate VIL, where fig. 1 gives the side elevation, fig. 2 
the top elevation and fig. 3 the section. The well-known working 
of the piston and the valve, the successive communication of the 
valve ports 5 and 5’, each individually by means of the slide hole 
2 with the suction valve port 1 or with the delivery valve port 4 
and together by means of the ringshaped opening 3 may be seen 
without further comment from the section. The pump displaces 
360 M? an hour, hence, when exhausting at a pressure of 2 ¢.m., 
about 10 M*® gas, measured normally can circulate. At Leiden it is 
used almost exclusively with an additional vacuumpump exhausting 
at the compression side. It exhausts then till 2 m.M. 

As a lubricant and for the airtight fittings to be described in the 
following pages, only bone-oil is used which after having been tested 
at the exhaustpump has proved to have no perceptible vapour pressure. 

For the technical work ordinary ring packings are quite sufficient, 
I have, however, replaced them by folded packings as described in 
Comm. 54 Jan. ’00 for the compressor and the auxiliary compressor. 
The leather ring of the packing is supported there as in Plate IV 
b,, by the india rubber ring b,, (for an exhausting packing comp. 
E,, Pl. VI fig. 3 Comm. 54). The packing cylinders have been made 
long enough to contain two folded packings (one for exhausting and 
one for compression) and a bronze tightening piece, but as a rule 
they only hold the packing for exhaust. 

New additions are the vessels 0, and O, see also plate II filled 
with oil (or with glycerine for those gases which cannot be used 
with oil); they serve to protect the packing cases of the cylinder 
and the slide valve box entirely from the atmosphere and also to cool 
the piston rod. The covers O,, and Q,, protect the lubricant against 
dust or moisture. 

For the oil holders S,S, we have chosen the construction explained 
in detail in fig 7.~S,, is an ordinary oilpot for visible cylinder lubri- 


KAMERLINGH ONNES. Methods and apparatus used in the Cryogenic Laboratory. III. Baths 
of very uniform and constant low temperature (continued), A Cryostat of modified form 


for apparatus of small dimensions. 


Plate IV. 


ad 
‘Pesedings Royal Acad, Amsterdam, Vol. V. 


Plate V. 


Mn 


5 wr 


NT 


| 


mmm nnen mens 


— „à 


Plate VIL, 


1 KAMERLINGH ONNES. Methods and apparatus used in the Cryogenic Laboratory. IV. Permanent bath of 
liquid nitrogen. 


Plate VL 


SEN 


so 
| 


El 


- 
L 


Lees 


Protecdi 
toceedings Royal Acad. Amsterdam. Vol. V- 


KAMERLINGH ONNES. Methods and apparatus used in the Cryogenic Laboratory. V. Arrangement of a BURCKHARDT-WEISS 
H. 4 
vacuumpomp for use in the circulations for low temperatures. 


Plate VI. 


OT 


Proceedings Royal Acad. Amsterdam. Vol, V- 


(6359) 


cation in vacuo. The cover 5S,,, has been tightly screwed on the 
hollow rod S,,,, and presses the glass S,,, hermetically on to the 
packings. By means of the winged nut /S,,, the point is adjusted 
so that the oil drops regularly through the openings JS,,,, into the 
space S,,, which communicates with S,,, through S,,, and which 
may be watched through the glass windows in S,,,. For our purpose 
the oil holder S,, is placed on a stout tube S,, onto which by 
means of india rubber rings and tightening bands the glass cylinder 
S,, is fixed on a copper bottom, soldered to S,,. The glass cylinder 
is filled with oil and covered with a lid $,,. By means of S,,, new 
oil can be admitted from the reserve vessel into the lubrication 
vessel. In this way the air is sufficiently prevented from entering 
the lubrication apparatus. 

Lastly, between the exhaust tube z and the compression tube p 
a safety valve has been placed, which prevents the pressure on the 
compression side from rising above a certain height (usually */, atmos- 
phere). Hence it is possible to let the pump work on and to open 
and shut the cocks as the work requires. The noise of the safety 
valve gives warning that the cocks have not been properly used. 
In any case no difficulty is to be feared if the possible output of the 
pump might diminish in any way in relation to the intake. Fig. 4 
shows a diagram of this connection, some of the parts being drawn 
to proportion ; fig. 6 shows a section of the safety valve case itself, 

The side tube p, is connected by a joint A with the tube wv, 
which opens into the space below the safety valve. The space above 
the safety valve communicates with the exhaust tube through the side 
tube z,. The broad valve v, is coated at the bottom with an india 
rubber sheet which presses against the narrow rim v,. The spring 
v, is stretched with the key v, while the plate v, with the nut »,, 
and packing is tightly screwed on to the rim 7,,. The packing 
cylinder v,,, like the packing just mentioned is kept under oil; a 
cover v,, above it protects it from dust. 

The connection K between the tubes p, aid v7, could not be brought 
about with flanges or with screw joints without causing tension in 
the tubes. Therefore it was made in the following manner as shown 
by fig. 5. A widened piece #, is soldered on p,, v, fitting into 
this piece. The india rubber connection &, is kept in oil; for this 
purpose a rim #, was used which was soldered on to p, and a 
rim /:, which was soldered on to z,. Over these rims a wide piece 
of tubing #, is drawn which is fastened to #, and 4, by means of 
india rubber rings /, %, and tightening bands, and forms together 
with these an oilreservoir. 


125 


( 636 ) 


Besides being connected through the safety valve case and the 
above mentioned connection, the compression tube and the exhaust 
tube are also connected (comp. again the diagrammatic fig. 4, as an 
explanation of figs. 1, 2, 3) by the cocks 7,,7,,7,,7, and may be 
connected with an airpump /, an indicator 7 and a vacuummano- 
meter m. The use made of this auxiliary apparatus in regular working 
or in preparing, mounting, testing, drying and exhausting the pump, 
requires no further explanation. As a matter of course, the pump 
is not introduced into a circulation unless it has worked for a long 
time with the exhaust- and compression sides closed and no change 
has been found in the vacuum. 

I further remark that the principle of an oilconnection as illustrated 
by fig. 5 may be profitably applied when wide tubes have to be 
connected, which have neither flanges nor nuts and joints or in cases 
where it is not advisable to make these contrivances. The method then 
to be followed is illustrated by fig. 8 where K’,, A’, and A’, are 
loose pieces slid on the tubes 6, and 6,. which we want to connect 
A good fit is obtained by means of the india rubber rings A’,,, 
K’,,, K’,, K’,, K’,, under brass tightening bands. K’,, and A, 
serve to admit and to run out the oil. In this way one always suc- 
eeeds in making within a short time an airtight fit. For the connec- 
tion of the pump tubes to the conduit at 7, and f, (comp fig, 1) 
this method has been used in a manner which will be clear from 
the figure. 


Physics. — Communication n°. 84 from the Physical Laboratory at 
Leiden “Zsotherms of diatomic gases and their binary mixtures. 
V. An accurate volumenometer and nuving apparatus.” (By 
H. KAMERLINGH Onnes and H. H. F. HyYNDMAN). 


§ 19. A compression tube of larger dimensions. In $ 6 of Comm. 
n°. 69 March 'Ol we have explained that the apparatus described in 
§§ 3 and 4 hardly gave the accuracy required in the determinations of 
density, if the total quantity of compressed gas was smaller than 
5 ec. Since, however, at most 600 cc. of gas under normal condi- 
tions is available in this apparatus it is not suitable for densities 
of more than 120 times the normal. 

On Pl. L a compression tube is shown which has about three 
liters capacity and hence which is suitable for measurements up to 
densities of some 500 times the normal and with at least the same 
accuracy as the above. The drawing is, as usual, schematic in 


the connections but the individual parts are drawn to scale, it can 
be compared with Pl. I of Comm. n°. 69. For those parts which 
correspond the same letters are retained, where an alteration has 
been made the letters are accented, while new parts are characte- 
rised by new letters. A detailed description is hence unnecessary, 
but it may be noted that the screw head a, is changed, that a 
closed nut screwed on at c,,, has been added by which the pressure 
can be suddenly released if necessary, and that a cock c,, has been 
introduced, to enable the level glass to be shut off if required. 

The compression tube <A’, is designed for use in the first place 
with piezometers of the kind described in § 2 but of larger dimen- 
sions. The use of this tube A’, is then the same as the original 
A, (comp. §§ 3 and 4) and it may be introduced directly in place of 
this into the system shown on Pl. I of Comm. n°. 69. 

In the second place this compression tube serves to hold glass 
tubes with a stem 6,—4#, (cf. Pl. IL fig. 2 Comm. n°. 69) onto which 
other apparatus can be screwed in place of the simple nut and 
capillary shown there. In Pl. I fig. 2 is shown a three way cock 
with two steel capillaries g,’ and g,’’ which is employed as follows. 

One of the capillaries g,’ is connected directly with the small 
measuring piezometer of the type of f fig. 2 Pl. IT Comm. N°. 69 
the other g,’’ with a volumenometer, so that when #,,, is shut and 
hes, and A, are open a known quantity of gas can be brought 
into the compression cylinder from the volumenometer. On the other 
hand when £,,, is open and #,,, shut this gas can be compressed 
into the piezometer where the temperature and pressure are measured 
as before. The large glass tube with stem and the piezometerreservoir, 
form in this way a piezometer of variable volume (constant quantity) 
and the difference with the former method consists in the measure- 
ment of the normal volume in a volumenometer instead of in the 
piezometer itself. The volume of the large glass tube in this 
method is not required to any high accuracy and the small w tube 
at the bottom may be omitted (g, Comm. n°. 50 PL I fig. 4 June ’99 
and 6, Comm. n°. 69 Pl. IJ March ’01). The accuracy is now 
really that obtainable with the volumenometer (cf. § 20) in so far 
as the determination of the normal volume is concerned. The spaces 
Koor Kisos Kiso Of the small three way steel cock must be also 
accurately calibrated. Care is taken also that the pins really shut 
properly into the sockets which makes the whole absolutely trust- 
worthy up to at 100 At. 

Although we wish to confine ourselves to the method of variable 
volume (constant mass) a second measurement with the volumeno- 


( 638 ) 


meter is required, in the same manner as would be necessary if we 
employed the method of constant volume. For, we have already 
mentioned in § 1 that this compression apparatus is suitable for this 
method. The measurement is made by shutting /,,, under known 
pressure and allowing the compressed gas to expand through the 
capillaries g,/’ and gy,’ into the volumenometer and reading as before. 
This second volumetric measurement, with its necessary corrections, 
gives the determination of the normal volume after the measurements 
at high pressure and compares with the second normal volume 
determination of the original method. 


§ 20. An accurate volumenometer. The volumenometer mentioned. 
above in § 19 was designed to give isothermal measurements of an 
accuracy of ———~ up to 60 Ats pressure. Hence the same accuracy 

: 10000 ks 
was desired as with the standard piezometers of Comm. n° 50 June ’99, 
while at the same time the determination of the deviations from 
Boyre’s law at ordinary pressures was kept in view. The most 
analogous apparatus is that employed by Lepuc; that of Wrrkowsk1, 
who has used a form more closely analogous with ours, does not 
appear to have been designed for high accuracy. 

The measuring vessel Zj, (Pl. Il fig. 1 and more in detail fig. 2) 
where the gas is shut off by mercury entering through /%,, consists 
principally of 5 bulbs /), such of 250 ce. and a smaller bulb #4, 
of 25 ce. capacity. These are separated by short really cylindrical 
portions Zi... Lj, on each of which there is a mark, near to 
which the mercury meniscus is brought for the measurements. 

At the lower end of the measuring vessel is a contrivance after 
the scheme of Comm. n°. 27, for catching any dust or stray gas which 
may perchance come from the rubber tube at C/, PI. II fig. 2. At the 
upper end the vessel terminates in a capillary tube /;,, which is - 
divided almost immediately into two ZZ, and Mt, One of them is 
terminated near the apparatus by a cock 7,. The other ends in a 
glass or steel capillary terminated also by a cock. On PI. IT fig. 2 
e. g. the volumenometer is connected to the mixing apparatus /” by a 
capillary tube soldered on to it after it has been mounted in Z, by 
the cock 7, At Ei, (Pl. Il fig. 1) e.g. 7, the-steel capillary 9,” 
proceeding from the three way cock mentioned in § 19 may be 
connected. The small bulb 7, is calibrated by mercury at the same 
time as the larger and serves to determine the small volumes above Zi, 

To keep the temperature of the gas constant and uniform the 
measuring vessel is firmly fixed to the bottom of the copper case Kas, 


rachid 


( 639 ) 


through which water at constant temperature flows from the thermo- 
stat described in Comm. n°. 70 III May ’01 (see Zo, on Pl. II. fig. 1). 
Uniformity of temperature is also assisted by the movement of the 
stirrer on to which the thermometer 7% is fixed. 

The ring /,, together with the bottom plate is soldered to the case 
Ks, and is large enough for the measuring vessel to be put through 
it. The closing plate /, is made fast to the measuring vessel and is 
so arranged, that it can easily be made watertight and that it can 
bear the weight of the whole mass of mercury when the tube is 
full without any danger to the glass as long at least as it is not 
displaced from its vertical position. The closing plate with flange and 
packing is pressed against the ring /,, at the bottom of dy by 
the screw s.,. The different parts will be seen by an inspection 
of Pi. II fig. 1. &., the ring and packing, made large enough to 
be brought over the measuring vessel, /, and “/,, round copper 
plates provided with a thread and cut out at /., and , enough 
to pass over the tube M,, so that they can be put on from the side 
and made fast together by the screws Z,; together they form the 
closing plate which is screwed into ,; Hy, and Ly, the halves from 
a round vuleanite plate which rest on the ring /,, with bottom Z, 
and support the enlargement Zi. Lp, and Zp, the two halves of a 
rubber plate which are united by rubber solution and pressed into 
the ring ZE, to make the whole watertight. 

When the closing plate has been made fast perpendicularly to 
the measuring glass and has been screwed against the lower rim of 
KE, the two parts of the conical top Z„ are brought together into 
place and the measuring glass centered and held fast by the cork Z2 
The whole waterbath is then brought into as vertical a position 
as possible. N 

There are windows in the case #, which enable the tube to be 
lighted and read. These are formed by thin pieces of plate glass held 
between stout brass frames Zj, and /,, one of which is soldered 
to the wall of £, . The screws Lj, enable the plate to be equally pressed 
against the rubber packing Zj, and the glass. It is quite necessary to 
have the case completely tight, which was here obtained, to prevent 
the felt in which MZ, is packed from becoming wet, and hence from 
an irregular loss of temperature. 

In spite of the verticality of the entire case the glasses require to 
be tested with a contact spirit level, in order that the necessary 
correction to the cathetometer reading may be made. 

To determine the volume of an enclosed quantity of gas the position 
of the meniscus is not read with reference to the marks on the glass 

43 


Proceedings Royal Acad. Amsterdam. Vol. V. 


( 640 ) 


tubes, but on finer lines etched on to small glass plates /,,—4#,,, 
provided with connections /,, and screws /,, to fix them to the 
cylindricals portions of the measuring vessel. By a proper arrange- 
ment of these the meniscus and the lines can be sharply seen over 
the whole length of the case. 

The measuring vessel is calibrated by temporarily blowing on, at 
the lower end, a small glass cock with a fine point (ef. Comm. N°. 70. 
IV. May ’OL). The mercury is introduced through this in the care- 
fully exhausted apparatus and the menisci are then read in the 
manner described above for the measurements and with the same 
precautions as to lighting and temperature. The mercury drawn off 
at the cock is weighed. As before the readings are made on the glass 
plates but in order that the calibration shall not be lost if these have 
to be removed, they are also compared with the lines on the eylin- 
drical tubes. This would be necessary if the tube had to be removed 
cleaned and dried after the method of Comm. N°. 27, but usually 
it is sufficient to suck up the various liquids and to dry by repeated 
evacuation admission of dry air through 7, and 7, of Pl, II fig. 2. 

The measuring vessel can be completely shut off from the mer- 
cury reservoir, see Pl. II fig. 2 or the manometer by the clamp C7,. 
All these connections are carefully cleaned good thickwalled black 
rubber tubes, which are strengthened by wrapping them spirally in 
strong tape. The mercury meniscus (ef Comm. N°. 67 Dee. ’00 for 
what is here implied) remains quite clean after a series of measure- 
ments, if only dry gas is admitted to the volumenometer (this is 
only true when the gas has no action on the fat of the cocks and 
joints). The small changes in the position of the meniscus to bring 
it to the required position are made by manipulating the clamp C/, 
and the resevoir. During the measurements this clamp is always closed. 

The pressure of the gas in the volumenometer is given by the 
height of the mereury in the manometer tube when C7, is quite 
open. This is itself connected to a barometer and-a resevoir at con- 
stant temperature by airtight connections in the manner of Comm. 
N°. 60 June 00 and the same precautions are taken to ensure 
accuracy in the temperature determinations of these two mercury 
columns. The volumenometer meniscus and etched lines, manometer, 
barometer and standardseale (ef Comm. N°. 60) are so placed that 
they can be read without altering the telescopes of the cathetometer. 

The menisci of the barometer and manometer are read as described 
before, that of the volumenometer by the help of a brass plate with 
a 2 mm. slit in it, which is brought with a glow lamp to the same 
level as a meniscus and gives good definition. 


heid 


( 641 ) 


In order that the required accuracy may be obtained it is neces- 
sary that the pressure shall not fall below 0,5 Atm. 

To determine the theoretical normal volume measurements are 
made at two or if possible at three positions with the same quan- 
tity of gas. Whenever the third virial coefficient C (ef Comm. N°. 71 
June *O1 and N°. 74)*) does not come into account at the pressures 
considered and to the accuracy required, the same value of the coef- 
ficient B must be found by a combination of any two of the three 
measurements. This gives directly the deviations from the law of 
Borre and hence the theoretical normal volume. 


§ 21. The mixing apparatus. On Pl. IL fig. 2 the volumenometer 
described in § 20 is shown connected with other apparatus for the 
preparation of accurate mixtures of gases and for the investigation of 
their compressibility. 

The drawings do not require much explanation. The mixing vessel 
F and the reservoir G have about 2 liters capacity. G is provided 
with a three way cock and is particularly useful when a number of 
mixtures are required with a small proportion of one component 
which can be contained therein. 

The connecting tubes between 7,, 7,, 7, and from / to 7, are nar- 
row so that the uncertainty of their temperature may have no influence 
on the accuracy of the measurements, the other tubes are large enough 
to allow free connection between the various parts and the pump 
and to help rapid exhaustion. 

When a mixture of given composition is required, and the mercury 
stands above the closed clamps C/,, C/,, Cl, Cl, the whole apparatus 
is pumped out through 7, and is filled through 7,, while 7, is shut, 
from say the gas apparatus connected to 7,, after being washed out 
with this gas. 

Then 7, is shut and 7, so turned that the gas is shut up in G 
while / is brought into connection with the pump through 7,. The 
cocks 7,, 7, and 7, are then opened and /# and # and the connec- 
tions pumped out again. By raising Ar and opening C/, widely and 
Cl, (to prevent air entering from J/) only partially the mercury 
is caused to enter / and to fill first Z,, without enclosing any 
gas, then /, up to the required position, when C7, is shut. The 
space between 7,, 7,, r, is repeatedly washed out by a small 
quantity of gas from G through the cock 7,, from here also gas is 


? 
ie) 


1) Livre jubilaire dédié à J. Bosscua; Archives Néerlandaises, Ser. Il. T. VI. 
p. 874—888. 1901. 


( 642 ) 


brought into EZ and the whole pumped to a good vacuum. The 
required quantity of gas can then be brought into # through 7, and 
y,. The volume temperature and pressure of the gas in /, shut off 
by r, and 7, are then accurately measured and when 7, is opened 
nearly the whole of this can be brought over into /. The remaining 
portion in Zj, and /,, is then measured by expanding to /,, or 
E,,, and Cl, is again closed so that # can be again evacuated. The 
second gas is then brought directly into the volumenometer from 
r, and the volume measured in the same manner. 

When this is finished 7, is again opened and the second compo- 
nent in # mixed with the first in / where it stands for some 
time. The admixture of the total quantity is completed by 
drawing the combined gases several times backwards and forwards 


between the two vessels. The mixture is then preserved in /’and as 


much as may be necessary is driven into /, or through 7, into 
other apparatus for measurements on the compressibility. 


(April 24, 1903). 


H, KAMERLINGH ONNES and H. H. F. HYNDMAN, „Isotherms of diatomic gases and 
their binary mixtures. V. An accurate volumenometer and mixing apparatus ” 
PLATE [. 


| » &h 
| %5 N 
\ 
OU N_N 
am | dy pr A 
Ae 1 IRIS 
fens a N 8 
RG 2 
te 9 \ N 
| NN 
an! N N 
: SN 
cy N \ 
Om mom neem | \ 
| Ge N 
a 320 = N N 
C35 \ 
th \ > 
cp a \ TD 
ee, NN 
N 
\ 8 
| 
oe ©) 
mN Ne 
3 ST, \ 
Si) 
N = 
Ne GN 
ib NN 
=f 
: | 2 NISNS Ig À 
D= N X EA MS QVnpRmn AA-_@{ AZ 
Ne, je N N 1 ODD NSS SS N SS Di ? \ 
H N N © aye 5 5 a Ko 3 Py 5 190 
ch N NRE ea 
HX Om) N = 
a eN Fig. 2 
H G N i) 
| VaR’ 
: MIA 
Ce C AV 
NH 3 1 
5 1 
Fig. fe 


Proceedings Royal Acad. Amsterdam. Vol. V. 


- Í MANE, 
' METTEN ATR ETM A 
_ | VU PUTA 


Uk. 


7 So oon hen 


H. KAMERLINGH ONNES 


Proceedings Royal Acad. Ax 


leter and mixing apparatus.” Praca IE 


a) «0 Jo 6 
eel i L 1 | | | 
bic J 2 5 


H KAMERLINGH ONNES and H. H. F. HYNDMAN, „Isotherms of diatomic gases and their binary mixtures, V, An accurate volumenometer and mixing apparatus.” Puate II, 


ede) 


sc 


Proceedings Royal Acad, Amsterdam. Vol V. 


PVA ag ee ee ON 


SNe ee Pee 


KONINKLIJKE AKADEMIE VAN WETENSCHAPPEN 
TE AMSTERDAM, 


PROCEEDINGS OF THE MEETING 
of Friday April 24, 1903. 


EE 


(Translated from: Verslag van de gewone vergadering der Wis- en Natuurkundige 
Afdeeling van Vrijdag 24 April 1903, DL. XI). 


CONTENTS. 


C, A. Losry pr Bruyn and C. L. Juncius: “Dissociation in and crystallisation from a solid 
solution”, p. 643, 

E. H. Biicunur: “The transformation of diphenyliodonium iodide and chloride and its velocity”. 
(Communicated by Prof. C. A. Lopry pr Bruyn), p. 646. 

J. J. Branksma: “Nitration of symmetrical dinitroanisol”. (Communicated by Prof. C. A, 
Logsry pe Bruyn), p, 650. 

J. H. Bonnema: “Two new mid-cambrian erratic-blocks from the Dutch diluvium”. (Com- 
municated by Prof. J. W. Morr), p. 652. 

J. C. Krurver: “An analytical expression for the greatest common divisor of two integers”, 
p. 658. 

W. H. Juris: “On maxima and minima of intensity sometimes observed within the shading 
of strongly widened spectral lines”, p. 662. 

H. A. Lorentz: “On the emission and absorption by metals of rays of heat of great wave- 
lengths”. p. 666. 

G. VAN Iverson Jr.: “The decomposition of cellulose by aérobic micro-organisms”. (Com- 
munieated by Prof. M. W. BEIJERINCK), p. 685, (with one plate). 


The following papers were read: 


Chemistry. — “Dissociation in and crystallisation from a solid 
solution”. By Prof. C. A. Lory pr Bruyn and Mr. C. L. Junatus. 


(Communicated in the meeting of March 28, 1903). 


It is no longer necessary to be reminded of the analogy between 
liquid and solid solutions but it is still a matter of importance to 
trace and investigate new instances of the similarity of the two 
solutions. For this reason attention may be called to the following 
phenomena and observations. 

The new phenomena relate to the interesting intramolecular rear- 
rangement discovered by CrAmiciAN and Sinper') in which solid or 

1) Ber. 34. 2040 (1901). 

44 


Proceedings Royal Acad. Amsterdam. Vol. V, 


( 644. ) 


dissolved o-nitrobenzaldehyde is converted, under the influence of the 
blue rays of sunlight *) into o-nitrosobenzoie acid: 

ÁNNO, HOK RO 

EN re 

23 Sn 
and where consequently an oxygen atom of the nitrogroup migrates 
to the neighbouring aldehyde group and oxidises the same to carboxyl. 
CramiciAN and Singer have investigated this reaction more closely, 
principally with solutions in different liquids; as regards the trans- 
formation taking place in the solid condition, in which we happen 
to be particularly interested, they merely say: „dass die Krystalle 
nach und nach ihre lichtgelbe Farbe verlieren, undurchsichtig, griin- 
lich und sehliesslieh weiss werden”. 

The said changes in colour, the occurrence of the green coloration 
and the subsequent turning white render the phenomenon precisely signi- 
ficant for the knowledge of the properties of solid solutions. This 
will become evident when we think of the general and very interesting 
property of the organic nitrosoderivatives to suffer polymerisation and 
become colourless when in a solid condition; in solution, however, 
they are wnimolecular and coloured (generally blue or green). This 
behaviour is quite Comparable to that of nitric peroxide. Ina certain 
ntumber of cases the depolymerisation has been traced by cryoscopic 
means, as it often takes place very slowly: the lowering of the 
freezing point then gradually becomes greater while the colour becomes 
more and more intense. In this way it has been ascertained that in 
the colourless solid nitroso-compound two molecules have become 
united showing that an intense colour must beattributed to the single 
molecules. The same happens with NO, (the nitroso-compound of 
oxygen) which has an intense colour, whilst its polymerisation product 
N,O, is colourless. 

After these remarks it is not difficult to see in what manner the 
transformation of solid o-nitrobenzaldehyde into solid o-nitrosobenzoic 
acid must be conceived. The displacement commences as soon as 
the crystal is exposed to sunlight; after about 15 minutes a faint 
green tinge is perceptible which gradually deepens ; the nitrosobenzoic 
acid, which is formed from and in the solvent, first remains in solid 
solution and, to judge from the green colour, in the unimolecular 
condition, On continuing the exposure to sunlight the colour becomes 
more intense, until finally the saturation point is reached; the outer 


') We have ascertained that an elevation of temperature does not cause the 
displacement. 


( 645 ) 


layers of the erystal then become dull and a lighter green, the 
nitrosobenzoic acid, which erystallises out, is now however white 
and consequently bimoleculair'); finally the surface of the crystal 
becomes quite white and opaque. The process then apparently comes 
fo a standstill because the sunlight cannot any longer penetrate the 
interior of the crystal or only in an insufficient degree. In this case 
the interior of a sufficiently big crystal still contains a green trans- 
parent nucleus. 

The titration of five different specimens has given the following 
result: 


After 2'/, day about 3 °/, of nitrosobenzoie acid. 


I 6 /. I I > fl I 
I 10 ft I 1 1 I I 
I 15 I fl 15 I I 
" 34 I fl 24 I I 


The surfaces of the last erystals had turned quite white. 

Conclusions as to the velocity of transformation cannot of course 
be drawn from these figures, as on the one hand the source of light 
varied too much in intensity, whilst on the other hand the crystals 
were of a different thickness. 

It was considered of importance to try and determine the maximum 
solubility of o-nitrosobenzoie acid in o-nitrobenzaldehyde. From the 
surface of those green crystals, which commenced to deposit the 
white acid, the latter was therefore as far as possible removed by 
mechanical means. By titration 2.6°/, of nitrosobenzoic acid was 
then found; if now we may assume that the concentration of the 
acid inside the crystal is not smaller than that at the surface the 
saturated solid solution contains about 2.6 mols. of acid per 100 mols. 

Another conclusion may still be drawn from the above, namely 
that o-nitrosobenzaldehyde is capable of forming mixed crystals with 
2.6 mols. of o-nitrosobenzoic acid; whether these two substances 
are isomorphous is not known as the system of crystallisation of 
nitrosobenzoic acid has not been determined. Very probably they 
are not isomorphous as otherwise the power to form mixed crystals 
would occur over a larger interval or even for all proportions. 


1) It has not been possible to ascertain, by the ordinary means at disposal, not 
even by the highest possible enlargement, that the o-nitrosobenzoic acid formed 
is crystalline. This cannot be a matter of surprise if we consider that the separa- 
tion of the acid proceeds very rapidly and that the diffusion in solid solution is 
particularly slow. Still we may speak here of crystallisation as the separated 
substance, in contrast to amorphous compounds, exhibits definite physical constants 
(fixed melting point, solubility etc.). 


44* 


( 646 ) 


By determining the meltingpoint line of the system of the two 
substances (the aldehyde melts at 45°, the acid is decomposed at 
about 200°) the point up to which they are still capable of forming 
mixed crystals may perhaps be determined more accurately. It is 
not improbable that in the intramolecular rearrangements of other 
solid substances solid solutions may also be formed; if possible this 
will be further investigated. 


Chemistry. — “The transformation of diphenyliodonium todide and 
chloride and its velocity’. By Mr. E. H. Bécuner. (Communicated 
by Prof. C. A. LoBrr DE BRUYN). 


(Communicated in the meeting of March 28 1903). 


It is about 10 years ago that Vicror Meyer and HARTMANN !) 
announced the important discovery of a new class of iodine deriva- 
tives, the iodonium bases, substances with a trivalent iodine atom, 
having about the same basic power as the ordinary alkalis and capable 
of forming salts. The simplest representative of this interesting 
class of substances is diphenyliodonium-hydroxide: (C,H,), JOH; 
the salts, such as the chloride or the nitrate, when dissolved in water, 
appeared to possess a conductive power corresponding with that of 
the alkali salts ®). 

The behaviour of the halogen salts of the base, when heated, is 
peculiar; Victor Meyer and HARTMANN noticed that on fusing these 
salts at 175° a decomposition sets in, which spontaneously leads to 
a complete conversion into halogen-benzene (C,H,), = J—J = 2C,H,J 
with strong evolution of heat. 

This transformation now deserved a closer study. It may be con- 


sidered as a depolymerisation but is distinguished however from 
many other similar reactions, not only by the great difference in 
character between the decomposing substance and the products of 
decomposition but also by the fact that the transformation is not 
reversible. At all events, up to the present no process is known 
which leads straight from iodobenzene to diphenylodoniumiodide. 
In this latter respeet the above mentioned reaction is distinguished 
from the transformation with which it has been compared namely 
that which tetramethylammonium iodide suffers on heating; the latter 
substance is readily prepared from its products of decomposition at 
the ordinary temperature. 


1) Ber. 27. 502, 1594. (1894). 
2) Suruvan Z. ph. Ch. 28, 523. The salts are, therefore, not dissociated hydrolytically. 


( 647 ) 


It was to be expected that the decomposition of the diphenyliodonium- 
salt would take place at temperatures considerably below the melting- 
point, and this is actually the case. 


1. Beforehand, however, it was deemed desirable to study the 
behaviour of the iodide towards light as in the study of the velocity 
of transformation account had to be taken of a possibly existing 
sensitiveness to light *). 

I have found that in the case of the iodide the transformation 
is caused by exposure to light *); whilst it remains quite intact when 
kept in the dark for 2'/, months. It was to be expected that the 
source of the light would affect the transformation. The following 
results were obtained : 


Electric Are-Light: after 1 hour titre: 26.6°/, J, converted about 14.5°/, 


" 7] mentele yn 249 , I ded AO 
Sunlight: ná I" y 30.0 4 it IJ 3.5 # 
" „ 30 " fe EIO i, " pe GON 
Auer Light: „170 " oe iar i li IJ FF 6.4 » 
Diffuse Daylight: a. „ 10 weeks: 24.7 ‘y " i ee 
7 b. / 203 / 1" pes Ln 


The decomposition of the iodide is therefore most rapidly effected 
by the arc-light. 


2. If now the solid iodide was exposed to temperatures consider- 
ably below its meltingpoint a more or less slow conversion seemed 
to take place. Whereas 1°/, at most was decomposed at 90° after 
3 hours, about 36°/, had disappeared at 100° after 13 hours, whilst 
after heating at 123° for 31/, hours only 5°/, was left undecomposed. 
This shows that the decomposition of the solid substance already 
takes place even at temperatures considerably below the meltingpoint. 
This also applies to the solid chloride which however is more 
stable than the iodide. 

Several series of experiments were now made with the solid iodide 

1) The quantitative estimation of iodonium haloid and halogen-benzene in the 
presence of each other is simply done by titration with AgNO;; the first when 
introduced into water yields one of the halogen atoms as ion whilst iodo- or 
chlorobenzene does not react with AgNO,. 

For diphenyliodonium-iodide was found: according to Garws 62.1 and 62.19/, J, 
calculated 62.2°/4; by titration 31.0 and 31.1%, J. The chloride gave on titration 
11.158 9 Cl, calculated 11.20/,. 

*) V. Meyer states that it turns yellow on exposure to light. 


( 648 ) 


at temperatures of L05—110°; the results obtained will be commu- 
nicated on a future occasion. 


3. It was obvious that I should try to make a closer study of 
the velocity of transformation of the iodide in solution. Its great 
insolubility, however, rendered the operation impossible; of the many 
solvents which were tried, pyridine proved to be the best; the 
solubility of the iodide was however still too small, namely only 
about ee 

The more soluble diphenyliodonium-chloride was better suited for 
the purpose; the solubility in water, although not large, proved sufti- 
cient at the temperature at which the operation took place (98—99°). 

The results obtained in fifteen velocity determinations were at 


first very unsatisfactory and pointed to the existence of many inter- 
fering influences. The coefficients obtained on applying the formulae 
for unimolecular and bimolecular reactions were anything but constant 
and often pointed to a very irregular course. In one experiment 
coefficients were obtained which were many times greater than those 
got in another apparently quite analogous case. Sometimes the coeffi- 
cients diminished equally, sometimes the reaction after proceeding 
for a while, suddenly ceased. After many similar negative results it 
at last appeared that the conversion of diphenyliodoninm-chloride into 
chloro- and iodobenzene is influenced to an extraordinary degree by 
the presence of very small quantities of impurities. Very small 
quantities of acid retard the reaction to a remarkable extent or bring 
it to a standstill: the presence of traces of iodine causes a regular 
full in the reaction coefficient; a litthe of the free base (diphenyl- 
iodonium-hydroxide) accelerates, on the other hand, the decomposi- 
tion in a strong degree. The halogenbenzenes formed during the 
reaction appeared hoivever to be inert. 

On now using a very pure preparation free from acidity and of 
a pure white colour and applying the formula for reactions of the 
second order, coefficients were obtained which could be considered 
as constants. (see table p. 649). 

On adding 6 ce. of ™/,, HCl, the coefficient (which, moreover, was 
not constant) fell to about half the value obtained in experiment I 
while the presence of 8 ec. of "/,, (C,H,), JOH increased the coefficient 
about + or 5 times’). 


1) The following experiment also may show how sensitive the transformation is 
to very trifling quantities of foreign substances. To a solution of the chloride 
(Co = Yo9.2, T— 99.0), which after 3!/, hours had fallen from 30.67 AgNO, to 
23.71, was added 39.3 milligr. of a well crystallised chloride which was coloured 


Say ri 99° Cat... B 


2.909 gr. in 250 em*. 


oe ccm. AgNO, | Ky | Ky 
Kaa 
RENS 
18 | 42.95 | 0.0152 | 1.32 
20 1.87 | TEN 1.97 
99 aa | 443 | 4.31 
24 10.87 135 | 1.96 
25) 10.50 136 | 190 
98 Q 94 | 130 1.97 
30) 9.42 | 4199} 4.30 


TW. T=99.0 ¢,=%., 
trace of iodine added. 
t Keno, |K, 
0 715 
11/, h 25 1.43 
31, 23.00 1.33 
Blf. 29.00 1.40 
111), 18.37 1.00 
gg, |. 45.77 0 88 
If, by 


0 37.17 
1!/5 33.82 0.0973 1.11 
All, 27.85 295 | 4.32 
9 DT 236 1.49 
7 22.95 299 1.16 
| 
nen 
ive PA 6,16. ar 


loo; ; 
25 om}, n/a, HCl added to 150 em*, 
Cone. of the HCI therefore '/,., n. 


t AgN( ), 
1) PAT MANO, 
2 hi. 2150 
4 en 

22 | 26.61 


neutral. with NaOll 


26 | 21.32 
28 17.87 
eneen 


means of the van ’r Horr formula’), we ecalculate the 


order of the reaction from the communicated experiments and also from 


a few which are not yet communicated, we find n= 2.1,1.9 and 2.1. 


From this, and also from the fact that in experiment I the K,’s are 


constants, it follows that the transformation 


somewhat yellow, but gave on analysis the theoretical number for chlorine. By 
this addition the titre naturally increased and came to 26.10; 21/, hours later the 
solution did not appear to have changed (found 26.08). The somewhat coloured 


chloride was found to have a faint acid reaction and to give blue colour with 


starch solution a‘ter some time. 


i) K, is calculated according to the formula for reactions of the first, Ky according 


to that for reactions of the second order. 


2) Vorlesungen, I. 193. 


— 


( 650 ) 


(Cs He abel Cech GH 
is a bimolecular one. 

Since the chloride is comparable with a salt such as KCl, it may 
be concluded that the transformation does not oceur in the non- 
dissociated molecules but between the ions. This idea would agree 
with that propounded by Waker and Hamry *) for the transformation 
of ammonium isocyanate in aqueous or alcoholic solution into urea, 
a reaction which also appeared to be a bimolecular one. WALKER 
and Hamry were enabled to support their view by showing that 
either ammonium- or isoeyanie acid ions cause a retarding intluence 
on the reaction investigated by them as both diminish the dissociation 
of ammonium isocyanate. In our case a similar behaviour of chlorine 
and iodonium atoms does not present itself. Hydrochloric acid has 
certainly a retarding influence but this is too large to be explained 
by a diminution of the ionisation. Then again, iodonitum hydroxide 
has a strong accelerating power. We must, therefore, think here of 
a special catalyzing influence of hydrogen- and hydroxyl ions: 
apparently the first acts here as a retarding catalyzer, an influence 
of which up to the present but few instances are known. Then, if 
the acid is neutralised (compare expmt. IV), the transformation proceeds 
in a regular manner whilst the chlorine ion is still present in about 
the same concentration. 

The most probable view of the mechanism of the transformation 
of the iodonium haloids is therefore that the reaction takes place 
between two molecules. 

A trace of iodine retards the transformation in an increasing degree. 

This investigation will be continued later on. 


Organic. chem. Laboratory, University of Amsterdam. 


Chemistry. — “Nitration of symmetrical diutroanisol.”” By Dr. J. J. 
BLANKSMA. (Communicated by Prof. C. A. Losry pr BRUYN). 


(Communicated in the meeting of March 28, 1903). 


In a previous communication?) it has been stated that pentanitro- 
phenol is readily formed by the action of nitric acid on symmetrical 
dinitrophenol whilst symmetrical dinitroanisol is attacked with difficulty 
by nitric acid. It seemed, however, not impossible that symmetrical 
dinitroanisol might still be further nitrated and this indeed appeared 
1) J. Ch. Soe. 67. 746 (1895). 

2) Proc. Royal Acad. 25 Jan. 1902. 


( Got } 


to be the case. If symmetrical dinitroanisol is treated for two hours 
on the waterbath with a mixture of HNO, (density 1.44) and sulphuric 
acid, trinitroanisol is formed m. p. 104°. The nitrogroup introduced 
into this substance is mobile and easily replaced by OH, OCH,, NH, 
NHCH, ete. If the NO, group is replaced by OH dinitroguaiacol is 
formed m.p. 121°. By treatment with alcoholic methylamine, methyl- 
amido-dinitroanisol is formed m.p. 168°, which is converted by nitric 
acid of 1.52 sp. gr. into oxymethyl-dinitrophenyl-methylnitramine m.p. 
118° already obtained by Grimavx and Lerùbvre®) by nitration of 
dimethyl-orthoanisidine. This goes to prove that the nitrogroup in 
regard to the OCH,-group has been introduced into the ortho place 
and that, therefore, the constitution of trinitroanisol is represented by 
ott. OOH: (NO eb Bb a. 

If trimitroanisol is treated with a solution of Na OCH, in methyl 
alcohol the NO, group 2 is replaced by OCH, and the dimethylether 
of dinitropyrocatechine is formed, m.p. 101°. Treatment with alcoholic 
ammonia yields dinitroanisidine C, H, (OCH,) NH, (NO,), 1. 2. 3. 5, 
m.p. 174; with aniline and aethylamine are formed compounds 
melting respectively at 155° and 123°. 

If trinitroanisol is nitrated with a mixture of nitric acid of 1,52 
sp. gr. and sulphuric acid a tetranitroanisol is formed m.p. 154°. On 
treatment with 2 mols. of Na OCH,, this substance is converted into 
erystals which melt at 165° and assume a purple-brown color when 
exposed to light. 

Analysis shows that two NO, groups are replaced by OCH,. Lorine 
JACKSON *) by treating symmetrical tribromodinitrobenzene with 3 mols. 
of NaOCH, has prepared a compound with the same properties as 
the above mentioned; he however considered that he had obtained 
the dimethylether of dinitroresorcinol. The latter substance melts 
however, according to Fruryss®) and Merpora *) at 154°, whilst Merrum 
Trrwoer*) and L have found 157°. It is therefore very probable 
that Loring Jackson has been dealing with the trimethylether of 
dinitrophloroglucinol as, on treating symmetrical tribromodinitrobenzene 
with Na OC,H,, all three Br-atoms may be replaced by OC,H, ®. 

That the compound obtained from tetranitroanisol and NaOCH, is 
really identical with that from symmetrical tribromodinitrobenzene 


1) Compt. Rend. 112. 727. 

2) Amer. Chem. Journ. 18. 180. 
3) Centr. Blatt. 1901. I. 739. 

4) Proc. Chem. Soc. 17. 131. 

5) Rec. 21. 288. 

6) Amer. Chem. Journ. 21. 512, 


( 652 ) 


was shown bv taking the meltingpoint of a mixture of the two 
substances; no lowering of the meltingpoint was noticed. It is 
therefore proved that from tetranitroanisol and NaOCH, the trimethyl- 
ether of dinitrophloroglucinol is obtained and consequently the con- 
stitution of the tetranitroanisol is: 


C,H OCH, (NO,), 4. 2. 3. 


OCH, OCH; 


NO 6 NE NO,/ \NOz 
| 
NO. me JSO, SN / OCH, 


If symmetrical tribromodinitrobenzene is treated in aleoholie solution 
with six mols. of methylamine, the three bromine atoms are readily 
replaced by NHCH, and we obtain fine orange-red needles m.p. 220° 
(with decomposition. When this symmetrical C,H(NO,), (NHCH,), 
is dissolved in nitric acid of 1.52 sp. gr. and then ited with water 
a fine white crystalline powder is obtained which, when dissolved in 
elacial acetic acid, deposits small beautiful white needles, which explode 
between 200° and 203°, sometimes causing aflame. From the analysis 
it appears that this is the symmetrical trinitropheny ltrimethy Hrinitramine. 


NO, 
NICH, NCH, 
Ne No, \NO, 
= NO, NO, 
cas /smten CHa ANN 
2 
x NO. 
Geology. — “ Two New Mid-Cambrian Erratic- Blocks from the 


Dutch Diluvium?. By J. H. Boxxema at Leeuwarden. (Com- 
municated by Prof. J. W. Morr). 


I. When I had been appointed assistant at the Geologieal-Mineralogie 
Institute at Groningen, L was charged with the task of determining 
the fossils that are found in the collection of Groningen sedimentary 
erratic-blocks. If we succeed in this with a fossil, we can as a rule 
more or less accurately, for the erratie-block in which it occurs, fix 
the age of the layer of which it formerly formed part; at the same 
time it may be found out whether suchlike stone is still known as 
firm roek, — and whether the same kinds of erratic-bloeks have 
been met with in any other places. 

With many pieces I suceeeded, but with a not inconsiderable 
number I failed, owing to various causes. To the latter division 
belonged i.a. two small pieces of lime-stone, the largest dimensions 


( 653 


of which are about 4 centimetres. They originally made part of one 
erratic-block, which was found when the ramparts near one of the 
former Groningen gates (Boteringepoort) were dug off. One of the 
pieces still shows a part of the original surface possessing distinct 
elacierscratches. 

From the pieces preserved it may be concluded that this erratic- 
block consisted of green-grey, rather compact, marly lime-stone, in 
which with a magnifying glass many little grey grains and here and 
there little dark-green lustrous Glauconite-grains may be distinguished. 
I observed one single Pyrite-erystal. At the surface it had, to a depth 
of about 1 centimetre, become more or less yellow, under the influence 
of corrosion. 

The part preserved also shows that through this erratie-block van 
a layer that was rich in Trilobites-remains. For the greater part the 
transverse sections of them are visible. In one piece, however, some 
remains are partly or entirely exposed to view. A mid-shell is the 
most important of them. 

This mid-shell, across which run various flaws, and which conse- 
quently is not likely to have entirely retained its original shape, is 
lengthwise rather strongly vaulted and has a length of 12 millimetres, 
its breadth amounting to about 14 millimetres. It is almost every- 
where the same, the lines that connect the beginning and the termi- 
nation of the facial suture, running almost parallel to the longitudinal 
axis. The front-edge is regularly curved. The occipital-furrow is 
shallow, especially on the glabella. The length of the rather broad 
glabella is about */, of that of the mid-shell. It is tongue-shaped and 
bounded by shallow dorsal furrows. The latter first ran nearly parallel 
to each other and then turn to the centre, where they meet. Lateral 
furrows are not to be distinguished on the glabella. That part of the 
mid-shell which lies in front of the glabella, slants down rather 
quickly. The parts on either side slant down more slowly. 

As to the sculpture, along the front-edge of the mid-shell, parallel 
to it, run fine stripes. The shell moreover shows all over, very near 
each other, fine pricked points. The colour of the shell is partly black, 
partly yellow-grey (eream-coloured). 

In spite of repeated efforts I had never before succeeded in dis- 
covering what species of Trilobites this mid-shell came from. This 
summer, however, | was more fortunate. On my journey to Oeland 
it chanced that near the hospital at Borgholm a pit was being dug 
and that, while doing this, people had penetrated as far as the layer 
with Paradoxides Oelandicus Sjögren. The stone that had been produced 
from the pit, was still present. It consisted of greenish marl-slate, 


( 654 ) 


which had entirely fallen asunder, and of rather large lime-coneretions. 
This clashes with LiNNArsson’s ') opinion, that at Borgholm this layer 
should consist of marl-slate only, which opinion was afterward made 
use of by Rommer *) and Reme.¥ *). 

In the said lime-concretions I found, besides some remains of 
Paradoxides Oelandicus Sjogren and a couple of nearly complete spe- 
cimens of Ellipsocephalus Polytomus Lixnarsson, countless mid-shells 
of the latter species of Trilobites. 

Here was confirmed the opinion of Linnarsson *) that the absence 
of stripes on the front-edge of the mid-shells, and that of the pricked 
points, on the scale of the Ellipsocephalus-species occurring at 
Borgholm, by which this species was said especially to differ from 
the Stora Fré-species, must be attributed to the circumstance that 
his Borgholm material came from marl-slate, and that of Stora Fré 
from lime-stone. The stripes and the pricked points are remarkably 
distinct in the mid-shells I gathered from the lime-concretions at 
Borgholm. Consequently there is no reason any more for not ranging 
the Ellipsoeephalus-remains of Stora Frö under the head: Ellipsoce- 
phalus Polytomus LaxNarssoN, the difference in size only not sufficing 
to maintain the contrary. 

One of the lime-concretions contained a layer that was peculiarly 
rich in mid-shells of Ellipsocephalus Polytomus. While breaking this 
concretion to pieces, I was immediately reminded of my Groningen 
erratic-block; and now that I have compared the latter with the 
pieces I brought from Borgholm, I know that they are exactly alike. 
In both the stone is the same, except that the Groningen piece has 
a yellow tint, which must be attributed to the influence of corrosion. 
The mid-shells of Ellipsocephalus Polytomus, occurring in both, also 
resemble each other, in colour as well as in their numerous flaws. 

Consequently it may with perfect certainty be declared that the 
erratie-block mentioned above has the same age as the layer with 
Paradoxides Oelandicus Sjögren (the oldest of the Mid-Cambrian), and 
that a corresponding kind of stone is still found at Borgholm in 
Oeland. It is probably also met with at Stora Frö in the same 
island. I cannot say so for certain, however, as I did not go there 
and so do not possess any limestone from that place, which might 


be used for comparison. 


1) Linnarsson. Om |aunan i lagren med Paradoxides Oelandicus. Geol, Férenin- 
gens 1 Stockholm Förhandlingar. Bd. 3. pag. 354. 
2) Roemer. Lethaea erratica. pag. 37. 
5) Remeceé. Zeitschr. d. deutsch. geol. Gesellschaft. Bd. 33. 1881, pag. 183, 701, 


4) Linnarsson. Loc. cit. pag. 364. 


This is the first time that mention is made of such an erratic- 
block from the Dutch diluvium. Many of the kind, with remains 
of Ellipsocephalus Polytomus or of other fossils, occurring in Oeland 
in the layer with Paradoxides Oelandicus, have already been found 
in the German diluvium. The first of them was mentioned by Damgs’) 
and comes from Rixdorf near Berlin. A few years after, RemEns *) 
deseribed two such erratic-blocks from the neighbourhood of Ebers- 
walde. Later on, Rormer*) made mention of two erratic-bloeks of 
the same age. One of them comes from Rostock and bears much 
resemblance, according to the description, to the Groningen piece. 
This cannot with so much certainty be said of the second block, 
which was found at Bromberg and does not seem to be greenish. 
In Sleswick-Holstein, too, corresponding erratic-blocks seem to have 
been found, as Srornrmu *) writes about „grünliehe Kalkgeschiebe der 
Oelandicus-Zone”. 

This erratic-bloek also confirms my supposition formerly ®) men- 
tioned, that in the Hondsrug occur more sedimentary erratic-blocks 
with a West-Baltic character, than was formerly generally supposed. 


If. For some time already I have had in my collection several 
pieces of an erratic-block consisting of limestone that has been tinted 
dark-grey, even almost black, by bitumen. It was found in the loam- 
pit near Hemelum. Its calcium-carbonate having for the greater part 
crystallized, this limestone approaches antraconite. Some nests of little 
pyrite-erystals and a small phosphorite-nodule are found in the stone. 

For a long time the only fossil that was exposed to sight was 
(with the exception of a few unimportant remains, probably of a 
Paradoxides) what I supposed to be the internal cast of the inside of 
a piece of Trilobite-shell. Its largest dimension amounts to 9 milli- 
metres. This internal cast is almost oval, and strongly vaulted. The 
top-part finishes in a bow. On the convex side of this bow it is 
steeper than on the concave one. In front, on the least steep part, 
is a frame in relief, soon turning round the most elevated point and 
then continuing on the steepest part, where it becomes tinier and 
tinier. Towards either side springs from this frame a net-work of 

1) Dames, Zeitschr. d. deutsch. geol. Gesellschaft. Bd. 31. 1879. pag. 795. 

2) Remeré, Zeitschr. d. deutsch. geol. Gesellschaft. Bd. 33, 1881. pag. 181, 700. 

3) Roemer, Lethaea erratica, pag. 26. 

4) Srottey, Die Cambrischen und Silurischen Geschiebe Schleswig-Holsteins und 
der benachbarten Gebiete, 1895. Bd. I, Heft 1, pag. 40. 

5) Bonnema. “Cambrian ervatic-blocs at Hemerum in the South-west of Frisia.” 
These Proc. 1902, p. 142. 


( 656 ) 


suchlike ones. This net-work is very distinet on the less steep part, 
not so distinct on the other, where it is scarcely to be seen with a 
magnifying glass. Moreover there are on this internal cast round 
elevations. 

It being quite impossible for me to find what species of Trilobites 
this off-print came from, the exact age of this erratic-block could not 
be fixed. The nature of the stone made it likely to be Cambrian, 
and that, too, Mid-Cambrian, because of the suppositional Paradoxides- 
remains. 

When, however, a few weeks ago, my friend dr. GRÖNWALL from 
Copenhagen, the author of “Bornholms Paradoxideslag og deres Fauna’ 
(Danmarks geologiske Undersögelse Il Raekke No. 13.) took a view 
of my collection of erratic-blocks, he recognized in the said off-print 
that of a right cheek of Conocoryphe Exsulans Linrs.') Herewith 
the age of this erratic-bloek was already exactly determined, for the 
occurrence of these Trilobites-remains is characteristic of the lower 
part of the layers with Paradoxides Tessini Brongn. 

This division consists, in Schonen, in Bornholm and (according to 
an oral communication of prof. MogerG) to the South of Mörbylinga 
in Oeland, of limestone, which after this Trilobite is at present 
mostly called Exsulans-limestone, whilst it ceased to be called Coro- 
natus-limestone. 

GRONWALL’S opinion was brilliantly confirmed, when, on his breaking 
the stone further to pieces, remains of the Trilobites Conocory phe 
Impressa Linrs,?) Liostracus Aculeatus Ang.*) and Solenopleura Parva 
Linrs.*) were exposed to view by him. Moreover a remnant of 
Acroteta Socialis v. Seebach was found, which, however, also oceurs 
in older and in younger layers, which is not the case with the 
Trilobites mentioned just now. 

The only remnant that has been well preserved, is a mid-shell of 
Conocoryphe Impressa Linrs. It is for the greater part exposed to 
view. Only on the sides it is still covered by the stone; so the 
facial sutures are invisible. It must have belonged to a young indi- 
vidual, its length being only 6 millimetres. It is slightly vaulted, the 
glabella a little more than the other part. In front it is bounded by 
a flat border along the edge, which border is broadest in the middle. 


1) Linnansson. Om. Faunan i Kalken med Conocoryphe exsulans (Coronatus- 
Kalken). Sveriges geologiska Undersökning. 1879. Ser. G. No. 35. pag. 15. tafl. II, 
fig. 24,20; 

2) LinNARsson. loc. cit. pag. 20. tafl. IL fig. 29, 30. 

3) _LinNArsson. loc. cit. pag. 11. tafl. 1 fig. 12—15. 

4) Linnarsson. loc. cit. pag. 14. tafl. I. fig. 16—19, 20? 


( 657 ) 


The occipital furrow is shallow, especially on the glabella. The neck- 
ring broadens towards the centre and bears a little tubercle there. 
The breadth of the glabella is at the back equal to its length, which 
is half the breadth of the mid-shell. The glabella becomes gradually 
narrower towards the front; in front it is rounded. On either side 
there are three very indistinct lateral furrows. The dorsal furrows 
are little developed. In front of the glabella the cheeks run almost 
imperceptibly into each other. On either side an oblong elevation is 
visible on the firm cheek, just behind the place where the dorsal 
furrow turns down towards the centre. It is scarcely to be observed 
that starting from this elevation a line-shaped one runs in the direction of 
the corners of the cephalon, as LiNNARSSON tells us. This must certainly 
be attributed to the eireumstance, that this mid-shell belonged to a 
young individual. The scale possesses no other sculpture than countless 
very fine impressed points, placed very close to each other. 

From the properties mentioned above one may easily convince 
oneself that the mid-shell described comes from Conocory phe impressa 
Linrs., and that consequently this erratic-block is a piece of Exsulans- 
limestone. 

The other Trilobites-remains, all of them pieces of mid-shells, are 
too incomplete to be described in such a manner, that the species of 
Trilobites which they come from might be recognized from the 
description. Moreover, such a description would be more or less 
superfluous, as the age of this erratic-bloek has already been suffi- 
ciently indicated. So I think I’d_ better leave it and refer to the 
authority of Dr. GRÖNwALL with regard to the remains of the other 
Trilobites mentioned. As he was so kind as to send me some mid- 
shells of these Trilobites for comparison, I could convince myself of 
the correctness of his determinations. 

As was mentioned above, Exsulans-lime is found as firm rock in 
Bornholm, in Schonen, and southward of Morbylanga in Oeland. 
Mörbylânga does not seem to have been mentioned yet in literature 
in this connection; but Prof. Mosrre told me of it. In Schonen, 
Exsulans-lime is without any doubt met with as firm rock near 
Andrarum, Gislöf and Kwiks Esperöd. Most probably it is also found 
as such, according to Linnarsson, near Fagelsang in the neighbourhood 
of Lund. 

GRONWALL tells me that my erratic-block does not, petrographically, 
correspond with the Bornholm Exsulans-lime, more with that in 
South-East Schonen. | cannot decide whether it also resembles that 
which is found at Mörbylänga in Oeland. 

In the Dutch diluvium an erratic-bloek of this kind was never 


before found. They also seem to be very rare in the German diluvium. 
As far as I have been able to find out, they are made mention of 
by SrouLur *) only. 


Mathematics. — “An analytical expression for the greatest common 
divisor of two integers.” By Prof. J. C. Krurver. 


In this paper we propose to construct certain functions z of two 
real variables 2 and y which for positive and integer values of these 
variables become equal to the greatest common divisor of . and y. 

A very simple solution of this problem is obtained as follows. 
Denote by [uw] the integer part of the number w and consider the 
arithmetical discontinuous function 


1 
P (u) S55 [u] = 
For any integer 7 we have 
1 1 
P(u + n) = P(w), P(x + 0) = — —, Pe OS 
We will take 
] 
Pin) =P in —)) == Be 


9 


and consequently 
n= Tn — 0E 2-— 1. 
Integer values of w excepted the wellknown relation 
1 Si 2 JEAN OL 


Pt) EE — 
n=l a TN 


holds and from it we deduce the identical equation 
pil u Pa up 
=> Plwt—jJ= 2 Plut+—]= P(e), 
p=0 a po a 
where « and 3 are relative prime integers. That the identity is 
still valid for integer values of 7 may be easily verified. 


By the equation 
vt pl Mes ot 
al) av 


a discontinuous function of the variables 7 and y is defined. We 
may regard it as a first solution of the proposed problem. For if 


1) SrouLey. loc. cit. p. 41. 


( 659 ) 


x and y become integers, say rv—aD, y= D, where « and g are 
prime to each other, we have 


bf kas ) uy aa it ae ) e eG ‘ == 
zen ee DS Pf ADRS 


„0 wv p= at 


In a somewhat different form this result is found in a paper by 
Stern’). A whole set of functions of the required kind may be 
deduced’ in quite the same way. We only have to notice that the 
function 


N= ¢os 2 HN U 
F,(«) = + — = stek) 


n=l n 


satisfies the fundamental relation 


mm | | 3 

e ~ y u 5 iy 
SF. (ute jas Fl ut | ator, (an), 
y=0 3 « vs) a 


where again @ and 8 are prime to each other. 


Hence if we put 
nf] F 
P10) 28 = ae (tE) ET GEE 


, 
=U wv 


we get for rc=aD, y= BD 


— l 2 „zal 2 
F,(0) 2 =D SF, (“) =@IDs XF, (Een, F(0), 


mn |) a u) a 
that is 
z= D. 


: : ; + { He : 5 
In the functional relation (ID) the term 4, (2) is not easily 


Lv 
evaluated; hence the series /’,(«#) may be suitably replaced by the 
latter of the two series 


en sn2wnu 


NB vwos2 an U 
gay: (u) = 2(—1)-1 ZS ——-- 
' 9 2: 
a (2 bej 4 n)? el 


Indeed, if we denote the Bernoullian polynomial of order i 
yn+i 1 am jen yin—l B, yn-3 
(m1)! Dede. Alet 4. (m—3)! 


by jm(u) the series y,, (Ww) is identical with /",, (u) for all values of 
uw between zero and unity. Therefore, whatever may be w, the series 
Im) may be regarded as a polynomial of the mt degree in 


1) “Zur Theorie der Function £(x).” Journal f. Math., 102, p. . 
45 


Proceedings Royal Acad. Amsterdam. Vol. V. 


( 660 ) 
u—{u| so that, if in the equation (II) we replace F (u) by gar (w), 


: ye lt u 
(—1)! Be 2k — gl SS Jak (2) REN or 2 (II) 


av 


p=0 
the thus defined function z is algebraically expressed in wv and y. 
Jut as well as in the equations (I) and (II) 2 is still discontinuous 
for integer values of 1 in equation (IID. By a slight alteration it 
is possible to make these discontinuities disappear. Without altering 
the value of ¢ for integer values of « and y we may write instead 
of (UD) 


I yp — [el] 1] 1 Li 

(ena as Sees (2) + > gak (0) + gar (4) Pw), (LV) 
pay { ik wv 4 

and the function 2 has become continuous everywhere. The same 


however is not true for the partial derivatives of 2 with respect to 
vor y; besides there is as in equations (1) and (II) a lack of symmetry. 
By interchanging w and y the value of 2 alters. To some extent 
these disadvantages may be eliminated. The process of integration is 
apt to level finite discontinuities, moreover symmetry may be intro- 
duced by it. And indeed a suitable expression of 2 in the form of 
a definite integral can be given. 
We consider the function z defined by 


1 


22k — gk wf gi (ru) ge (yu) da. ay a 


0 


By, 


2k! 


Now 2 depends symmetrically on « and y and is continuous 
throughout. The function has continuous derivatives; we may different- 
iate z a number of £—1 times with respect to # and also 4—1 
times with respect to y, either separately or subsequently, before 
the derivatives lose their continuity, so that by making / larger 
and larger the behaviour of z tends more and more to that of an 
analytical function of two real variables. 

We now again substitute in (V) «=aD, y= BD and as the 
trigonometrical series gz (ev) and yp (yu) are absolutely convergent 
(ander the supposition 4 >> 1) we may multiply termwise and 
integrate the partial products. 

But after integration a nonvanishing amount is furnished only by 
those partial products 

sim SU 


2ahaDu 
Cos 


‘Qal3Du, 


COS 
in which we have 


( 661 ) 


henee we find 


B. 4 Prk ly=o 
Ee Ne Prk 
2k! (2.2)? 2 yal gek 2k! 5 
and as before 
z == D. 


Had we integrated the product gn (eu) gu (yi), where m+n is 
even, urstead of gn (wt) gm (yu) the result would have been similar, 
only symmetry would have been lost. 

We may remark that the z in equation (V) is still an algebraical 
function. For remembering that 


d 
— Ok (U) = 94-1 (wu), 
du 

g, (u) = P (w), 


we deduce by repeated partial integration 


B. rs y= k—2 
in En (lr ale yk lt apy (w) ge (4) + 
== || ek 
ae (le? veok-l OP (wit) gar (yu) } k -f- (—1)* Py Jar +1 (Y)s 
— « 
or finally : 
Bi. „=k?2 
= ai 2 , (—1)? ak yi? gj (€) ge (y) + 
wk 
seer dk Jh (4) + 
Ll (Ly I 
Hikari) gon (EL) 4 — you (0) + you (y) P(e}. (VD) 
mil d a 


„al: 


From this equation we infer that the product 22% is a rational 
integral function of . and y of degree 4 J + 2, and generally speaking 
the equation represents an algebraical surface S of that degree. But 
it should be noticed that this surface S in reality is composed of an 
infinite number of partial surfaces, having contact more or less close 
along a system of plane curves C. And in fact the larger the integer 
kk be chosen the closer will be the contact of the partial surfaces. 
Equation (VI) contains the equations of all the partial surfaces, but 
each of them has a distinct equation the coefficients of which are 
made up from the integers 


[a], [y] and | | pee a TBS 7 a 


Hence we pass from one partial surface to an adjacent one in 
all places, where one at least of these integers increases by unity. 
45% 


WI 


Hi 


( 662 ) 


Thus the projections on the .y-plane of the curves € are of two 
distinct categories. To the first belong the straight lines w=n, y==n, 
regularly dividing the wy-plane in equal squares of side unity. The 
second category is formed by straight lines issuing from the vertiees 
of these squares and which, if produced, would pass through the 
origin. The number of these lines, which have their points of issue 
inside the square, bounded by the v-axis, the y-axis and by the lines 
vn, y=n is seen to be 22¢(n)'), that is on an average equal to 
6 
2 wm. Therefore the partial surfaces remote from the origin ultimately 
take the form of infinitely narrow strips, the length of which varies 


fron. foxy 2: 


In order to lower as far as possible the degree of the surface $, 
we should take 4=1 and we have from (V) and (VI) 
1 ; . \ p=[r] Ly il ts 
— 2=ary | Pau) Plyu)du=ad > 9, - J+ —4,(0)+9,(y) P(x) | — — 9, (y)- 
12 ; ; | pol ‘4 v Dig: iat \ y LN 


0 

A comparison with (LV) makes it evident that for integer values 
of rv and y the quantity 2 still becomes equal to the greatest common 
divisor. The surface S is of the 6% degree, the partial surfaces still 
hang together everywhere but in this case they have no contact along 


the curves C. 


Physics. — “On marina and minima of intensity sometimes obser- 
red within the shading of strongly widened spectral lines.” *) 
By Prof. W. H. Juus. 


While examining a series of photographs of the solar spectrum, 
made by Rowrarp in 1888 and 1889, Jewen. discovered one plate 
on which the shading of /7 and A was broken up into a system 
of faint, nebulous lines, symuinetrically arranged about the central 
absorption lines*). The distances apart of the component lines of 
the series increased as the distance from the central line increased. 
On some other photographs of the solar spectriun, taken by RowraNp 
and by himself, he only found feeble indications of these series; but 

') » (7) denotes the number of integers less than ” and prime to #. 

*) Part of the contents of this communication has already been shortly mentioned 
in a foot-note which was added to the English translation of a former paper 
(Proc. Roy. Acad. Amst. IV, p. 601) but did not occur in the Dutch original of 


the same. 
°) L, E. Jewett, Astrophysical Journal, IL p. 108, 1896, and VIL, p. 51—93, 1898, 


a 


mad Mt in «4 ee ah. RE nan en SE eee ae 
ee 
eS 


( 665 ) 


in the shading of some of the strongest lines of iron and a few 
other elements a similar structure was observed, the component lines 
being faint, nebulous, and close together. 

The plate which showed the structure of Hand A most plainly, 
displayed an additional peculiarity, as on it the general shading of 
those lines was unusually weak. 

In Hatn’s abnormal spectrum '), which was characterized by the 
extreme weakness of the shaded background of many absorption lines, 
maxima and minima of intensity were also distinguishable under a 
microscope, though they did not appear so clear nor so regularly 
arranged as in the case deseribed by Juwerr. 


If we suppose the principal cause of the shading of the Fraunhofer 
lines not to be the absorption, but rather the anomalous dispersion 
of the waves, which in the spectrum are situated on either side the 
central absorption line *), we can easily account for the phenomenon, 
before mentioned, as well as for the fact, that in very rare cases 
only it shows distinetly. 

Let us consider a narrow beam of light of an exactly defined 
wave-length, belonging to the shaded background of a Fraunhofer 
line. This beam has emerged from the deeper layers of the Sun 
with a certain divergence; we suppose it to proceed in the approxi- 
mate direction of the structure lines of the corona (l.c. p 597). Let 
iis wave-length be somewhat greater than that of the absorption 
line; for this kind of light, the medium will then possess a positive 
refraction constant, and the separate rays of the beam will curve 
about the denser parts of the “tubular” structure. If we had supposed 
the wave-length to be a little less than that of the absorption line, 
the refraction constant would have been negative and the rays 
would have curved about the rarer parts of the coronal structure. 
In either case the divergence of our monochromatic beam will alter- 
nately diminish and increase, and this partieular kind of light will 
reach the Earth with an intensity, determined by the degree of 
divergence (convergence perhaps) with which the beam left the 
ultimate traces of the corona. 

With respeet to a beam of other light, the wave-length of which 
differs only slightly less from that of the absorption line, the medium 
will have a considerably greater refraction constant, so that the rays 
of this particular beam may have made a bend, or part of a bend, 
more than those, belonging to the former beam, on their way through 

1) G. E. Hare, Astrophysical Journal, XVI, p. 232, 1902. 

*) W. H. Juus, Proc. Roy. Acad. Amst. IV, p. 589—602, 


( 664 ) 


the corona. This beam may, accordingly, arrive with a quite different, 
say a greater, divergence and consequently display a smaller intensity 
in the spectrum, than the neighbouring beam, first considered. 

Approaching still nearer to the absorption-line we shall come across 
waves that reach the Earth in beams whose divergence is smaller 
again, showing increased intensity, ete. It is plain that in this way 
periodical alternations of light and dark on either side the central 
absorption line must arise. The waves, corresponding to the middle 
of one of these fringes, will have achieved exactly one whole bend 
‘i.e. the distance between two consecutive points of inflexion of the 
path) more, or less, than those corresponding to the middle of the 
adjacent fringes. 

From the familiar type of the dispersion curve it follows directly, 
that, in moving away from the absorption line, to equal differences 
in refraction constant increasing differences in wavelength will 
answer. The distance between the fringes will accordingly increase 
from the centre to either side, as has in fact been observed. 

Our explanation requires besides, that this system of faint lines 
should be visible only when sunlight reaches us exactly along a 
coronal streamer of sufficient length. In my last paper (le.) I showed 
that, in case this condition is fulfilled, the average shading of the 
Fraunhofer lines must be abnormally weak. It is therefore not to be 
wondered at, that on the plate, plainly displaying the peculiar structure 
of H and A, the shading really was unusually faint. But the 
formation of a well defined line-system demands a further condition 
to be fulfilled, viz. that the configuration of that part of the (rotating) 
corona we are just looking through, offers all but the same aspect 
as long as the photographic plate is exposed. This, of course, requiring 
very special circumstances, we see why even in cases, in which the 
shading of the Fraunhofer lines is weak, the fringes may be missing 
all the same. 


In a few eases has a like structure been observed with some 
strongly widened emission lines of the arc-speetrum. Kayser came 
across this phenomenon in a line of the lead-spectrum *) ; ROWLAND 
too seems to have observed it once; and after many vain endeavours 
JEWELL succeeded in obtaining a photograph of the are spectrum of 
calcium, in which at /7 and A the series appeared rather distinetly. 
This plate was obtained by using an extremely powerful direct current 
and exposing for three or four seconds only. Under these conditions 


1) H. Kayser, Handbuch der Spectroscopie, Il, p. 353. 


( 665 ) 


the heated calcium vapour formed a much more extended atmosphere 
around the poles than with a weaker current. 

Kayser *) asserts, though, that it has hitherto remained unknown, 
what are the exact conditions upon which the phenomenon depends. 

In connection with the preceding considerations, 1 hold it possible 
that in those experiments the metallic vapour has, during the (short) 
exposures, formed a kind of flame of tubular structure, which happened to 
be in the exact direction of the spectroscope. This view seems reasonable 
if we bear in mind the well-known “blowing” which is of frequent 
occurrence in a powerful are loaded with much vapour. The radiations, 
proceeding from the core of the arc, which caused the wide emission 
band, underwent anomalous dispersion in the enveloping vapour and 
traversed the flame-shaped streamer, following sinuous paths. 


A simple experiment convinced me that the peculiar light-distribution 
observed in all strongly widened Fraunhofer lines’), may be strikingly 
imitated in the absorption-spectrum of sodium vapour. The only 
thing necessary was to force the absorbing vapour into a more or 
less tubular structure, such as we presumed it to exist in the corona. 

A slightly converging beam of electric light was thrown on to 
the slit of a grating-spectroscope. At a distance of rather more than 
100 ¢.m. from the sht, and about 1,5 ¢m. below the axis of 
the beam was the opening of a specially constructed bunsen-burner, 
from which a sodium-flame emerged. This opening was slit-shaped 
(30 ¢.m. long, 0,2 ¢.m. wide) and adjusted in a position exactly 
parallel with the axis of the incident beam. The pressure of the 
gas was somewhat variable, and a good regulator unfortunately not 
at hand. In order to supply the long flame with sodium, the con- 
sruction of the burner included a kind of narrow gutter on either 
side, into which had been poured a solution of a sodium-salt. This 
ascended into the flame by strips of asbestos paper. When viewing 
this flame lenethwise, it was as if one were looking through a com- 
pressed tube, the sides of which consisted of sodium-vapour. The 
density of the vapour diminished gradually towards the centre as well 
as towards the outside. 

The sodium-lines were observed in the spectrum of the third order. 
In spite of the great length of the flame the real absorption lines 
were narrow; they stood out from a pretty dark softly shaded 
background, the width of which amounted to several ÄNGsTRÖM 
wuts. The distribution of the light entirely corresponded to JEWELL’s 


Ye p. 354. 
2) Jewett, Astroph. Journ. Ill, p. 101; Hare, Astroph. Journ. Ill, p. 156—161, 


( 666 ) 


deseription of the strongly shaded Fraunhofer lines. Close to the 
central absorption line there was also an unmistakable increase of 
luminosity (resembling the supposed emission lines in the solar spec- 
trum); but this increase ought, without doubt, to be attributed to 
the most strongly curved rays being kept together by the tubular 
structure of the flame, and not to direct radiation from the flame. 
For, the electric light being intercepted, the emission-lines were 
scarcely visible in the dark field. And besides, as soon as the flame 
was disturbed by blowing upon it, or when it was partially covered 
by a diaphragm, the bright band, as well as the shading, became 
unsymmetrical with respect to the absorption line. Neither Doppier’s 
principle, nor the influence of pressure on wave-length can here 
have played an appreciable part. 

I moreover observed fringe-like maxima and minima in the shadings, 
but they showed irregular and so unsteady, that T could not think 
of measuring their distances. Nor can there be any question 
of photographing this peculiarity before means have been devised 
to keep a structure of sodium vapour, as deseribed above, steady 
for a reasonable time. Such means are however being prepared. 

Imperfect as our present experiment must be, it still serves to 


bear out the assertion, that numerous peculiarities of the solar speetrum - 


may be explained from anomalous dispersion. 


Physics. — “On the emission and absorption by metals of rays of 


heat of great wave-lengths.’ By H. A. Lorentz. 
Gk \ ” 


§ 1. Hagen and ReBexs have recently shown by their measure- 
ments of the reflecting power of metals *) that the behaviour of these 
bodies towards rays of great wave-lengths (larger than 8 u) may be 
accounted for, if one applies to the propagation of electric vibrations 
the equations that hold for slowly varying currents, and which con- 
tain no other physical constant of the metal but its conductivity. It 
follows from this result that a theory which can give an adequate idea 
of the mechanism of a current of conduction will also suffice for the 
explanation of the absorption of the rays that have been used by these 
experimenters. A theory of this kind has been developed by Rirckn *) 
and Dreper *). According to their views a metal contains an immense 
number of free electrons moving to and fro in much the same way 
as the molecules of a gas or as the ions in an electrolytic solution, 

1) Hagen and Rupens, Berliner Sitzungsberichte, 1903, p. 269; Berichte d. deut- 
schen phys. Gesellsch., 1903, p. 145. 

2) Riecke, Wied. Ann., Bd. 66, p. 353, 1898. 

3) Drupe, Drude’s Ann., Bd. 1, p. 566, 1900, 


7 


—— = 


( 667 ) 


the velocity of agitation increasing with the temperature. It is to be 
assumed that, in this “heat-motion”, every electron travels along a 
straight line, until it strikes against a particle of the metal; the path 
will therefore be an irregular zigzag-line and, so long as there is 
no cause driving the electrons in a definite direction, an element 
of surface will be traversed by equal numbers of electrons, travelling 
to opposite sides. Things will be different if the metal is exposed 
to an electric force. The motion of the electrons will still be an 
irregular agitation; yet, motions in a definite direction will predo- 
minate, and this will show itself in our observations as an “electric 
current.” 

Now we may infer from the relation between absorption and 
emission that is required by Kirennore’s law, that the mechanism by 
Which the emission of a body is produced is the same as that to 
Which it owes its absorbing power. It is therefore natural to expect 
that, if we confine ourselves to the case of great wave-lengths, we 
shall be able to explain the emission of a metal by means of the 
heat-motion of its free electrons, without recurring to the hypothesis 
of “vibrators” of some kind, producing waves of definite periods. 

In the following pages this idea has been worked out. After having 
calculated the emissive power we shall find that its ratio to the 
absorbing power does not depend on the value of those quantities 
by which one metal differs from another. According to the law of 
Kirennorr, the result may be considered as representing the ratio 
between the emission and the absorption for an arbitrarily chosen 
body, or as the emissive power of a perfectly black substance; it 
will be found to contain a certain constant quantity, whose physical 
meaning will appear from the theory. 


§ 2. The ratio of which L have just spoken is intimately connected 
With another important physical quantity, viz. the density of the enerey 
of radiation in a space enclosed by perfectly black walls, which are 
kept at a uniform absolute temperature 7. If the electromagnetic 
motions of which the aether in such a space is the seat, are deeom- 
posed into rays travelling in all directions, and each of which has 
a definite wave-length, the energy per unit volume, in so far as 
it belongs to rays with wave-lengihs between 2 and 2 + dà, may 
be represented by : 

F (a; T) da, 
F’ being a function which many physicists have tried to determine. 
BOLTZMANN and Wier have shown by thermodynamical reasoning 
that the above expression may be written 


( 668 ) 


1 
SADE 


where f (2 7’) is a function of the product #7. Afterwards Pranck ') 
has found for (1) the form 


Here ¢ is the velocity of light in aether and / and & are univer- 
sal constants. 

In the theory of PLaNnck every ponderable body is supposed to 
contain a great many electromagnetic vibrators, or, as PLANCK calls 
them, “resonators”, each of which has its own period of free vibra- 
tion, and which exchange energy with the aether as well as with 
the molecules or atoms of ponderable matter. The conditions of 
statistical equilibrium between the resonators and the aether may be 
thoroughly investigated by means of the equations of the electro- 
magnetic field. As to the partition of energy between the vibrations 
of the resonators and the molecular motions in the body, PLANcK has 
not endeavoured to give an idea of the processes by which it takes 
place. He has used other modes of reasoning, of which I shall only 
mention one, Which is to be found in his later papers on the subject and 
which consists in the determination of that distribution of energy that 
is to be considered as the most probable. I shall not here discuss the way 
im Which the notion of probability is introduced in PLANck’s theory 
and which is not the only one that may be chosen. It will suffice 
to mention an assumption that is made about the quantities of energy 
that may be gained or lost by the resonators. These quantities are 
supposed to be made up of a certain number of ginite portions, 
whose amount is fixed for every resonator; according to PLANCK, the 
energy that is stored up in a resonator cannot increase or diminish 
by gradual changes, but only by whole “units of energy”, as we may 
call the portions we have just spoken of. Besides, PLANck has found 
it necessary to ascribe to these units a magnitude depending on the 
frequency 2 of the free vibrations of the resonator, the magnitude 

hn 


represented by —. 
n 


being 


o 


As to the constant %, it has a very simple physical meaning; — 47 
) - | « ORTE) 


is the mean kinetic energy of the molecule of a gas at the tempe- 
rature 7’. 


1) Prange! Drude's Ann., Bd. 1, p. 69, 1900; Bd. 4, p.p. 553 and 564, 1901, 


( 669 ) 


It appears from the above remarks that the hypothesis regarding 
the finite “units of energy”, which has led to the introduction of the 
constant /, is an essential part of the theory ; also that the question 
as to the mechanism by which the heat of a body produces electro- 
magnetic vibrations in the aether is still left open. Nevertheless, the 
results of PLANcK are most remarkable. His formula represents very 
exactly the energy of the radiations for all values of the wave-lengths, 
whereas the following considerations are from the outset confined to 
long waves. We may at best expect to deduce from them the 
form which the function in (1) takes for this extreme case. 


§ 3. Since, if we trust to Kircnorr’s law, the ratio between the 
emission and the absorption must be regarded as independent of the 
dimensions and the position of the body considered, we may simplify 
the problem by an appropriate choice of circumstances. 1 shall 
therefore consider a plate with parallel plane surfaces and I shall 
suppose its thickness A to be so small that the absorption may be 
reckoned proportional to it and that the energy emitted by the pos- 
terior layers may be supposed to pass through the plate without any 
sensible absorption. I shall also confine myself to the absorption’ of 
perpendicularly incident rays and to the emission in directions making 
infinitely small angles with the normal. 

Let o be the conduetivity of the metal, i.e. the constant ratio 
between the electric current and the electric force, these latter quan- 
tities being expressed in the modified electrostatic units 1 have lately 
introduced. *) Then the absorbing power of the plate, the coefficient 
by which we must multiply the energy of normal incident rays, in 
order to get the absorbed energy, is given by *) 

Ee a ae 
F 

Here we shall substitute for o the value furnished by Drupr’s 
theory. Let the metal contain different kinds of free electrons, which 
we may distinguish as the 1s, the 2.4, the 3'¢ kind, ete., and let 
us suppose that all electrons of one and the same kind have equal 
charges, equal velocities of heat-motion, or, as we may say, “molecular” 
velocities, and travel over paths of equal mean length between two 
successive encounters with particles of the metal. 

We shall write e 


ae for the charges of the different kinds 


of electrons, w,, w,,... for the mean molecular velocities, /,, /,,... 


2) 


1) Lorentz, Proceedings Acad. of Science, Amsterdam, Vol. 11, p. GOS, 1903, 
>] Oo b J ’ | » 
*) See § 12 below. In electromagnetic units the formula becomes 


A —= Arco. 


( 670 ) 


for the mean lengths of the free paths, .V,, .V,,... for the number 

of electrons of the several kinds, contained in unit of volume. We 

shall finally suppose, as Drepr has done, that for every kind of 

electrons, the mean kinetic energy of one of these particles is equal 

to that of a molecule of a gas at the same temperature; we may 

represent it bve 7, if 7’ is the absolute temperature, and « a constant. 
In these notations Drupr’s value is *) 


1 
6=- —‘(e;" N, if u, + e,? et. U vete (4) 
Aa 1 : ous 


so that (3) becomes 


1 
—(e,? Nil, u, He, N, l,u, +...) Ds 


MEN 


dae! 

It is to be remarked that the formula (4) has been obtained in the 
supposition that the electric force remains constant, or at least that 
it keeps its direction and magnitude during an interval of time in 
whieh an electron has undergone a large number of collisions against 
particles of the metal. The results of HaGeN and Rupes are therefore 
favorable to the view that even the period of vibration of the rays 
is very large in comparison with the time between two succeeding 
impacts. Part of the following calculations are based on this assumption, 


§ 4. We have now to examine the emission by the plate. It 
follows from the fundamental equations of the theory of electrons, that 
every change, whether in direction or in magnitude, of the velocity 
of an electron produces an electromagnetic disturbance travelling 
outwards in the surrounding aether. Hence, it will be at the instants 
of the collisions that the electrons become centres of radiation. We 
shall caleulate the amount of energy, radiated in this way, in so far 
as it is emitted across a definite part @ of the front surface of the 
plate; this part of the emission is due to the electrons contained in 
a volume m4 of the metal. 

Let © be a point within the area w, OP the normal in this point, 
drawn towards the side of the aether, and 7? a point on this line, 
at a distance 7 frem QO, which is very large in comparison with the 
dimensions of w. In this point ? we place an element of surface @’, 
perpendicular to OP; our problem will be to calculate the energy 
radiated across this element. | choose QO as origin of coordinates and 
OP as the axis of 2. The components of the velocity of an electron 


will be denoted by vu, u, Uz. 


1) Drupe, Le, p. 576. This formula does not change by the introduction of our 


new units. 


a hs À ee 


(GT) 


Now, if an electron with charge e, is in O at the time f, and has 
du, du, dur 


at that instant the accelerations ——, ‚==, it will produce at the 
dt dt dt 


, y . 
point /, at the time ¢ + —, a dielectric displacement, whose com- 
( 


ponents are *) 
e du, e du, : 
— —— — ., — Te eS es, 

Amer dt 

On account of the great length of OP, these expressions may also 
be applied to an electron situated, not in QO but in any other point 
of the part of the plate corresponding to the area w. The whole 
dielectric displacement in 2? in the direction of wv (it is only this 
component that will be considered in the next paragraphs) at the 


We 
time t + — will therefore be 
{fs 


Dr = — — PNM a onsite de HP 


if the sum is extended to all electrons present in the volume wA 
at the time ¢. 

There will also be a magnetic force of the same numerical value, 
and by Poyntine’s theorem a flow of energy across the element w', 
in the direction from the plate towards P. The amount of this flow 
per unit of time is given by 

EE LEENE) 


$ 5. It will be necessary for our purpose to decompose the whole 
emission into rays of different wave-lengths and to examine the part 
of (8) corresponding to the rays that have their wave-lengths within 
certain limits. ‘This may be done by means of Fourimr’s series. 

Let us consider a very long time, extending from ¢= 0 to f= 9. 
During this interval the value of }, at the point 7 will continually 
change in a very irregular way ; it may however in every case be 
expanded in the series 


JE oe 99 …_ matt 
Oe ee Ain B en ee des ee (eli 
Mm t 


whose coefficients are given by 


df. … mat 
On max | EO OENE EEN: beta. te, (LO) 
D. Ù 


0 


1) The proof of Uus will be found in one of the next parts of my “Contribu- 
tions to the theory of electrons.” 


Now, if the plate is kept at a constant temperature, the radiation 
will also be stationary and d,? may be replaced by its mean value 


1 . 
Dn == =| De dt 
0 


during the time 9. Substituting the value (9), we get integrals of 


two different kinds, some containing the square of a sine, and others 
the product of two sines. The integrals of the second kind will 
disappear, and 


= 
De 


Tt ETE 1 
sin? i=. 3. 
Ya LN 


a 


so that 


=e | z= 
%,,| 

pee Sawa ee 
kli! 


As to the frequeney of the terms in (9), it is given by 


nr 12) 
== 3 En er eN GN: a 
5 az 


| 


it will therefore increase by equal differences if we give to m its 


successive values. 
By choosing for ® a value sufficiently large, we may make this 

ie B 

step — as small as we like, so that ultimately, even between two values 
vo 

of the frequency and # + dn, which are in a physical sense 

infinitely near each other, there will be a certain number of values 

of (12) and of corresponding terms in the series (LI). The number 


0 
of these terms will be — dz, hence, if we suppose an, or 


eo ip 


9 
ad 
an == ken nbd, ds at oe ER 
ut zl 
0 


to have the same value for each term of this group, the corresponding 
part of (11) will be 


i, On. 


me 
Substituting this for »,? in (8), we get for the radiation across 
w’, due to the rays with frequencies between 7 and 7 + dn, 
co 


EDE an RS En oe ee eee: eee (14) 
Jt 


a 


Se ee ll 


( 673 ) 


§ 6. We have now to calculate the coefficient a, by means of 
(13). After having substituted in the integral the value (7), we may 
still take for its limits O and ®, provided we reckon the time from 


5 
an instant, preceding by the interval — the moment from which it 


c 


has been reckoned till now. Thus: 


3 
il i : dit, 
n= — >| ef sin nt. — dt |, 
2x Ur / dt 


0 


or, after integration by parts, since sz nt vanishes at the limits, 


1 ut r 
tm — —— oe ESM CORI AME Ae en ( 15) 
Zrce Or 


The sum in these expressions relates to all the electrons in the 
part wA of the plate and it is by reason of the immense number 
of these particles that a definite value may be assigned to an. 

We shall begin by determining «?,, and the amount of the radiation 
in the supposition that there are only free electrons of one kind ($ 5). 
We shall write ¢= NwA for their number, e for the charge of 
each of them, and we shall further simplify the problem by supposing 
that the molecular velocity w, the same for all the electrons, is not 
altered by the collisions and that all the paths between two successive 
impacts have exactly the same length /. Then, the time 


l 
— 
u 
will also have a definite length. 
§ 7. Let ¢,,¢,,¢,,... be a. series of instants, between 0 and 9, at 


intervals + from each other. Then it is clear that, if we fix our 
attention on the positions of a single electron at these instants, we 
shall have one point on each of the sides of the zigzag-line described 
by this particle. 

Now we may in the first place determine the integral in (15) for 
the lapse of time during which an electron travels over the side of 
the zigzag-line on which it is found at the time ¢& As the length 


sate ts ee. 
rt of this interval is much shorter than the period — of the factor 


n 
cos nt, we may write for the integral 
GOE NIE Ug Wt vab va tee, Wte ALO) 


It is clear that we shall obtain the sum in (19), for the g electrons, 


if, after having multiplied (16) by e, we perform the two summations, 
indicated in the formula 


[cos nij = Dil rn EN (17) 
k 


We have in the first place to take the sum of all the values 
of u, for the system of electrons, at a particular instant #7, and 
then to add together all the results obtained in this way for the 
instants 7,,7%,, ete. 


$ 8. If we wish to find Sw, for a given time, we must keep 
in mind that the velocities wv of the electrons have at that instant 
very different directions. We may represent all these velocities by 
vectors drawn from a fixed point C. The ends JD of all these vectors 
will lie on a sphere with radius v, and if we let fall from each of 
these points a perpendicular DD’ on the diameter of this sphere 
that is parallel to OX, the distances of the projections from C will 
give the values of w,. The sum of all these values may therefore 
be represented by 

a qs: 
if $ is the positive or negative distance at which the centre of gravity 
of the points D’, considered as equal to each other, is situated from 
the centre ©. 

Of course, on account of the large number of the points, this 
distance will be very much smaller than the radius 7, and, if we 
repeat the construction of the diagram of velocities for each of the 
instants f£,. f,..., the small value that is found for § will be positive 
in one case and negative in another. It is to be remarked in this 
respect that there is no connexion at all between the values of &, 
which we shall find for two succeeding instants in the series ¢,, 4, ... 
Indeed, between any two such instants, every electron will have 
undergone a collision, and it may safely be assumed that, whatever 
be the direction of motion of an electron before the impact, all 
directions will be equally probable after the impact ‘). 

Now, in order to determine a?,, we have to take the square of 
the sum denoted by + in the formula (17). This square consists of 

k 
terms of two kinds, some having the form 


cos? n t FS a = 7 cos* nt 5, | 24S ae ae 


eh 


1 This is easily shown, as has been done by Maxwett in his first paper on the 
kinetic theory of gases, if both the electrons and the particles ot the metal are sup- 
posed to be perfectly elastic spheres. z 


\ 
Dn | call 


—. =" 


and others the form 


2 cos nt, cosnt,, [2 = u = 2 q’ cos nt, cos nt > the 
2 cos nt, cos n ol ae el, 2 q° cos nt, cosnt,, Ss, 5, (19) 
As has already been said, the time 9 contains a very large number 


“ 


of periods ——. A certain value of cos nt, once occurring in the series 
VL : 
cosnt,, cosnt,, cosnt,,... may therefore be supposed to repeat itself 


many times. Also, one and the same value of the product cos nt, cos n ty 
may be said to occur for many different values of % and 4. 
Such a product will therefore bave to be multiplied by very different 
expressions of the form Sz Sp, and, since the different values of § are 
mutually independent, the number of cases in which §; and 87 have 
opposite signs will be equal to that in which they have the same 
sign. It appears in this way that the terms (19) will cancel each 
other in the sum. It is only the terms of the form (18) that remain, 
and we shall have 


Pay ME ee | 
5: n'e'T'g 


a = [cos? nt. Sl a ee, amet (ADI 


mde 97? 7 


§ 9. Here we may begin by taking together those terms in which 
cosnt, has one and the same value. Let the number of these be 
(. Then, we have to repeat Q times the construction of the diagram 
of velocities, and it may be asked in how many of these Q cases 
§ will lie between given limits § and §+d6, or, what amounts to 
the same thing, what is the probability for § falling between these limits. 

This question may be reduced to a simpler problem. A series of 
planes, perpendicular to O X and at equal distances from one another, 
will divide the spherical surface into equal parts. Therefore, instead 
of distributing the points D on the surface in an irregular, arbitrarily 
chosen manner, we may as well immediately distribute the points 
D' at random over the diameter, without giving any preference 
to one part of the line over another. The probability in question is 
thus found to be *) 


; 1 a 2u2 > 
er 7, 5 
Pie pee den tete 


Hence, among the Q terms in the sum, occurring in (20), for 
which the factor cos° nt, has equal values, there will be QPdé 
terms, which may be said to have the same Sj. Together, they will 
contribute to the sum the amount 


1) See SS 13—15. 
46 


Proceedings Royal Acad. Amsterdam. Vol. V. 


cos? nt. QPS dE 
and the total sum of all the Q terms is got from this by an inte- 
gration which we may extend from §=—o to §=-+o. Conse- 
quently, the sum of those Q terms will not be altered, if, in each of 
them, we replace §*, by 


+o 
Pa [peas EE 


This expression being the same whatever be the particular value 
of cos? nt, the sum in (20) at onee becomes 


> KEN TT EERE Ee 


uv 


Again, since the instants f,, ¢,,.... are uniformly distributed at 
. , 2% 
distances that are very small parts of the period —, the sum will 
vi 


remain the same, if in every term we write 4 instead of cos? nt. 


ae 2 $e: 
The number of terms being —, we find for (23) 


i 4 
a za 
De 
and for (20) 
7, 2 
ae Bere 
m Sx or? > 


We have by (21) and (22) 


5e == 5 
5 3 
l 
hence, replacing t by —, we find 
u 
: n°e? glu n?e? NluA 
am — = = == = 
24e‘ Dr" 242°C Or? 


and for the emission (14), in so far as it is due to the one kind of 
electrons that has been considered 
nie? NluA 


SSS 
48m? 6° 7? 


This value must still be multiplied by 2 because we may apply 
to the second of the components (6) the same reasoning as to the 
first component, and the total radiation from the plate may obviously 
be considered as the sum of all the values corresponding to the 


( 677 ) 


different kinds of electrons. The final result is therefore *) 


2 


An? er? 


(ec? Nl, u, He, N‚l,u, +...) Aww'dn. . (24) 


$ 10. If now we divide (24) by (5), all quantities V,e, uv and /, 

by which one metal differs from another, disappear. This is what 
might be expected according to KircmnHorr’s law and the result 

an T 
ww dn 

6n?e?r? 
may be taken to express the emission by a perfectly black body 
under the circumstances we have supposed. It represents the amount 


of energy which, in the case of such a body, is transmitted per unit 
of time across an element w',‚ in the rays whose frequency lies 
between # and „ + dn and whose directions deviate infinitely little 
from the normal to the element, being contained within a solid angle 


42 
= Multiplying by eM „ we are led to the following expression for 
r cow 
the density of energy of which I have spoken in $ 2: 
Zan? T oF 
reg dn. ° . e ° . . . . ° (25) 


Taking for the group of rays those whose wave-lengths are included 
between 2 and 2-++ dà, we get for the corresponding energy per 
unit volume 

16 xeT 


EN EN a 
a Cage (a 


1) It is easy to free ourselves frora the hypothesis that for all electrons of cone 
kind there is a single length of path / and a single molecular velocity u. Indeed, 
the motion of an electron along one of the small straight lines 7, which it describes 
between the instants O and S, will furnish for the sum in (15) a quantity 


€ COS Nt. Uy T, 


if w is the velocity for the particular line / we wish to consider, and 7 the time 
required for the motion along it. 

Now, among all these rectilinear motions between two successive encounters, of 
one kind of electrons, we may select those for which « and / have certain definite 
values and we may begin by calculating the coefficient @m and the emission, in so 
far as they depend on the part of (15) which corresponds to these particular motions; 
in doing so, we may use the method shown in §§ 7—%. The total emission 
may be regarded as the sum of all the partial values (with different /’s and dif- 
ferent w’s) thus obtained, and after all the expression (24) will still hold, provided 
we understand by /,, J)... certain mear lengths o° path and by wy, 1»... certain 
mean molecular velocities. We need not however enter into these details, because 
the conductivity and the coefficient of absorption have not been calculated with 
a corresponding degree of accuracy. 


46* 


ocr v4 : : 2 ane 
This is found from (25) by using the relation n = Pe 


$ 11. The result of the preceding calculations not only conforms 
to the law of Krrennorr; it has also a form agreeing with those of 
BorrzMaNN and Wien. Indeed, the expression (26) follows from (1), 
if we put 


. 


ere 16 
JAT 5 dl. 


Our last task will be to evaiuate the constant @ by applying the 
formula (26) to experimental determinations of the radiation of black 
bodies, and to compare the result with what has been inferred about 
the same constant from other classes of phenomena. Combining the 
measurements of LummMEr and Princsuem'), who have gone far into 
the infra-red, with the absolute amount of the radiation as determined 
by Kuripaum *), I find 

erg 


gi) ane ; 
degree 


On the other hand, we get, starting from VAN DER WAALS’ evalua- 
tion of the mass of am atonr of hydrogen, 
aes: 

A comparison of my formula with that of PLANCK is also interesting. 

For very large values of the product 27, the denominator in 


: ch ‘ ‘ SxkT Tee : 
(2) becomes ar and the expression itself dû. This agrees with 
Ot ==. 

2 


Now the mean kinetic energy of a molecule of a gas would be 
2) 
vo 
> kT according to PrarxcK and has been represented in what pre- 
cedes by «7. There appears therefore to be a full agreement between 
the two theories in the case of long waves, certainly a remarkable 


conclusion, as the fundamental assumptions are widely different. 


On the absorption by a thin metallie plate. 


$ 12. Take the origin of coordinates in the front surface, the 
axis of z towards the metal, and let there be free aether on both sides. 
Writing € for the electric force, 3 for the current of conduction, 


1) Lummer and Prinesnem, Verhandl. d. deutschen phys. Gesellsch., 1900, p. 163. 
2) Kurupaum, Wied. Ann., Bd. 65, p. 754, 1898. 


(OMD) 


DH for the magnetic force and putting the magnetic permeability = 1, 
we have for the metal 


re 
rot D= — J, rot € = — — D, mt Pp 
C Y 
It is found by these equations that in electromagnetic waves travel- 
ling in the direction of the positive z, € and § can have the diree- 
tions of OY and O Y, and values equal to the real parts of the 
complex quantities 


G ee ee arl int —4(1+ i) 2 
Ob ae 1 


Ay = *ae (27) 


a being the amplitude of the electric force, and the constants a and 


x being given by 
(1 —2) Ce 
——— 7 — 
2n 


1 1 
a= nd. x 
c Zo 


Similarly, waves travelling in the opposite direction may be repre- 
sented by 


Ve 30 epee es de Gr (25) 


gi RE En 


For the aether the corresponding formulae are somewhat simpler ; 
in the first case 


Nn ee rite > 
Fr dl Ees Dy = ae 6 Sete ee al 
and in the second 
int + pe z inti et = 
EF, — dE x ’ Jy —=—ae ‘i Set Eee oo Te (50) 


Now, if rays fall perpendicularly on the front surface of the plate, 
we may unite all the systems of waves arising from the repeated 
reflexions into the following parts: 1st. a reflected system in the 
aether, 2d, transmitted waves in the aether behind the plate, 3". waves 
in the plate, travelling towards the back surface and 4t". rays in the 
metal, going in the opposite direction. Representing the incident rays 
and the motions mentioned under these four heads by the equations 
(29), (80), (29), (27), (28), with the values a,, a,, as, @,, 4; of the 
amplitude, we have, in virtue of the conditions at the two surfaces 
(continuity of €, and 5) 


a, Ja, =a, + 4, 


ad, — a, = %(a, — 4,), 
” 
na +s ape np 
desen == ye 
el 
=S +s —i—f 
0 Cc 


( 680 ) 


In these formulae, A is the thickness of the plate, and 
Ol eee or ee eee 
The solution, in so far as it is necessary to our purpose, is 
lm Namen Ard 
ays 
Get It ee — (Ite 


1 ZE 


2 


<a 
4% tA 
A, SSS oe 2 de 

(x+1)? ets — (x—1)? e—s 
In these expressions A and consequently s are now to be supposed 

| 3 
infinitely small. Replacing es and ets by 1—s and 1-++s, one finds 

À | ed A 


1 1 ZA 
a, =| 4 == ‚(- — | a, 


The first of these equations shows that the amplitude of the rays 
reflected by the thin plate is infinitely small, so that we may neglect 
their energy as a quantity of the second order. 

As to the transmitted rays, the amount of energy propagated in 
them will be equal to the product of the incident energy by the 
square of the modulus of the complex expression 


aes} 


This square is 


Oo 
1——A, 
C 
whence we deduce for the coefficient of absorption 
5 
eee er 
c 


On the probability with which one may expect that the centre of 
gravity of a large number of points distributed at random 


on a limited straight line will lie within given limits. 


§ 18. Divide the line into a large number p of equal parts, and 
call these, beginning at the end A of the line, the 1st, the 2°¢, the 
3d part, ete. Denote by q the number of points and let q be very 
much larger than p. 

We shall imagine the points to be placed on the line one after 
another, in such a way that, whatever be the position of the points 
already distributed, a new point may as well fall on one part of 


( 681 ) 


the line as on the other. The result will be a certain distribution 
of the whole number, entirely determined by chance. Let us conceive 
this operation to be very often repeated, say Q times, and let us 
calculate in how many of these Q cases, a desired distribution of 
the points over the p parts will occur. Dividing by Q we shall have 
the probability of the distribution. 

The probability that there will be a,6,... m points on the 1**, 
2nd, .... pth part of the line (a+6+...+ m=), is given by 


a tL q q! TE 
i Os GLb kS met 


Ls ee 
In the case of a very large value =, this probability becomes 
P 
extremely small, as soon as one of the numbers a, h,...m is far 


q : ae 

below —. Neglecting these small probabilities, we shall confine our- 
P 

selves to those cases, in which each of the numbers a,/,.... i is 


very large. Then, by the well known formula of STIRLING, 


== WAS 
als [2a (<) ‚etc. 
é 


and, if we put 


a es, m ; 
===. @,— 6, == ils 
g q g 
we shall find 
log P = — 3 (p—1) log (2279) — g log p — 
— [(a'g +3) log dl +...4+(mq4+ })logm']. . . . (32) 
It is to be remarked that the numbers a, b, ...7 can only increase 
or diminish by whole units. The numbers a’, 6’... m/ can change 


| 
by steps equal to —; this may be made so small that they may be 
q 


considered as continuously variable. 


$ 14. We shall in the first place determine the values of a’, 5’, . im’ 
for which the probability P becomes a maximum. We have 


1 1 
d log P= — (1 Sig Dal + q log aa a+... +(4 x Omi + qlog nt Jan | 


with the condition 


da’ + ...+ dm =), 
which is a consequence of 
Cp lad os oN cee ee eens ete. Renee 
The maximum will therefore be reached if 


so that the uniform distribution will be the most probable. 
We shall next consider the probability for a distribution differing 
a little from the most probable one. Let us put 


1 1 1 
a—-—+a , =p , ....mM=—-+4p.. (84) 
P P Pp 
and let us suppose the numbers «a, 6.... u, to be so small in com- 
1 : 
parison with —, that in the expansion of the quantities in (32) in 
P 


ascending powers of a,?....u, we may neglect all powers surpassing 
the second. We have for instance 


ee ; gered 1 1 1 : 
agt log ad) = - PR log p+ q+5 p-qlogp ap 1-5 Pte 


1 ‘ 
where, in the last term, we may omit the term ri, beeause it is 
much smaller than g. If we put 

1 1 
Seat (p—1) log (2 a q) + ae log p = log Pn 


and keep in mind that, in virtue of (33), 


a s+ feae eb =0 Ceo. NN 


the equation (382) becomes ‘ 
i 
log P = log Pn — PG (a? +p? +....+ p’), 


1 9 zo 9 
P= Pym SPITE te THY, 


It is seen from this that ZP, is the maximum of the probability, 


with which we shall have to do, if a=f=....=p=0. The 
equation shows also that, conformly to what has been said above, 
the probability will only be comparable to P,, so long asa, 8... .u 
: 1 ms 
are far below —. Indeed, if one of these numbers had this last value, 
P 

P, would be multiplied by 

ey id 

é 2p’ 


which, by our assumptions, is extremely small. 


§ 15. Let 2u be the length of the line, « the distance along the 


; u 
line, reckoned from the end A, and let us take — for the value or 
Pp 


ahh ne dd 


TE VE MEP WT TTET ee AET we VT 


mc dn dn kene dakini we ee 


Knit se 


4 


( 683 ) 


; u 

this coordinate for all points situated on the first part of the line, 3 — 
1 

for all points of the second part, and so on. Then, in the distribution 


that is characterized by a’, 0',.... i, the coordinate of the centre of 
gravity of the g points will be 


(eee CT Ss 
or, by (34), : 
u+fa+ 38+ 5y4+-. .+2p—Yul—. 
The positive or negative value of . 
§=—[a+368+5y4....4+ pbl et (0 


is thus seen to represent the distance between the middle point of 
the line and the centre of gravity. We have to calculate the proba- 
bility for this distance lying between § and § + ds. 

The problem is easily solved by means of a change of variables. 
Instead of the quantities a, 8,....u, which serve to define a mode 
of distribution, we shall introduce new ones a’, }',....u’, the substi- 
tution being linear and orthogonal. 

Let us take for the first of the new variables 


Ee ay ees. (37) 
a = —a-- — See re Ee AN 
Vp Vp Pp 


and for the second 


| 
zeef 


p-3 pl 


a Bp—...+ pe MO 
se x x 


where the numerators form an arithmetical progression, whereas z 
means the positive square root of the sum of the squares of the nume- 
rators. These expressions (87) and (38) may really be adopted, because 
the peculiar conditions for an orthogonal substitution are satisfied : 
in both expressions the sum of the squares of the coefficients is 1, 
and we get O if we add together the coefficients of (87) after having 
multiplied them by the corresponding coefficients in (38). As to the 
coeflicients in the expressions for y',...«, we may choose them as 
we like, provided the whole substitution remain orthogonal. 

The reason for the above choice of e@ and 8 will be clear; the 
condition (35) simplifies to 

=O 3 PSA rt EEN 
and, in virtue of (35), the value (36) will be equal to 
xu 


P 
in all cases with which we are concerned. 


Now, the modes of distribution for which the value of § lies 
between & and §+d6§ are those for which #' lies between #' and 


ke 


a dp, if 


/ E 
EEE VEE eT 


XI 


Since «/=0, every mode of distribution may be defined by the 
values of 8'...w’, these quantities being, like a, 3,...u, capable of 
very small variations. 

We can therefore select, among all the modes of distribution, those 
for which 8...’ lie between 8' and 8 + d8, y' and y + dy, ete. 
The number of these may be represented by 


MAB EU et en nl orev: a) 


where / is a coefficient whose value need not be specified. It suffices 
to know that it is independent of the values chosen for 9... 
This is a consequence of the linear form of the relations between 
these variables and a, 6,...m. 

As the just mentioned modes of distribution, whose number is 
given by (42), differ infinitely little from one another, the probability 
P may be taken to be the same for each of them. Hence, the proba- 
bility for the occurrence of one of these modes, no matter which, 
must be 

EER ee 

From this we may pass to the probability for 9’ lying between 
8' and #'-++ d;', whatever be the values of y'...u'; we have only 
to integrate with respect to these last variables. Now using the funda- 
mental property of an orthogonal substitution 


eB ee ep tens ee 
and attending to (89), we write for (43) 


1 “re m=. 
Ri ane 


he a Sed: 


If we integrate this expression from — oo to + 0, as may be done 
for obvious reasons, denoting by / a coefficient that does not depend 
on 8, we find for the probability in question 


1 
Rn ta RP 
On account of (40) and (41) this is equal to 
Pais 
ee ERE 


k being a new constant. 


zeen ven mn tende gn ee 


( 685 ) 


It remains to introduce the value of x?. According to the defini- 


il 
tion of this quantity, it is a p(p?—4), instead of which we may take 


af p*, because p is a very large number. In this way (44) changes into 


(Bae A A EN can rt (45) 

We may finally determine the coefficient 4’ by remarking that 

(45), integrated from — oo to + oo, must necessarily give 1. This 
requires that 


1 39 
k! EEK ze ’ 
u 2 
so that our result becomes 
1 EE 
= eS Ceo od S. 
u An 
Microbiology. — “The decomposition of cellulose by aérobic micro- 


organisms.” By G. VAN Irerson Jr. (Communicated by Prof. 
M. W. BrIJERINCK). 


(Communicated at the meeting March 28, 1903). 


When we introduce into the soil or into natural waters substances 
consisting of cellulose, such as linen, cotton or paper, it will be 
seen, that the greater part comparatively soon disappears, whilst 
the cellulose derived from the continually falling dead leaves and 
other parts of plants is also soon destroyed under natural conditions 
either totally or partly. It is also a known fact that the layer of 
humus in the primeval forests has a limited thickness, the decrease 
being just compensated by the increase caused by the falling of 
the leaves. Investigation shows that the cellulose, although chemi- 
cally so stable, is decomposed by micro-organisms. The observations 
by MrrscueriicH '), Poporr ®), VAN TieGHEM *), TAPPEINER *), VAN 


1) Ueber die Zusammensetzung der Wand der Pflanzenzelle, Monatsber. d. Berl. 
Akad., 1850, p. 102. 

2) Ueber Sumpfgasgiihrung, Archiv. f. ges. Physiol., 1875, Bd. 10, 5. 118. 

3) Sur le bacillus amylobacter et son rôle dans la putréfaction des tissus végétaux, 
C. R. t. 88, 1879, p. 88. — Identité du bacillus amylobacter et du vibrion buty- 
rique de M. Pasteur, CG. R. t. 89, 1879, p. 5. 

4) Ueber Celluloseverdauung, Ber. d. d. ch. G. Bd. 15, 1882, S. 999. — Ueber 
Cellulosegihrungen, Ber. d. d. ch. G. Bd. 16, 1883, S, 1734. — Ueber die Sumpf- 
gasgihrung im Schlamme der Teiche, Sümpfe u. Kloaken, Ber. d. d. ch. G. Bd, 
16, 1883, S. 1740. 


( 686 ) 


Spnvs') and particularly those of Hopper Sryier*) and of OMELIANSKI*) 
proved, that cellulose may be broken up by anaérobic bacteria, with 
production of methane and carbon dioxide, or hydrogen and carbon 
dioxide and simultaneous formation of acetic and butyric acids. In 
this communication it will be shown that cellulose may also be 
rendered soluble by aërobie bacteria. In the first place it was proved, 
that this substance may serve as a source of carbon for denitrifying 
bacteria and may, therefore, be made to disappear with great rapidity 
in the presence of nitrates. But it could also be shown that cellulose 
is fit as a carbonfood for common aérobic bacteria and although the 
solution then takes place slowly, there can be no doubt about the 
decomposition. The products derived from the cellulose play an 
important role in the nutrition of other microbes particularly the 
spirillae, so that an elegant accumulation experiment may be based 
on the use of cellulose as a source of carbon. 

Although the destruction of cellulose by anaërobie or aérobie 
bacteria requires a faintly alkaline medium, it may, with sufficient 
aëration, also be acted on in a faintly acid surrounding by various 
moulds and mycelia of higher fungi. This was first demonstrated in 
1886 by pr Bary for the genus Peziza and the same was shown 
by later observers for other moulds, whilst the destruction always 
appeared to be due to the action of an enzyme. Here we will prove 
that the power possessed by moulds to attack cellulose is not confined to 
certain species only, as one might imagine from the existing literature, 
but that a great number of the species of this group share that property. 

Finally, I wish to observe that I will occupy myself exclusively 
with the destruction of pure cellulose and not with that of lignified 
and corky ecell-walls, where in the first place higher fungi are at 
work, as is shown by the researches of R. Harrie *). 

1. The decomposition of cellulose by denitrifying bacteria. 

Meeser *) states in 1871 that in the presence of cellulose bacteria 


1) Bijdrage tot de kennis der cellulosegisting. Dissertation, Leonards, at Leiden, 
1890, (this contains a very complete literary review). 

2) Ueber die Gährung der Cellulose mit Bildung von Methan u. Kohlensäure, 
Zeitschr. f. Phys. Ch. Bd. 10, 1886, S. 401. 

3) Sur la fermentation de la cellulose, CG. R. t. 121, 1895, p. 653. — Sur un 
ferment de la cellulose, CG. R. t. 125, 1897, p. 970. — Sur la fermentation cellu- 
losique, C. R. t. 125, 1897, p. 1131, — Ueber die Gährung der Cellulose, Centrbl. 
f. Bakt. Abt. II, Bd. 8, 1902, S. 193. 

*) Die Zersetzungserscheinungen des Holzes, Berlin 1878. 

5) De la putréfaction produite par les bactéries en présence des nitrates alcalins 
C. R. t. 81, 1876, p. 533. Nitritbildung durch Bacterien, Ber. d. d. cb. G. Bd. 8, 1875, 5. 
1214, 


4 


( 687 ) 


reduce nitrates to nitrites; he has, therefore, proved denitrification, in 
the largest sense of the word, as being possible with cellulose, but from 
his short notes we do not understand his modus operandi or the nature 
of the cellulose used in the experiments. DEn#ratn') positively states in 
1897 that he has not been able to observe denitrification with flax 
fibres and the attention of OMELIANSKL (l.e.) has also not been attracted 
to this process when engaged in the study of the fermentations of 
cellulose. This investigator induces the methane or hydrogen fermen- 
tation by means of a nitrogenous food composed of ammonium sul- 
phate or phosphate and sometimes he also adds asparagine, peptone, 
extract of meat or of manure. Strange to say, he has not worked 
with nitrates; had he done so, he would have noticed that the nature 
of the process is completely modified, for instead of the methane or 
hydrogen fermentation denitrification sets in which is characterised 
by the production of free nitrogen and carbon dioxide. 

In a previous research *) on accumulation experiments with deni- 
trifying bacteria, I have shown that these aérobic organisms can 
oxidise many different organic substances out of contact with air 
with the aid of nitrates or nitrites, according to the formulae: 

5C+4K NO, +2H,O —=4K HCO, +2N,+ CO, 
3C+4K NO, + H,O = 2K HCO, + K, CO, + 2N,. 

Denitrification was noticed with lactates, tartrates, citrates, malates, 
acetates, glucose, starch, asparagine, gelatin, broth, methyl and 
ethyl alcohol and it was, therefore, thought worth while to try 
whether cellulose might also be used as a source of carbon supply 
in the denitrificationprocess, which indeed proved to be the case. 

Before describing my experiments in detail, I will first make some 
remarks as to the nature of the cellulose employed. Asa rule Swedish 
filterpaper was taken. Although this paper gives a faint blue colour 
with a dilute solution of iodine it was found to be very difficult to 
remove the impurity with boiling water; the so-called starch-free 
paper from ScHrricHER and Scrürr, which has been purified with 
hydrofluoric acid, showed the same reaction. Sometimes linen tissues 
and cottonwool were used, from which the first also gives a blue 
coloration with dilute solutions of iodine, whilst the latter does not 
show this reaction. The little impurities, present in the cellulose 
employed, were however, of no moment in my experiments, as 
the effect on the cell walls was judged by the changes observed 
by a microscopical investigation. 

1) Recherches sur Ja réduction des nitrates, Ann. agron. t. 23, 1897. 

2) Van Irerson, Accumulation experiments with denitrifying bacteria. Proc. Acad. of 
Science, Amsterdam July 1902. 


I obtained the best results with a paper pulp prepared by triturating 
Swedish filterpaper in water, care being taken that this pulp contained 
2°/, of cellulose. 

In order to obtain a thorough denitrification with cellulose, a 
bottle holding about 200 ce. is filled with the following mixture: 


Tapwater ') 100, paper 2, KNO, 0,25, K,HPO, 0,05, 


and the mixture is then inoculated with a few ec. of mud (from a diteh). 

The bottle is then quite filled up in the manner described in 
my former communication (Le), to prevent access of air, and the 
cultivation takes place at 35°, 

After the lapse of about 8 days the action is perceptible, but only 
after 12 days a brisk fermentation sets in. The cellulose is carried 
to the top by the generated gasbubbles and a quantity of liquid is 
forced out of the bottle by the slimy froth, while the paper-pulp is kept 
back by the stopper. In the beginning of the process a strong formation 
of nitrite may be observed, but the nitrates and nitrites soon decrease 
and after the lapse of about 15 days, these compounds have disappeared. 
The liquid is now carefully decanted from the pulp, which may be 
done without appreciable loss of paper fibres, as these readily agglo- 
merate. The bottle is then refilled with the following liquid: 

Tapwater 100, KNO, 0,25, K,HPO, 0,05. 

The process now starts much quicker than in the first cultivation, 
the nitrate disappears in + or 5 days and by repeating the operation 
a few times more, cultures may be obtained of an increasingly active 
denitrifying power, with which it is possible to completely reduce in 
one or two days 0.5 gram of KNO, dissolved in 200 ec. of water. 
This method of working is preferable to adding a fresh quantity of 
KNO, to the original culture, as it is then not possible to reduce 
on the whole more than about */, °/, of KNO, (calculated in regard 
to the quantity of the liquid used, or 25 °/, in regard to the cellulose) 
because the process then comes to a standstill by the alkaline potas- 
sium carbonate formed from the nitrate. 

If now a sterilised liquid is inoculated with the strongly denitrifying 
rough culture and the cultivation allowed to take place under the same 
circumstances as described above, the action commences much more 
rapidiy than in the first preliminary experiment, whilst the same 
phenomena occur. Even after repeating the inoculation ten times, 
no change in the intensity of the process could be observed. 

Not only paper, but raw flax fibres, cottonwool and linen appeared 


1) From the Downs at Loosduinen. 


u 
Eo aes sail 


—_— dik se ha il aen dee a 


( 689 ) 


capable of inducing denitrification, the cottonwool, however, being 
attacked with great difficulty. No denitrification could be observed 
with sawdust or turf, whilst Van Servus (Le. pg. 104) has also been 
unable to observe decomposition of wood-cellulose by real anaerobie 
bacteria. This extraordinary difficult decomposition of wood-cellulose 
out of contact with the air, is, according to this investigator, perhaps 
the key to the explanation of the formation of humine substances, 
peat, browncoal and coal. 

The distribution of the microbes, engaged in the denitrification of 
cellulose, in the mud from canals, seems to be a very general one, 
as each sample employed contained these germs. Although they 
are also very generally distributed in the earth, their number per 
cc. appears therein to be less, for, on using earth as infecting material, 
the action was delayed. Even in sea water, taken from the port of 
den Helder, were always microbes found, which in the presence ot 
cellulose could induce denitrification ; in how far these forms are similar 
to the terrestrial ones has not yet been ascertained, but I wish to 
call particular attention to the fact, that, at least near the shore, 
cellulose may disappear by denitrification. 

The changes, which cellulose undergoes during this process, 
are visible to some extent with the naked eye: the white fibres 
soon turn orange and the pulp acquires a viscous consistency. 
Microscopically, it appears, that already very soon after inoculation 
some of the fibres are inclosed in a bacterial mucus and after 
a prolonged culture this is the case with nearly all the fibres. 
At first, the whole of the fibre is still very plainly visible within 
this mucus, but gradually, on account of the decomposition, it 
completely disintegrates into loose fibrillae and at last we only 
find a few particles of cellulose left, or the fibre disappears altogether 
(fig. 1). This destruction of the cellulose becomes very pronounced, 
when instead of paper-pulp strips of filterpaper are used. By 
repeatedly adding fresh nitrate we then finally obtain bacteria-mem- 
branes, which still have the exact shape of the strips of paper but 
in which we only meet isolated fibres disintegrated into fibrillae 
or even still more decomposed. As is already stated, the woody 
substance is not attacked by denitrifying bacteria, the few annulated, 
spiral and pitted vessels, which are contained as impurities in the 
filterpaper, are found unaltered in this mucus. Fig. 2 shows the 
form of two very strongly dissolved paperfibres (a) and some 
non-attacked woody elements (3, y and d), which are still found in 
such preparations. 

The gases, liberated during the denitrification of cellulose and of 


( 690 ) 


which some litres were collected, consist exclusively of free nitrogen 
and carbon dioxide; no trace of hydrogen, methane or nitrous 
oxide (N,O) was found. 

As regards the micro-organisms which take part in this process, 
a microscopical examination of the said bacterial mucus, which consists 
of a finely granulated substance, shows the presence of very small 
rod-like bacteria (fig. 1) and further there are found in the cultures 
infusoria, amoebae, monads, spirillae, other small bacteria and vibrionae; 
larger rod-bacteria or spore-forming organisms were not detected. 
That the bacteria, involved in the process, are no spore forming 
organisms, was also shown by the fact, that no pasteurised material 
of whatever origin (mud from a ditch or from the soil) can cause 
denitrification in the presence of cellulose. 

Many experiments have been made with the object of isolating 
the bacteria taking part in the denitrification, but always with a 
negative result. By inoculation on meat-gelatin and cultivating at 
24°, I several times obtained pure cultures of Bacillus stutzeri: Nev. 
and LenM., which bacterium was also found in large numbers in 
those cases where other denitrifying bacteria were present, so that 
denitrification with cellulose is a new accumulation experiment for this 
important species, which, however, does not attack the cellulose itself. 

On using meat-agar or one of the following culture liquids: 


Tapwater 100, agar 2, sodium lactate 2, KNO, 0,05, K,HPO, 0,05, 
Tapwater 100, agar 2, glucose 2, KNO, 0,05, K,HPO: 0058 


and cultivating at 35°, other bacteria besides B. stutzeri were found 
and these were nearly always denitrifying ones. Very often a mucous 
colony of a motionless, non-spore forming demtrifying bacterium 
became conspicuous, while in other cases a small, slightly denitrifying 
spirillum may be isolated. No permanent denitrification with paper 
could, however, be obtained with any of these forms or with any 
combination thereof, even the erude mixture as it is formed on the 
plates was not capable to do this. The fact, that these bacteria may 
cause a temporary faint evolution of gas (which, at first, made me 
suspect, that the destruction of cellulose could be accomplished by 
ordinary denitrifying bacteria) must be attributed to the presence of 
small quantities of impurities in the cellulose. Stil, I think we may 
take it for granted, that we are dealing here not with an anaérobic 
but with an aérobic bacterium, first of all, because all known denitri- 
fying bacteria are aérobie and only behave anaérobically in the presence 
of saltpetre, secondly because methylene-blue is not reduced, when 
added to a medium in which cellulose is denitrifying, whilst in 


( 691 ) 


cultures of the know anaérobic bacteria this compound is always 
decolorised. We therefore come to the conclusion, that the bacterium, 
Which causes the denitrification of cellulose, does not grow on the 
used nutrient media, or else, growing there, loses immediately its 
denitrifving properties. 

If now we compare the hydrogen and methane fermentations with 
the denitrifying process we find the following points of difference. 


Is. In the hydrogen or methane fermentation the liberated gaseous 
products are carbon dioxide and hydrogen, or carbon dioxide and 
methane. 


2d, To those fermentations chalk must be added to neutralise 
the formed butyric and acetic acids, whilst in our case the saltpetre 
yields potassium carbonate and no volatile acids can be detected. 


3d, Those processes take place in a medium wherein sulphates can 
be reduced to H,S and therefore methylene-blue is decolorised. In my 
experiments such a reduction of sulphates is quite out of the question 
as long as traces of nitrates and nitrites are still present. 


4. The methane and hydrogen fermentation are caused by 
comparatively large, well characterised spore forming organisms, our 
denitrification by very small bacteria, forming no spores. 

The velocity with which cellulose disappears during the denitri- 
fication is about the same as in the methane or hydrogen fermenta- 
tion of this substance. In a volume of 500 ¢.c., I succeeded in 
completely dissolving 8 grams of cellulose all but a few fibres, by 
means of 36 grams of KNO,, in a month’s time. The quantity of 
KNO, theoretically required amounts to only 24 grams, but in my 
experiments a portion of the nitrate was lost in the expelled liquid 
and, therefore, more nitrate was required. By means of the hydrogen 
fermentation, OMELIANSKI succeeded in dissolving 41.6 grams of cellulose 
contained in a volume of 3 litres in 3*/, months, and about 12 grams 
in a volume of 1 litre in 5 months, which velocities agree with the 
values found by me for the denitrification. 

Notwithstanding the possibility of denitrification of saltpetre under 
the influence of cellulose, in the presence of this substance nitrification 
of ammonium salts and nitrites can proceed without interruption. 
This has already been shown by OmELIANski'), who cultivated the 
nitrite ferment on paper. We also observed nitrification of ammonium 
salts and nitrites, when a very small quantity of cellulose (about 


*) Kleinere Mitteilungen über Nitrifikationsmikroben [, Centrbl. f. Bakt. Abt. II, 
Bd. 8, 1902, S. 785. 
47 


Proceedings Royal Acad. Amsterdam. Vol V. 


(692 5 


0,05 °/,) was introduced into a thin layer of one of the following 
eulture liquids, which were inoculated with earth: 

Tapwater 100, NH,Cl 0,05, K,HPO, 0,05, 
~~! * » KNO, 0,05, N 0,05, 

In my previous communication | have already pointed out, that 
nitrification and denitrification may take place together in garden 
soil and that the aération decides, which of these processes will be 
the predominant one; the same conclusion may, therefore, now be 
drawn for cellulose as a nutrient material. A closer examination 
however shows, that the two processes cannot occur simulta- 
neously in the same particle, but that a localisation must take place, 
in this way, that strong aëration is necessary in the particles where 
nitrification sets in, whilst the exclusion of air is necessary for the 
denitrification process. 

As has already been previously observed formation of nitrite 
takes place in the first stage of the denitrification process in the 
presence of cellulose and as this substance by no means prevents the 
oxidation of the nitrite to nitrate, these two processes, occurring simul- 
taneously, may cause the steady disappearance of cellulose. 

We therefore see, that these same processes may cause the disap- 
pearance of cellulose in soil and in waters, which plainly shows their 
great importance in the ““self-purification ”, as also in the biological 
purification of sewage. 


Di. The aerobic decomposition of cellulose hy hacteria. 


In order to demonstrate denitrification in the presence of cellulose 
in the manner described above, a very small quantity of this sub- 
stance (about 0,05°/,) only must be present, for on using more 
say, 2°/, the nature of the process is completely changed. This must 
be attributed to a strong decomposition of the cellulose by aérobie 
bacteria, which then takes place and which produces a large quantity 
of soluble organic matter, rendering the nitrification impossible. This 
last phenomenon may be best observed when use is made of the 
following culture medium : 

Tapwater 100, paper 2, NH,CI 0,1, K,HPO, 0,05, chalk 2. 

Instead of NH,Cl we may also add KNO, (0,1), KNO, (0,1), peptone 
(O,1) or an unlimited quantity of MgNH,PO,. The cultivation takes 
place at 28—35° in ERLENMEIER flasks in a layer from 0,5—J cm. 
in thickness, thus, under very aérobic conditions, so that on using 
KNO, or KNO,, no denitrification can be expected, at least not at 
the commencement. 


Par Te 


( 693 ) 


If mud from a ditch is used as infecting material a decided growth 
is already noticed after 5 or6 days, the cellulose turns to an orange 
colour and may even disintegrate to a thin paste after 3 or 4 weeks. 
Microseopically, we see, that we obtain besides the cellulose-dissol- 
ving bacteria a very rich accumulation of spirillae, which however 
do not themselves attack cellulose. I have often repeated these 
experiments and always with the same result: the cultures become 
extremely rich in spirillae and these consist of many varieties. 
As a rule different species were found in a same culture, large 
spirillae with several windings in company with small, very mobile 
ones, but sometimes it also happened, that it looked under the 
microscope, as if we were dealing with pure cultures of special 
spirillae. These different results being no doubt connected with the 
nature of the germs in the infecting materials employed. Often 
however, we meet besides the spirillae, infusoria, monads, amoebae 
and small forms of bacteria, sometimes also rod bacteria and spore 
forming organisms, but the spirillae are always in the majority. 

If such cultures are transported into the same sterile medium, 
the chief character remains the same, but the growth takes place 
more rapidly and as a rule the mumber of species of spirillae is much 
reduced, so that frequently but a single one remains. Here it is perhaps 
the proper place to state, that an accumulation of spirillae may also 
be obtained in using a nutrient liquid composed as follows: 


Tapwater 100, calcium lactate 2, peptone 0,05, K,HPO, 0,05, 


which is infected with a small quantity of diteh-mud. 


At temperatures from 28—37° exceedingly rich spirillae cultures 
are formed in this liquid. It would, however, be too rash thence to 
conclude, that lactate is formed as a transient decomposition product 
of the cellulose. j 

The destruction of the cellulose is not only apparent from the strong 
growth of microbes, but also from a microscopical examination of the 
fibres. As in the case of the denitrification process, these are here also 
found to be enveloped with a bacterial mucus in which is always found 
a very small rod-bacterium, and occasionally a large micrococcus, which 
itself does not attack cellulose, but much accelerates its dissolution by 
the small bacterium. The destruction is no doubt caused by the latter, 
for sometimes, we have obtained cultures, which exclusively contained 
this species only. | 

That the decomposition is here an aërobie one, is shown by the 
fact, that it Commences at the surface of the culture and also takes 
place equally well when we cultivate in a very thin layer. 


47% 


( 694 ) 


Owing to the dissolution of the cellulose the absorption of oxvgen 
in the cultures may become so strong, particularly when working 
with thick layers of cellulose paste, that anaërobie processes become 
possible. If, now, nitrates or nitrites ave still present in the culture 
denitrification will set in, but if these compounds are already decom- 
posed, or if originally another source of nitrogen had been added, 
methane or hydrogen fermentation becomes possible. In the last case 
Wwe microscopically observe the very characteristic rods with spores, 
accumulating on the fibres. In this anaérobic stadium the spirillae 
are for the greater part expelled but the destruction is now much 
more intense than when it took place exclusively under aérobiec 
conditions so that in a short time the paper pulp gets for the greater 
part dissolved and leaves behind a bacterial mucus. 

When using as infecting material soil, instead of mud from a 
ditch, we observe on the whole the same phenomena, only we 
do not find then that variety in species of spirillae noticed with 
ditch-water. As a rule a short, thick, granulated spirillum with one 
half winding is then conspicuous and 1 have succeeded in preparing 
pure cultures of this species, already observed previously *). 

An experiment with sea water showed, that this also causes the 
aerobic decomposition of cellulose and an accumulation of different 
species of spirillae was obtained at the same time. In this case the decom- 
position in the anaërobie stadium may also be caused by an anaérobie 
spore forming organism, which much resembles the bacteria of the 
methane and hydrogen fermentations but still presents a different shape. 

| have tried to isolate the bacteria connected with the aérobic 
destruction but was not more successful than in the denitrification 


experiment. On sowing on broth-gelatin or broth-agar a number of 


bacteria species were found: jluorescents, B. coli commune, B. sub- 
lis, B. mesentericus and several others unknown to me, but none 
of these species or none combination thereof was capable of attacking 
cellulose. 

Our result that cellulose may be attacked by aërobie bacteria 
widely occurring in nature, is confirmed in a particularly convincing 
manner by the following experiment : 

In a glass box are placed two dises of Swedish filterpaper between 
Which has been sprinkled a little quantity of powdered MeNH,PO, ; the 


paper is imbibed with a solution of 0.05 gram of K,HPO, in 100 ce. of 


tapwater. If now we introduce upon the plate thus prepared a little 


') Beterinck. Ueber oligonitrophile Microben. Centrbl. f. Bakt. Abt. IL, 1901 
Bd. 7, S. 574, 


( 695: ) 


quantity of water containing in suspension humus, garden soil or, still 
better, diteh-mud, and if we cultivate at 24—28", the paper gets covered 
after 4 or 5 days with vellowish-brown spots which, microscopically, 
are found to consist of bacteria. These spots spread with great rapidity, 
and it is highly interesting to observe how in a short time the white 
ilterpaper is covered with the rusty culture. This is accompanied by 
a decided decomposition of the paper fibre, which is shown in the 
first place by the fact that the paper becomes quite soft and pulpy 


just on the spots exposed to the action of the brown bacterium, losing 


there all coherence and sinking down along the edges of the phos- 
phate. The phenomenon becomes still more pronounced, when instead 
of filterpaper, linen or cotton is used; after about 10 days, the affee- 
ted spots of the originally strong material have lost all power of 
resistance and after 15 days large holes will be formed when carc- 
fully pouring water on them. 

Microscopically, it appears that a powerful destruction of the fibre 
is taking place (fig. 3) due to the action of a brown, very mobile, 
little rod bacterium (Bacillus ferrugineus fig. 4. The fibre is again 
enveloped by a mucus in which is found, in many cases, the 
same micrococcus as mentioned above (fig. 5 and 6). Owing to the 
combined action of these two bacteria the fibre may disappear com- 
pletely and leave behind a mucus containing only microcoeci; we then 
obtain an image as shown in fig. 7. In addition to amoebae and 
monads other small bacteria are found, but there is no question of 
the presence of anaérobics, which occur in the hydrogen or methane 
fermentations, the action being a purely aërobie one and taking 
place very well in filterpaper both sides of which are exposed to 
the air. 

On transferring the brown spots to previously sterilised paper dises, 
between which MgNH,PO, has been sprinkled and which have been 
saturated with a sterile 0,05°/, solution of K,HPO,, the phenomenon 
remams constant. On inocculating them into the above deseribed cel- 
lulose pulp a culture is obtained resembling that which arises by 
the direct action of diteh-mud or earth, but no spirallae are found 
this time, for these being microaerophilous cannot grow in the 
aërobie culture on the paper dises. On the other hand the cultures 
from paper pulp were occasionally capable of producing brown spots 
on paper dises, showing that in both cases the destruction of the 
cellulose may be caused by the same microbe. I also noticed a few 
times that the dises were covered with colorless spots caused by a 
larger mucus-secreting rod, and as moreover the paper pulp cultures 
often are only little colored, it must be assumed, that the aérobie 


( 696 ) 


decomposition of cellulose may be caused by two microbes at least, but 
amone these the brown pigment bacterium is the most conspicuous. 

On using sea water as infecting material, similar brown spots were 
observed. When these were transferred to paper without addition 
of 3°/, NaCl they caused no destruction, which shows that we are 
dealing here with a sperifie sea bacterium. 

I have made several experiments with various culture materials 
in order to isolate this very interesting cellulose-destroying brown 
pigment bacterium, which | was particularly anxious to accomplish 
after having observed, that the crude bacteria-mixture as grown on 
different culture media often again produces spots when spread 
over paper, which shows that on these media the said bacterium had 
kept alive. But I was again unsuccessful in isolating a species which 
either alone or in combination with other bacteria was capable of 
causing the brown spots on paper. Though I succeeded in isolating 
from these spots a brown and a yellow bacterium, which as a rule, 
were present in large numbers, yet, as in the case of the denitrifica- 
tion process, no destruction of cellulose could be induced by their pure 
cultures. The explanation of this circumstance has not yet been found. 

The aérobie destruction of pure cellulose and also the more 
difficult destruction of the lignified cell walls, *) on which we cannot 
enter in this investigation, must, like the denitrification (which is only 
possible with non lignified cellulose and takes place out of contact 
with air) play an important part in the disappearance of vegetable 
substances in nature. The well known fact that wooden piles, when 
partly immersed in water are attacked exactly at the place of contact 
between the water and the air, the breaking of ropes, when suspended 
in water, exactly at its surface and also the aërobie decay of wood 
must be attributed mainly to the action of aërobie destroyers. VAN 
Senus (le. 108) who was acquainted with these facts, did not deny 
the possibility of a decomposition by aérobic bacteria but thought 
it very unlikely “as no phenomenon ever pointed to such a fact.” 

That the above-described yellowish-brown pigment bacterium plays 
indeed an important part in the disappearance of the cellulose, is 
shown by the following experiment. 

On October 14, 1902 were buried in the garden of the bacteriolo- 
vical laboratory at about 15 ¢.m. below the surface a linen cloth 
with a red colored border, and in two other places four sheets of 
filterpaper, all in’ a horizontal position. Left in the soil untouched 
during the recent winter and on exhuming them March 22, 1903 

1 The great stability of wood-cellulose towards microbie life is directly opposed 
to the ready decomposition of wood paper under chemical influences, 


CORA) 


not a trace could be found of the filterpaper, whilst the linen cloth 
had become soft and pulpy, had lost all coherence and could only 
he removed from the soil in pieces; the red border, however, had 
retained its original structure. The originally white tissue had 
assumed the same yellowish-brown colour so familiar to me from 
the cultures on the paper dises, while on microscopical ivesti- 
gation the fibres appeared to be much decomposed and disinte- 
erated into fibrillae and besides moulds and amoebae only small bac- 
teria were observed. On putting some of the well-cleaned fibres 
on the paper dises prepared as described above, [ obtained after three 
days the rapidly spreading, yellowish-brown spots of the destructive, 
small, rod-shaped pigment bacterium. A cellulose-destroying mould, 
Myeoyone puccinioïdes, also could be isolated from the linen, but the fact 
that the yellowish-brown pigment bacterium was here predominant, 
could not be doubted. 


3. The decomposition of cellulose by moulds. 


The fact that cellulose may be attacked by certain fungi has been 
first stated by pr Bary’) for Peziza sclerotium, and the same was 
found by Kissing ©) and by Marswant Warp *) for a kind of Botrytis, 
by BrureNs®) for Pseudodematophora, Botrytis vulgaris, Cladosporium 
herbarum and Aspergillus glaucus. This last investigator did not notice 
any decomposition by JMucor stolonifer, Penicillium glaucum and 
Penicillium luteum. KouNstamM *) prepared a cellulose-destroying enzyme 
from Merulius lacrymans the common wood fungus. Went") has 
shown, that Monilia sitophila, the “ontjom” mould from Java, is capa- 
bie of digesting cellulose and Koning’) has found that one of the 


1) Ueber einige Sklerotien u. Sklerotienkrankheiten, Bot. Zeit. 1886, S. 377. 

*) Zur Biologie der Botrytis cinerea, Diss. Dresden, 1889. 

5) A lily disease, Annals of Botany, Vol. IL, 1888/89, p. 346. 

4) Troekene u. nasse Fäule des Tabaks. Der ,Dachbrand”, Zeitschr. f. Planzenkr. 


3d. HL, 1893, p. SL. — Untersuch. über den Würzelschimmel der Reben, Centr.bl. 
f. Bakt., Abt. If, Bd. 3, 1897, S. 584. — Beitrage zur Kenntniss der Obstfäulnis, 
Gentrbl. f. Bakt. Abt. If, Bd. 4, 1898, S. 514. — Unters. über die Gewinn. der 


Hanffaser durch natürl. Röstmethoden, Gentrbl. f. Bakt. Abt. 11, Bd. 8, 1902, S. 114, 
5) Amylolytische, glucosidspaltende, proteolytische u. cellulose lösende Wermente 
in holazbewohnenden Pilzen. Beihefte z. Bot. Gentrbl. Bd. 10, Heft 2, 1901, S. 90. 
6) The influence of feeding on the secretion of enzymae by Monilia sitophila. 


Proce. Jan. 1901. — Ueber den Einflus der Nahrung auf die Enzymbildung durch 
Monilia sitophila (Moxr) Sacc Jahrb. f. wiss. Bot. Bd. 36, Heft 4, 5. 643. 
7) Genootschap ter Bev. v. Natuur- en Heelkunde Amsterdam, 2 series, dl. IV, 


Afd. 5, Zitling 7 Dec. 1901, 


( 698 ) 


most common humus-inhabitants from the forest of Spanderswoude, 
Trichoderma koningit, possesses the same property. 

We have succeeded in finding an experiment by means of whieh 
the cellulose-destroying moulds may be isolated from nature in 
a direct and certain manner. Two sterile discs of Swedish filterpaper 
are placed in a glass box and moistened with the following liquid: 

Tapwater 100, NH,NO, 0,05, KH,PO, 0,05. 


As infecting material earth or humus may be used, but the best 
results are obtained by simply exposing the opened box for about 12 
hours to the open air. If then we cultivate at 24° and take care to keep 
the paper moist, colonies of moulds already become visible after 5 or 
6 days, but it is only after 14 days or three weeks, that we notice 
the enormous richness of these cultures, and then we are surprised 
at the great number of mould species, which make their appearance. 
Many kinds which we seldom or never notice on malt-gelatin are 
found in large numbers on these paper dises. These species certainly 
are also capable of growing on malt-gelatin, but their germs, as 
they occur in nature, apparently find thereon an unfavorable soil. 
Another advantage of the cultivation on paper is that it is particu- 
larly favorable to the formation of perithecia and picnidia, which 
do not readily develop on rich soils ©). 

From these culture experiments it appears that a continuous rain 
of spores from cellulose-destroying moulds falls in the garden as well 
as in the rooms of the bacteriological laboratory. For instance on 
March 11, when the weather was dry whilst the earth was moist, 152 
cellulose-destroying moulds were collected on a plate of 275 ¢.m. square, 
after this had been exposed for 12 hours to the open air, and among these 
moulds about 85 species were recognised. As these germs must con- 
tinually drop on the soil, it might be expected that the latter would 
be remarkably rich in living moulds and it appeared from experi- 
ments. that this is really the ease at the surface of the garden soil, 
but in a much less degree than might have been expected, while 
lower down in the soil the number of moulds seems to be still less. 
Krom this it follows that most of the spores, which fall on the earth 
rapidly die oft. 

In order to prepare a pure culture of the fungi isolated by the 
““paper-experüment”” some material from the raw cultures was trans- 
ferred to malt-gelatin, where it appeared that the moulds were 
generally much contaminated with bacteria, from which however, 

') Compare Morrrarp, Role des bactéries dans la production des périlhèces des 
Ascobolus, G. R. t. 136, 1903, p. 899. 


( 699 ) 


they could be freed by another inoculation. These bacteria are sapro- 
phytes which do not attack cellulose but grow at the expense of the 
products generated by the action of the moulds on cellulose. This 
result was not unexpected for, as stated in the preceding paragraph, 
the cellulose-destroying bacteria live in a faintly alkaline medium, 
whilst in the ease of moulds the reaction is acid, owing to the presence 
of KH, PO,. In order to be perfectly certain of the pureness of the 
moulds, cultures from the spores were finally made on malt-gelatin. 
The following species, which were detected in these cultures, have 
been submitted to a closer examination : 
1. Sordaria humicola Ovp. 
2. Pyronema confluens Tvr. 
3. Chaetomium kunzeanum Zoer. 
4. Pyrenochaeta humicola Ovp. 
5. Chaetomella horrida Ovp. 
6. Trichocladium asperum Harz. 
Stachybotrys alternans Ovn. 
8. Sporotrichuin bombycinum (Corda) Ras. 
9, F roseolum Ovp. en Bruner. 
10. ie griseolum Ov. 
11. Botrytis vulgaris Fr. 
12. Mycogone puceinioides (Preuss) Sacc. 
13. Stemphylium macrosporoidenm (B. en Br.) Sacc. 
14. Cladosporium herbarum (Purs.) Link. 
15. Kpicocenm purpurascens. KMRENB. 


In the determination of these species, of which Nes. 9) and 4, 
are new, we have been kindly assisted by Prof. Dr. C. A. J. A. 
OupEMANS, to whom we have to express our thanks. 

In order to form an opinion on the destruction of cellulose by the 
isolated species, and also to study their fructification, pure cultures 
were inoculated on paper discs, which after sterilisation, were drenched 
with the above-named solution. Instead of merely placing the spores 
on the paper, it was found desirable to push them in it by means of 
a platinum wire and then to reduce the spots there to pulp. The culti- 
vation is made at 24°, care being taken to keep the paper moist, for 
which it was found advantageous not to use water only but the said 
liquid, as the nitrogen in particular is rapidly used up. The above-named 
moulds all grow over the paper dises, form their fructification-organs 
in avery characteristic manner and often produce intensively colored, 
brown, black and red pigments, which are absorbed by the paper 


1) Nederl, Kruidkundig Archief, Januari, 1905, 


( 1008) 


fibre. Interesting are the cultures obtained in this way of Chaetomium 
kunzeanum, Which sometimes produces a carmine-red pigment and 
which forms dark red peritheciae, the asei of which contain eight grey 
spores; those of Chaetomella horrida, which forms delicate black hairy 
pyenidiae, and particularly those of Pyrenochaeta humicola, which 
produces an intense black pigment, stable towards acids and alkalis, 
and which communicates a dark colour to the fibres, quite resembling 
the humus coloring matters. This latter species however, grew more 
readily on an alkaline medium, so that we prefered in this case the 
said drenched paper dises, between which Mg NH, PO, had been sprin- 
kled. An interesting culture is also that of Sordaria humicola, as 
this ascomycete is only then capable of forming perithecia on paper 
dises, when these give no longer any reaction on ammonia or nitrates. 
Besides the above-named species, a luxurious growth was obtained 
of Trichocladium asperum, Mycogone puccinioïdes and Stemphylian 
macrosporoïdeum, Which three species exhibit great similarity both 
in their morphological and physiological properties. /picoceum pur- 
purascens also grew strongly on the paper and formed a purple- 
red pigment. This species I met several times in the air and also 
(in company with Cladosporium herbarum) on half decayed leaves 
of Populus balsimifera. 

Cultures of these moulds were not only made on paper dises, but 
also on cellulose in ERrLENMEYER flasks, into which was introduced a 
thin layer of the following culture liquid: 


Tapwater 100, paper-pulp 2, NH, NO, 0,05, KH, PO, 0,05. 


In this case a repeated addition of NH, NO, proved very advant- 
ageous. On the pulp the cellulose-destroyers grow still better than 
on the paper dises and in 3 or 4 days the cellulose is converted 
by the mycelium into a coherent mass. Afterwards, the fructification 
organs appear, and with Botrytis rulygars even formation of sclerotia 
was observed. 

The destruction of the cellulose may be regarded as certain when 
strong growth on the paper dises and on the paper pulp are being 
observed. The impurities contained in the paper may also cause 
a slight growth of moulds which do not attack cellulose, but 
these soon cease to develop. The decomposition may be seen 
very clearly by a microscopic examination of the cultures on -filter- 
paper, when these have stood a long time. It will then strike us 
how a large number of fibres have suffered a process of dissolution; 
sometimes pores are formed perpendicularly to the direction of the 
fibre, sometimes the fibres have disintegrated into fibrillae. Fig. 9 


ZON 


of our illustration shows the image of the destruction by Mycogone 
puccinoides, in which the structure of the fibrillae and the said pores 
are visible. 

The degree of destruction also may be ascertained by direct weighing. 
A culture with Mycogone pucemioides was made on a double dise 
of filterpaper, two equally heavy filters serving as control. After 
a culture, lasting 40 days, the dises, from which the strongly 
developed mycelium was not removed, weighed 1.00 gram, whilst 


the controlling dises weighed 1.16 gram, showing that about 14°/, of 


0 
the cellulose had disappeared. A similar experiment with 7richo- 


cladtum asperun gave a loss of 9°/,. These great losses only can 
be explained by the oxidation of the products derived from the 
cellulose under the influence of the respiration process. The oxidation 
of cellulose also was studied with filterpaper pulp, namely by 
weighing the amount of carbon dioxide, liberated during a culture 
of Chaetomium kunzeanum. In this experiment an oxidation of 
about 4°/, of the cellulose could be noticed after a 28 days culture, 
a quantity large enough to remove all doubt about the destruction 
of the cellulose. 

No, growth or only a very small one, was observed when culti- 


vating the moulds on: 
Tapwater 100, agar 2, NH,NO, 0,05, KH,PO, 0,05, 


but as soon as cellulose was added a strong development set in, 
showing in a surprising manner, that agar is a less nutrient food for 
these moulds than cellulose. The cellulose used in these experiments 
must be very finely divided and was prepared by treating cottonwool 
with concentrated hydrochloric acid, which causes the cotton fibres 
to break up into very small fragments. A preparation, which appeared 
to be still more suitable was prepared as follows: Paper which has 
been converted into soda-cellulose by the action of strong soda-lve, 
is readily soluble in sodium xanthogenate to a light yellow liquid: 
the “viscose” of Cross and Brvan'), which is purified by precipitation 
with alcohol; on adding hydrochloric acid to its aqueous solution 
cellulose is precipitated in a very pure condition. I have to thank 
Mr. pr JONGH SCHEFFER, for a specimen of this preparation, which 
he prepared in the chemical laboratory of the Polytechnie School 
at Delft. 

I found that, when cultivating on this agarcellulose, the growth 
entirely depends on the quantity of the cellulose added: with much 
cellulose a strong erowth was observed. 


) Cross and Bevan, Cellulose, 1895, p. 25. London, Longman Green and Co, 


( 702 ) 


As in the case of the moulds investigated by the above-named 
observers, also the species employed by me showed the presence of 
an enzyme, which dissolves cellulose and to which the name of 
“cellulase” may be given’). If cultures on cellulose pulp were treated 
with chloroform, the liquid, after being freed from chloroform by 
evaporation, appeared capable of reducing FRALING’s copper solution. 
If the culture had been boiled before being treated with chloroform, 
no reduction took place. From these last experiments, which were 
conducted similarly to those of BeHRENS (lc), it appears that the 
moulds only produce the quantity of reducing matter necessary for 
their growth and no more. That the quantity or the nature of the 
enzyme secreted by the moulds differs considerably, is shown by the 
great difference in destructive power, as may be readily observed 
from the growth on the paper dises and from the dissolution of the 
cellulose in the paper-pulp cultures. To the powerful destroyers belong: 
Trichocladium asperum, Miycogone puceinioïdes, Stemphylium MACTO- 
sporoideum, Chaetomella horrida, Botrytis vulgaris, Epicoceum pur- 
perascens. To the moderately strong ones: Chactomimm kunzeanum, 
Stachybotrys alternans, Cladosporimm herbarium, Pyrenochaeta hume- 
cola, Pyronema confluens. To the weak ones: Sordaria humicola, 
Sporotrichum bombycinum, Sp. reseolum, Sp. griseolum and Aspergillus 
niger. No destruction was noticed with Mucor stolonifer, Mucor 


mucedo, Dematiin pulilans and Rizopus oryzed. 


Summary of results. 


|L. Cellulose may be made to dissolve by the action of denitrifying, 
non-sporeforming aërobie bacteria provided there be an (ited supply 
of air. 


2. Although nitrification cannot take place in the presence of a 
somewhat large quantity of soluble organic matter, cellulose does not 
feet this process in case of sufficient aëration. 


3. The combined action of nitrification and denitrification must play 
an important part in the disappearance of cellulose in nature, for 
instance in the self purification of waters and of the soil, as also in the 
biological purification of sewage. 

') This name, already used by Kouystamm (lc.) is preferable to the name cy/ase 
which has been used by Brown and Morris (Journal of Chem, Soe. 57, 1890, 
p. 408) for the cellulose-dissolving enzyme in germinating seeds and should aceord- 
ing to Merscunxikorr (Ann. Inst. Pasteur, 1899, t. 12, p. 737) be given to an 
alexin occurring in normal serum. 


14, A 


LURE MY, 


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PROCEEDINGS ROYAL ACADEMY AMSTERDAM. 


( 708 ) 


4. Cellulose may also be attacked, when there is a full supply of 
air by widely distributed, aérobic, nou-sporeforming bacteria, among 
which a brown pigment bacterium (B. ferrugineus) is predominant. 
The destruction is particularly strong in symbiosis with a vellow 
micrococcus, which itself is inert. 

5. Extraordinarily rich spirillae cultures are formed in nutrient 
liquids in which cellulose is being attacked by aërobie bacteria after 
infection with ditch-mud or garden soil. Probably the distribution of 
the spirillae in nature is mainly governed by cellulose. 


6. The property of moulds to attack cellulose is a very common 
one. The dissolution is due to a specific enzyme to which the name 
of “cellulase” may be given. 

7. One of the causes of the origin of humus coloring matters is 
the formation of pigments from cellulose by bacteria and moulds. 

This investigation has been made in the bacteriological laboratory 
of the Polytechnic School under the guidance of Prof. BEIJERINCK. 


Delft, March 1903. 
EXPLANATION OF THE FIGURES. 


Fig. 1. Fibre of filterpaper with denitrifying bacteria, disintegrated into fibrillae, 
enclosed in mucus. Enlargement 550. 

ig. 2. Debris of filterpaper at the end of the denitrification process, most of 
the fibres are dissolved. z the last debris of cellulose fibres, B, y and 3 nonaltacked 
elements of “woodcellulose”. Knl. 100. 

ig. 3. Fibre of filterpaper with aérobic bacteria disintegrated into fibrillae, 
enclosed in mucus. Enl. 550. 

Fig. 4. Pacterium from the preceding figure more strongly enlarged; arrows 
represent motion. Enl. 1500. 

Fig. 5. Fibre of filterpaper attacked by an aérobic bacterium with sapropliylic 
micrococcus, commencing to disintegrate into fibrillae. Ent. 550. 

Vig. 6. Two fibrillae of the preceding fibre more strongly enlarged, with z aérobic 
destructive bacteria and 3 saprophytic micrococcus. Eni. 1500. 

Wig. 7. End of the destruction in fig. 5 the fibrillae having become invisible; 
micrococci only visible. Ent. 550. 

Fig. 8. Fibre attacked by aérobic bacteria, disintegrating into fibrillae and enclosed 
in a thin mucous layer as medium for a spirillae culture in which 3 species are 
recognisable. Enl. 550. 

Fig. 9. Destruction of a fibre of fillerpaper by Mycogone puccinioides, besides 
the fibrillary structure, cross pores have been formed in the fibrillae owing to the 
action of the cellulase. Enl. 550. 


(May 27, 1903). 


Ss am Sg id gs 


ABSORPTION (On the emission and) by metals of rays of heat of great wavelengths. 666. 

ABSORPTIONBAND (Observations on the magnetic rotation of the plane of polarisation 
in the interior of an). 41. 

— (The caleulation “ from the magnetic rotation of the plane of polarisation for 
substances without an) in the visible spectrum. 413. 

ACCUMULATION experiments with denitrifying bacteria. 148. 

ACETALDEHYDE + paraldehyde (Equilibria of phases in the system:) with and without 
molecular transformation. 283. 

ACID (On the prussie) in the opening buds of Prunus. 31. 

actps (On the so-called compounds of sulphonearboxylic) with sulphuric esters. 482. 

AEROBIC micro-organisms (The decomposition of cellulose by). 685. 

ALBERDA VAN EKENSTEIN (w.) and C. A. Lopry pr Bruyn: “Formaldehyde 
(methylene)- derivatives of sugars and glucosides.” 175. 

ALLoys (The course of the meltingpoint-line of solid) or amalgams. (I). 424. (II). 511. 

AMALGAMS (The course of the meltingpoint-line of solid alloys or). (1). 424. (II). 511. 

AMPHIOXUS LANCEOLATUS (On the structure of the light-perzepting cells in the spinal 
cord, on the neurofibrillae in the ganglioncells and on the innervation of the 
striped muscles in). 350. 

Anatomy. J. W. van Wisnr: “A new method for demonstrating cartilaginous mikro- 
skeletons.” 47. 

ANGLES (On the connection of the planes of position of the) formed by two spaces S, 
passing through a point and incident spacial systems. 53. 

ANTIMONY (On the atomic weight of). 543. 

ARC (The influence of variation of the constant current on the pitch of the singing). 311. 

ARONSTEIN (L.) and A. S. vaN Nierop. On the action of sulphur on toluene 
and xylene. 288, 

Astronomy. E. F. van DE SANDE BAKHUYZEN: “On the yearly periodicity of the rates 
of the standardelock of the Observatory at Leyden, Hohwü No. 17.” (1). 68. 
(LI). 193. 

—- E‚ F. van Dr SANDE BAKHUYZEN: “Preliminary investigation of the rate of the 
standardelock of the Observatory at Leyden, Hohwii N°. 17 after it was mounted 
in the niche of the great pier.” 267. 

— J. Wreper: “On interpolation based on a supposed condition of minimum.” 364. 

ATMOSPHERIC PRESSURE (Measurements on the magnetic rotation of the plane of pola- 


risation in liquefied gases under). 248. 


45 


it CO Not ENS: 


ATOMIC WEIGHT (On the) of Antimony. 543. 
atoms (Intramolecular rearrangement of) in azoxybenzene and its derivatives, 51. 
— (The intramolecular rearrangement of) in halogenacetanilides and its velocity, 
(1). 178. (II). 359. 
AURICLE of the mammalian heart (On the duration of the compensatory pause after 
stimulation of the). 378. 
AZOXYBENZENE (Intramolecular rearrangement of atoms in) ard its derivatives. 51. 


BACTERIA (Accumulation experiments with denitrifying). 148. 
Bacteriology. M. W. Bryerinck and A. van DELDEN: “On a colourless bacterium, 
whose carbon food comes from the atmosphere.” 398. 
BACTERIUM (On a colourless), whose carbon food comes from the atmosphere. 598. 
BAKHUIS ROOZEBOOM (H. W.) presents a paper of Prof. ue, Dusots : “Geolo- 
gical structure of the Hondsrug in Drenthe and the origin of that ridge.” (LD). 101. 
— presents a paper of Dr. W. Rerxpers: /Galvanic cells and the phase rule.” 182, 
— A representation in space of the regions in which the solid phases, which oceur, 
are the components, when not forming compounds. 279. 
— Equilibria of phases in the system : acetaldehyde + paraldehyde with and without 
molecular transformation. 283. 
— Tinamalgams. 373. 
— presents a paper of Dr. A. Smits and L. k. Worrr: “The velocity of trans- 
formation of carbon monoxide.” 417. 
— presents a paper of Mr. J. J. van Laar: “The course of the melting-point-line 
of solid alloys or amalgams.” (L). 424. (ID. 511. 
— presenis a paper of Mr. J. J. van Laan‘: ‘On the potential difference, which 
occurs at the surface of contact of two different non-miscible liquids, in which 
a dissolved electrolyte has distributed itseif” 431. 
BAKHUYZEN (E. F. VAN DE SANDE). See SANDE Baknuyzen (B. F. vaN DE). 
— (H. G. VAN DE SANDE). See SANDE DBAKHUYZEN (H. G. VAN DE). 
BATH of very uniform and constant low temperature in the cryostat. 502. 628. 
— (A permanent) of liquid nitrogen at ordinary and at reduced pressure. 631. 
BEKMAN (BE. H. M.). On the behaviour of disthene and of sillimanite at high 
temperature. 240. 
BELZER (A. H. J.). The velocity of transformation of tribroomphenol bromine into 
tetrabromophenol. 556. 
BEMMELEN (J. M. VAN) presents a paper of Mrs. L. Aronsrern and A. 8, VAN 
Nrerop: “On the action of sulphur on toluene and xylene.” 288. 
BENZIDINE transformation. 577. 
BEYERINCK (M. W.) presents a paper of Mr. G. van Iverson Jr: “Accumulation 
experiments with denitrifying bacteria.” 148. 
— presents a paper of Mr. G. van Iverson Jr: “The decomposition of cellulose 
by aërobie micro-organisms.” 685. 
— and A. VAN DELDEN, On a colourless bacterium, whose carbon food comes from 
the atmosphere. 398. 


CON TEN T Ss. Tit 


BLANKSMA (J, J.). The intramolecular rearrangement in halogenacetanilides and its 
velocity. (L). 178. (II). 359. 

— Nitration of symmetrical dinitroanisol, 650, 

BOEKE (J.). On the structure of the light-percepting cells in the spinal cord, on the 
neurofibrillae in the ganglioncells and on the innervation of the striped museles 
in Amphioxus lanceolatus, 350. 

BOILINGPOINT-CURVE (The) of the system: hydrazine + water. 171. 

BONNEMA (J, H.). Cambrian erratic-blocks at Hemelum in the South-West of Frisia. 140. 

— Some new under-cambrian erratie-bloeks from the Dutch diluvium. 561.' 
— Two new mid-cambrian erratic-blocks from the Dutch diluvium. 652. 

BORNEO (Influence of changed conditions of life on the physical and psychical develop- 
ment of the population of Central-). 525. 

Botany. fi. Verscrarrrrr: “On the prussic acid in the opening buds of Prunus”. 31. 

— J. ©. Scuoure: “Die Steliir-Theorie”. 497. 

BRUIJN (CG. A. LOBRY DE). See Lopry ve Brun (C, A). 

BUCHNER (B. H.). The transformation of diphenyliodonium iodide and chloride and 
its velocity. 646. 

Bubs (On the prussic acid in the opening) of Prunus. 31. 

e 

CALCULATION — (Ihe) from the magnetic rotation of the plane of polarisation for sub- 
stances without an absorptionband in the visible spectrum, 413. 

CARBON FOOD (On a colourless bacterium, whose) comes from the atmosphere, 398. 

CARBON MONOXIDE (The velocity of transformation of). 417. 

CARDINAAL (J.). On the geometrical representation of the motion of variable 
systems. 586, 

CARTILAGINOUS Mikroskeletons (A new method for demonstrating). 47. 

CELIS (On the structure of the light percepting) in the spinal cord, on the neurofi- 
brillae in the gangiioncells and on the innervation of the striped muscles in Amphi- 
oxus lanceolatus. 350. 

CRLLULOSE (The decomposition of) by aérobic micro-organisms. 685, 

Chemistry. I]. M. Knipscuren: “Intramolecular rearrangement of atoms in azoxybenzene 
and its derivatives”. 51. 

— C. A. LoBry pr Bruyn and J. W. Drro: “The boilingpoint-curve of the system : 
hydrazine + water”. 171. 

— C. A. Lopry pr Bruyn and W. ALBERDA VAN EKENSTEIN: “Formaldehyde 
(methylene)-derivatives of sugars and glucosides”. 175. 

— J. J. BLANKsMA: “The intramolecular rearrangement in halogenacetanilides and 
its velocity”. ([). 178. (IL). 359. 

— W. Reivers: “Galvanic cells and the phase rule”. 182. 

— H. W. Bakuuis Roozrnoom: “A representation in space of the regions in which 


the solid phases which occur, are the components, when not forming compounds”. 


279. 


iv Gio NTEN Ts, 


Chemistry. I. W. Bakuurs Roozesoom: “Equilibria of phases in the system: acetaldehyde 
+ paraldehyde with and without molecular transformation”. 283. 
— LL. ARONSTEIN and A. S. van Nierop: “On the action of sulphur on toluene and 
xylene’. 288. 
— H. W. Bakuuis Roozenoom: “Tinamalgams”, 373. 
— J. Porrer van Loon: “Benzidine transformation”. 377. 
— A, Smits and L. K. Worrr: “The velocity of transformation of carbon monoxide”. 


417. 

— J. J. van Laar: “The course of the melting-point-line of solid alloys or amal- 
gams”’. (I). 424. (ID). 511. 

— J. J. van Laar: “On the potential-difference, which occurs at the surface of 
contact of two different non-miscible liquids, in which a dissolved electrolyte has 
distributed itself”. 431. 

— A.P. N. FRANCHIMONT: “On the so-called compounds of salts of sulphoncar- 
boxylie acids with sulphuric esters”. 482. 

— E. Conen and Tu. Srrencers: “On the atomic weight of antimony”. 543. 

— RE. Coen and U. A. Losey DE Bruyn: “The conductive power of hydrazine and 
of substances dissolved therein’. 551. 

— A. H. J. Berzer: “The velocity of transformation of tribroomphenol bromine into 
tetrabromophenol”. 556. 

— C. A. Lory DE Bruyn and C. L. Junerus: “Dissociation in and erystallisation 
from a solid solution”. 643. 

— E.H. Biécuner: “The transformation of diphenyliodonium iodide and chloride 
and its velocity”. 646. 

— J. J. Buanxsma: “Nitration of symmetrical dinitroanisol”. 650. 

cuLORIDE (The transformation of diphenyliodonium iodide and) and its velocity. 646. 
COMEN (E) and Tu. StrencErs. On the atomic weight of Antimony. 543. 

— and C. A. LoBry DE Bruyn. The conductive power of hydrazine and of substances 
dissolved therein. 551. 

COMMON DIVISOR (An analytical expression for the greatest) of two integers. 658. 

COMPENSATORY PAUSE (On the duration of the) after stimulation of the auricle of the 
mammalian heart. 378. 

COMPONENTS (A representation in space of the regions in which the solid phases which 
occur, are the), when not forming compounds. 279. 

COMPOUNDs (On the so-called) of salts of sulphoncarboxylic acids with sulphuric esters. 482, 

CONDITION of minimum (On interpolation based on a supposed). 364. 

CONDUCTIVE POWER (The) of hydrazine and of substances dissolved therein. 551. 

constants (The value of some magneto-optic). 458. 

corona (Peculiarities and changes of FrAuNuHorem-lines interpreted as anomalous 
dispersion of sunlight in the). 589, 

CRITICAL STATE (The equation of state and the g-surface in the immediate neighbour- 


hood of the) for binary mixtures with a small proportion of one of the compo- 
nents. 321. 336, 


© OUN ADS ERIN SP ra Vv 


CRYOGENIC Laboratory (Methods and apparatus used in the). ILL, Bath of very uniform 
and constant low temperatures in the cryostat, 502. 628. A cryostat of modified 
form for apparatus of small dimensions. 628. LV. A permanent bath of liquid nitrogen 
at ordinary and at reduced pressure. 631. V. Arrangement of a BurckHaRrpt-WEIss 
vacuumpump for use in the circulations for low temperatures. 633. 

cryostat (Bath of very uniform and constant low temperatures in the). 502. 628. 

— (A) of modified form for apparatus of small dimensions. 628. 

CRYSTALLISATION (Dissociation in and) from a solid solution, 643, 

CURRENT (The influence of variation of the constant) on the pitch of the singing arc. 311. 

DELDEN (A. VAN) and M. W. Beyertncx. On a colourless bacterium, whose 
carbon food comes from the atmosphere: 398. 

DIAGONALS of parallelotopes (Relations between). 540. 

DIFFRACTION of Röntgen-rays. 247. 

DILUVIUM (Some new under-cambrian erratic-blocks from the Dutch). 561. 

— (Two new mid-cambrian erratic-blocks from the Dutch). 652. 

DINITROANISOL (Nitration of symmetrical). 650. 

DISPERSION of sunlight (Peculiarities and changes of FrAUNHOFER-lines interpreted as 
anomalous) in the corona, 589. 

DISSOCIATION in and crystallisation from a solid solution. 643. 

DISTHENE (On the behaviour of) and of sillimanite at high temperature. 240. 

piro (J. w.) and QC, A. LoBry pe Bruyn. The boilingpoint-curve of the system: 
hydrazine + water. 171. 

puBOIsS (uUG.). The geological structure of the [londsrug in Drenthe and the 
origin of that ridge. (L). 93. (II). 101. 

EFFECT (A new law concerning the relation between stimulus and). 392. 441. 

EISENROSE (On an) of the St. Gotthard. 605. 

ELECTRIC CIRCUIT (Some remarkable phenomena, concerning the) in electrolytes. 465, 

ELECTRIC CURRENT (On the advantage of metal-etching by means of the). 219. 

ELECTROLYTE (On the potential-differenee, which occurs at the surface of contact of 
two different non-miscible liquids, in which a dissolved) has distributed itself. 431. 

ELECTROLYTES (Some remarkable phenomena, concerning the electric circuit in), 465, 

ELEGTROMAGNETIC PHENOMENA (The fundamental equations for) in ponderable bodies, 
deduced from the theory of electrons. 254. 

ELECTRO-MECHANIGS (Statistical). (1). 22. (LI). 114. 

ELECTRONS (Contributions to the theory of. (I). 608. 

— (The fundamental equations for electromagnetic phenomena in ponderable bodies, 
deduced from the theory of). 254. 

EMISSION (On the) and absorption by metals of rays of heat of great wavelengths. 666. 

ENTROPY (Lhe principle of) in physiology. (LL). 57. 

EQUATION OF srate (The) and the y-surface in the immediate neighbourhood of the 
critical state for binary mixtures with a small proportion of one of the components. 


DIEM 
— (The variability with the density of the quantity 4 of the). 487. 


VI CONTENTS. 


EQUATIONs (Reduction of observation) containing more than one measured quantity. 236. 


— (The fundamental) for electromagnetic phenomena in ponderable bodies, deduced 


from the theory of electrons. 254. 


EQUILIBRIA of phases in the system: acetaldehyde + paraldehyde with and without. 


molecular transformation. 283. 
ERRATIC-BLOCKS (Cambrian) at Hemelum in the South-West of Frisia. 140. 
— (Some new under-cambrian) from the Dutch diluvium. 561. 
— (Two new mid cambrian) from the Dutch diluvium. 652. 

ERRATUM. 217. 

rsrers (On the so-called compounds of salts of sulphoncarboxylic acids with sulphuric).482.« 

ErHANE and Methylalcohol (Critical phenomena of partially miscible liquids). 473. 

Ethnology. A. W. Nieuwenuuis: “Influence of changed conditions of life on the 
physical and psychical development of the population of Central-Borneo.” 525, 

FORMALDEHYDE (Methylene-) derivatives of sugars and glucosides. 175. 

FRANCHIMONT (a. P. N.). On the so-called compounds of salts of sulphoncarboxylic 
acids with sulphuric esters. 482. 

FRAUNHOFER-LINES (Peculiarities and changes of) interpreted as anomalous dispersion 
of sunlight in the corona. 559. 

GALVANIC CELLS and the phase rule. 182. 

GANGLIONCELLS (On the structure of the light percepting cells in the spinal cord, on 
the neurofibrillae in the) and on the innervation of the striped muscles in Am- 
phioxus lanceolatus. 350. 

Gases (Isotherms of diatemie) and their binary mixtures, V. An accurate volumeno- 
meter and mixing apparatus. 636. 

— (Measurements on the magnetic rotation of the plane of polarisation in liquetied) 
under atmospheric pressure. 245. 

Geology. Eve. Dusors: “The geological structure of the Hondsrug in Drenthe and the 

origin of that ridge”. (I). 93. (IL). LOL 

— J. H. Bonnema: “Cambrian erratic-blocks at Hemelum in the South-West of 
Frisia”. 140. 

_ J. H. Boxnema: “Some new under-cambrian erratic-blocks from the Dutch dilu- 
vium’’. 561. 

—_ J. H. Bornema: “Two new mid-cambrian erratic-blocks from the Dutch dilu- 
vium”. 652. 

GEOMETRICAL representation (On the) of the motion of variable systems. 386. 

eiucostpEs (Formaldehyde (methylene)- derivatives of sugars and). 175. 

— (Investigations of) in connection with the internal mutation of plants. 295. 

HAGA (Hm) and C. H. Winp. Diflraction of Rontgen-rays 247. 

HALLO (3. J.). The value of some magneto-optic constants. 458. 

HALOGENACEFANILIDES (The intramolecular rearrangement in) and its velocity. (1). 178. 
(II). 359. 

uzart (On the duration of the compensatory pause after stimulation of the auricle of 
the mammalian). 378. 

HEMELUM (Cambrian erratic-blocks at) in the South-West of Frisia. 140. 


YY = VR 


— 


CO NSE ENS: VII 


HOGENRAAD (G. B). On an /Eisenrose” of the St. Gotthard. 605, 

HONDSRUG in Drenthe (The geological structure of the) and the origin of that ridge. 
(93. (Snore 

HYDRAZINE (The conductive power of) and of substances’ dissolved therein. 551. 

— + water (The boilingpoint-curve of the system :). 171. 

HYDROGEN (The course of the values of 4 for), in connection with a recent formula 
of Prof. van DER Waars. 573. 

HYNDMAN (H. H. FR) and H. Kamertinau ONNes, Isotherms of diatomic gases 
and their binary mixtures. V. An accurate volumenometer and mixing apparatus. 636. 

HYPOTHESIS (An) on the nature of solar prominences. 162. 

INDEX (On the refractive) of rock-glasses. 602. 

INNERVATION (On the structure of the light-percepting cells in the spinal cord, on 
the neurofibrillae in the ganglioncells and on the) of the striped muscles in 
Amphioxus lanceolatus. 350. 

INTEGERS (An analytical expression for the greatest common divisor of two). 658. 

INTENSITY (On maxima and minima of) sometimes observed within the shading of 
strongiy widened spectral lines. 662. 

INTERPOLATION (On) based on a supposed condition of minimum. 364. 

INTRAMOLECULAR rearrangement of atoms in azoxybenzene and its derivatives. 51. 

— rearrangement (The) in halogenacetanilides and its velocity. (1). 178. (LI). 359. 
ropipE (The transformation of diphenyliodonium) and chloride and its velocity. 646. 
ISOTHERMS of diatomic gases and their mixtures. V. An accurate volumenometer and 

mixing apparatus. 636. 

ITERSON JR. (G. va N). Accumulation experiments with denitrifying bacteria. 148. 

— The decomposition of cellulose by aérobic micro-organisms. 685. 

JULIUS (W. H.). An hypothesis on the nature of solar prominences. 162. 

— presents a paper of Prof. E. Corner and Tu. Srrencers: “On the atomic weight 

of antimony”. 543. 

— Peculiarities and changes of Pravnuoree-lines interpreted as anomalous disper- 
sion of sunlight in the corona. 589. 

— On maxima and minima of intensity sometimes observed within the shading 
of strongly widened spectral lines. 662. 

JUNGIUS (c, L.) and C. A. Lopry pe Bruyn. Dissociation in and crystallisation from 
a solid solution. 643. 

KAMERLINGH ONNES (H.) presents a paper of W. H. Kersom: “Reduction of 
observation equations containing more than one measured quantity”. 236. 

— presents a paper of Dr. L. H. Srertsema: “Measurements on the magnetic rotation 
of the plane of polarisation in liquefied gases under atmospheric pressure, LL. 
Measurements with methylehloride”. 243. 

— presents a paper of Dr. J. E. Verscaarreir: “Contributions to the knowledge 
of VAN DER WAALS y-surface. VII. The equation of state and the y-surface in 
the immediate neighbourhood of the critical state for binary mixtures with a smali 
proportion of one of the components”. 321. 336, 


Vr CO NAT Nate, 


KAMERLINGH ONNES (H) presents a paper of Dr. L. H.Sierrsema: “The 


. é . . . . . 
valeulation — from the magnetic rotation of the plane of polarisation, for sub- 
UL 


stances without an absorptionband in the visible spectrum”. 415. 

— presents a paper of Prof. J. P. KueneN: “Critical phenomena of partially mis- 
cible liquids-Ethane and Methylaleohol”. 473. 

— Methods and apparatus used in the Cryogenic Laboratory. LIL. Bath of very 
uniform and constant low temperatures in the cryostat. 502. 628. A cryostat of 
modified form for apparatus of small dimensions. 628. IV. A permanent bath of 
liquid nitrogen at ordinary and at reduced pressure. 63i, V. Arrangement of a 
BURCKHARDT-WEISS vacuumpump for use in the circulations for low temperatures. 633. 

— and H. H. Fr. HYNDMAN. Isotherms of diatomic gases and their binary mix- 
tures. V. An accurate volumenometer and mixing apparatus. 636. 

KEESOM (w. H.). Reduction of observation equations containing more than one 
measured quantity. 236. 

KLUYVER (J. C.). An analytical expression for the greatest common divisor of two 
integers. 658. 

KNIPSCHEER (H. M.). Intramolecular rearrangement of atoms in azoxybenzene and 
its derivatives, 51. 

KOLK (J. L.C. SCHROEDER VAN DER). See SCHROEDER VAN DER Kork (J. L. C.). 

KORTEWEG (p. J.). Plaitpoints and corresponding plaits in the neighbourhood of 
the sides of the -surface of VAN DER Waars. 445. 

KUENEN (J. P.). Critical phenomena of partially miscible liquids-Ethane and Methyl- 
alcohol. 473. 

LAAR (5. J. VAN). The course of the melting-point-line of solid alloys or amal- 
gams. (I), 424. (LI). 511. 

— On the potential-difference, which occurs at the surface of contact of two different 
non-miscible liquids, in which a dissolved electrolyte has distributed itself. 431. 

— On the course of the values of 4 for hydrogen, in connection with a recent 
formula of Prof. vaN DER Waars. 573. 

LANGELAAN (J. w.). The principle of entropy in physiology. (LI). 57. 

Law (A new) concerning the relation between stimulus and effect. 392. ALL, 

Lire (lufluence of changed conditions of) on the physical and psychical development 
of the population of Central-Borneo. 525. 

uquips (Critical phenomena in partially miscible). 307. 

— (Critical phenomena of partially miscible)-Ethane and Methylaleohol. 475. 

— (On the potential-difference, which occurs at the surface of contact of two difle- 
rent non-miscible), in which a dissolved electrolyte has distributed itself. 431. 

LOBRY DE BRUYN (c. A.) presents a paper of Dr. H. M. Knipscueer: “Intra- 
molecular rearrangement of atoms in azoxybenzene and its derivatives.” 51. 

— presents a paper of Dr. J. J. Buanxsma: “The intramolecular rearrangement in 
halogenacetanilides and its velocity.” (1). 178. (ID. 359. 

— presents a paper of Dr. Tu. Weevers: “Investigations of glucosides in connec- 


tion with the internal mutation of plants,” 295. 


CHAOS NE TAN LS? IX 


LOBRY DE BRUYN (Cc. A.) presents a paper of Dr. J. Porter van Loon: “Benzi- 
dine transformation.” 377. 

— presents a paper of Mr. A. H. J. Berzer: “The velocity of transformation of 
tribroomphenol bromine into tetrabromophenol.’’ 556. 

— presents a paper of Mr. E. H. Bicuner: “The transformation of diphenylio- 
donium iodide and chloride and its velocity”. 646. 

— presents a paper of Dr. J. J. BLANKSMA: “Nitration of symmetrical dinitro- 
anisol’’. 650, 

— and W. ALBERDA VAN EKENSTEIN. Formaldehyde (methylene)- derivatives of 
sugars and glucosides, 175. 

— and HE, Conen. The conductive power of hydrazine and of substances dissolved 
therein. 551, 

— and J. W. Divo. The boilingpoint-curve of the system: hydrazine + water. 171, 

— and C. L. Junetus, Dissociation in and crystallisation from a solid solu- 
tion. 645, 

LOON (J. POTTER VAN). See Porrer VAN LOON (J.). 

LORENTZ (H. A.). The fundamental equations for electromagnetic phenomena in 
ponderable bodies, deduced from the theory of electrons. 254. 

— presents a paper of Mr. A. H. Srrks: “Some remarkable phenomena, concerning 
the electric circuit in electrolytes”. 465. 

— Contributions to the theory of electrons. (I). 608. 

— On the emission and absorption by metals of rays of heat of great wave- 
lengths. 666. 

MAGNETO-OPTIC Constants (The value of some). 438. 

MARTIN (K.) presents a paper of Prof. Euc. DuBois: “Geological structure of the 
Hondsrug in Drenthe and the origin of that ridge.” (1). 93. 

Mathematics. P. H. Scuoure: “On the connection of the planes of position of the 
angles formed by two spaces Sx passing through a point and incident spacial 
systems.” 53. 

— S, L. van Oss: “Five rotations in S, in equilibrium.” 362. 

— J. CARDINAAL : “On the geometrical representation of the motion of variable 
systems.” 386. 

— Jan pe Vries: “On the spheres of Monee belonging to ordinary and tangential 
pencils of quadratic surfaces.” 484. 

— P. H. Scuoure: ‘‘Relations between diagonals of parallelotopes.” 540. 

— J. C. Krurver: “An analytical expression for the greatest common divisor of 
two integers.” 658. 

MEASUREMENTS on the magnetic rotation of the plane of polarisation in liquefied 
gases under atmospheric pressure. IT. Measurements with methylchloride. 243. 

MELTING-POINT-LINE (The course of the) of solid alloys or amalgams. (D), 424. 
(IL). 511. 

METAL-ETCHING (On the advantage of) by means of the electric current. 219. 

METALS (On the emission and absorption by) of rays of heat of great wave-lengths. 666, 

METHOD (A new) for demonstrating cartilaginous mikroskeletons. 47. 


x CONTENTS. 


METHODS and apparatus used in the Cryogenic Laboratory. III. Bath of very uniform 
and constant low temperatures in the cryostat. 502. 628. A cryostat of modified 
form for apparatus of small dimensions. 628. IV. A permanent bath of liquid 
nitrogen at ordinary and at reduced pressure. 631. V. Arrangement of a BURCKHARDT- 
Weiss vacuumpump for use in the circulations for low temperatures. 633. 

METHYLALCOHOL (Critical phenomena of partially miscible liquids-Ethane and). 473. 

METHYLCHLORIDE (Measurements with). 243. 

METHYLENE-derivatives. See FORMALDEHYDE (methylene)-derivatives. 

Microbiology. G. van Iverson Jr.: “Accumulation experiments with denitrifying bac- 
teria”. 148. 

— G van Iverson Jr.: “The decomposition of cellulose by aérobic micro-orga- 
nisms.” 685. 

MIKROSKELETONS (A new method for demonstrating cartilaginous). 47. 

Mineralogy. E. H. M. Brexman: “On the behaviour of disthene and of sillimanite 
at high temperature.” 240. 

— P. Trescu: “On the refractive index of rockglasses.” 602. 
— G. B. Hocrnraap: “On an /Eisenrose” of the St. Gotthard.” 605, 

MIXING APPARATUS (An accurate volumenometer and). 636. 

mMIxTuREs (The equation of state and the y-surface in the immediate neighbourhood 
of the critical state for binary) with a small proportion of one of the components. 
321. 336. 

— (Isotherms of diatomic gases and their binary). 636. 

MOLECULAR transformation (Some observations on the course of the). 303. 

MOLL (J. w.) presents a paper of Mr. J. H. Bonnema: “Cambrian erratic-blocks at 
Hemelum in the South-West of Frisia.” 140. 

— presents the dissertation of Dr. J. C. Scourge: “Die Stelär-Theorie.” 497. 

— presents a paper of Mr. J. H. Bonnema: “Some new under-cambrian erratic- 
blocks from the Dutch diluvium”. 561. 

— presents a paper of Mr. J. H. Bonnema: “Two new mid-cambrian erratic-blocks 
from the Dutch diluvium.” 652. 

MONGE (On the spheres of) belonging to ordinary and tangential pencils of qua- 
dratic surfaces. 484. 

MOTION of variable systems (On the geometrical representation of the). 386. 

MUSCLES in Amphioxus lanceolatus (On the structure of the light-percepting cells in 
the spinal cord, on the neurofibrillae in the ganglioncells and on the innervation 
of the striped) in Amphioxus lanceolatus. 350. 

MUTATION of plants (Investigations of glucosides in connection with the internal). 295. 

NEUROFIBRILLAE (On the structure of the lightpercepting cells in the spinal cord, 
on the) in the ganglioncells and on the innervation of the striped muscles in 
Amphioxus lanceolatus. 350. 

NIEROP (A. S. VAN) and L. ARONSTEIN. On the action of sulphur on Toluene and 
Xylene. 288. 

NIEUWENHUIS (A. w.). Influence of changed conditions of life on the physical 
and psychical development of the population of Central-Borneo, 525. 


CONTENTS XI 


NITRATION of symmetrical dinitroanisol. 650. 

NITROGEN (A bath of liquid) at ordinary and at reduced pressure. 631. 

OBSERVATORY AT LEYDEN (On the yearly periodicity of the rates of the standardeloek 
of the), Hohwü n®. 17. (L). 68. (ID. 193. 

— (Preliminary investigation of the rate of the standardclock of the) Hohwü no. 17, 
after it was mounted in the niche of the great pier. 267. 

Oss (Ss. L. VAN). Five rotations in S, in equilibrium. 362. 

PARALDEHYDE (Equilibria of phases in the system: acetaldehyde +) with and without 
molecular transformation, 283. 

PARALLELOTOPES (Relations between diagonals of), 540. 

PEKELHARING (c. A.) presents a paper of Prof. kK. F. WenckesBacu: “On the 
duration of the compensatory pause after stimulation of the auricle of the mam- 
malian heart”, 378. 

PENCILS (On the spheres of Monrer belonging to ordinary and tangential) of qua- 
dratic surfaces. 484. 

PERIODICITY (On the yearly) of the rates of the standardeloek of the Observatory at 
Leyden, Hohwü No 17. (I). 68. (II). 193. 

PHASE RULE (Galvanic cells and the). 182. 

PHASES (A representation in space of the regions in which the solid) which occur, 
are the components, when not forming compounds. 279. 

— (Equilibria of) in the system: acetaldehyde -+- paraldehyde with and without 
molecular transformation. 285. 

PHENOMENA (Critical) in partially miseible liquids. 307. 

— (Critical) of partially miscible liquids-Ethane and Methylalcohol, 473. 

— (Some remarkable), concerning the electric circuit in electrolytes. 465. 

Physics. J. D. van DER Waars: “Ternary Systems”. (IV) 1. (V). 121. 

— J. D. van per Waats Jr.: “Statistical electromechanics”. (L). 22. (IJ). 114. 

— P. ZEEMAN: “Observations on the magnetic rotation of the plane of polarisation 
in the interior of an absorption band”. 41. 

— W. H. Jurrus: “An hypothesis on the nature of solar prominence”. 162. 

— A. H. Srrks: “On the advantage of metal-etching by means of the electric 
current’. 219, 

— J. D. van per Waats: “On the conditions for the occurrence of a minimum 
critical temperature for a ternary system”. 225. 

— W. H. Krrsom: “Reduction of observation equations containing more than one 
measured quantity”. 236. 

— L. H. Srertsema: “Measurements on the magnetic rotation of the plane of pola- 
risation in liquefied gases under atmospheric pressure. If. Measurements with 
Methylehloride”, 243. 

— H. Haca and C. H. Winp: “Diffraction of Röntgen-rays” (2nd communication). 
247. 

— H. A. Lorentz: “The fundamental equations for electromagnetic phenomena in 
ponderable bodies, deduced from the theory of electrons”, 254, 


XII C.O,N-2 ENE: 


Physics. J. D. van per Waats: “Some observations on the course of the molecular 
transformation”. 303. 
— J. D. van per Waals: “Critical phenomena in partially miscible liquids”. 307. 
— J. K. A. WERTHEIM SALOMONSON: “The influence of variation of the constant 
current on the pitch of the singing arc”. 311. 
— J. E. VERSCHAFFELT : “Contributions to the knowledge of VAN DER WAALS -sur- 
face. VII. The equation of state and the y-surface in the immediate neighbour- 
hood of the critical state for binary mixtures with a small proportion of one of 


the components.” 321. 336. 


4 é - : 
— L. H. Srertsema: “The calculation — from the magnetic rotation of the plane 
mM 


of polarisation, for substances without an absorptionband in the visible spectrum”. ~ 


413. 

— J.J. Harro: “The value of some magneto-optic constants”. 438. 

— D.J. Korrewea: “Plaitpoints and corresponding plaits in the neighbourhood of 
the sides of the y-surface of VAN DER WAALS”. 445. 

— A. H. Srrxs: “Some remarkable phenomena, concerning the electric circuit 
in electrolytes”. 465. 

— J. P. KveNEN: “Critical phenomena of partially miscible liquids-Ethane and Me- 
thylaleohol”. 473. 

— J. D. van DER Waars Jr.: “The variability with the density of the quantity 5 
of the equation of state”. 487. 

— H. KAMERLINGH Onnes: “Methods and apparatus used in the Cryogenic Laboratory: 
UI. Baths of very uniform and constant low temperatures in the cryostat. 502. 628. 
A eryostat of modified form for apparatus of small dimensions. 628. IV. A permanent 
bath of liquid nitrogen at ordinary and at reduced pressure. 631. V. Arrangement 
of a BurckHarpt-WeIss vacuumpump for use in the circulations for low tem- 
peratures. 633, 

— J. J. van Laar: “On the course of the values of 4 for hydrogen, in con- 
nection with a recent formula of Prof. vaN per Waats”. 573. 

— W. H. Junius: “Peculiarities and changes of FRAUNHOFER-lines interpreted as 
consequences of anomalous dispersion of sunlight in the corona.” 589. 

— H. A. Lorentz: “Contributions to the theory of electrons.” (I). 608. 

— H. KAMERLINGH ONNEs and H. H. Francis HynpMan: “Isotherms of diatomic 
gases and their binary mixtures. V. An accurate volumenometer and mixing 
apparatus.” 636. 

— W. H. Juxrus: “On maxima and minima of intensity sometimes observed within 
the shading of strongly widened spectral lines.” 662. 

— H. A, Lorentz: “On the emission and absorption by metals of rays of heat of 
great wave-lengths.” 666. 

Physiology. J. W. LANGELAAN: “The principle of entropy in physiology.” ID. 57. 


a 


CONTENTS XIII 


Physiology. J. Porke: “On the structure of the light-percepting cells in the spinal cord, 
on the neurofibrillae in the ganglioncells and on the innervation of the striped 
muscles in Amphioxus lanceolatus.” 350. 

— K. F. Wenckesacu : “On the duration of the compensatory pause after stimulation 
of the auricle of the mammalian heart.” 378. 

— J. kK. A. WERTHEIM SALOMONSON: “A new law concerning the relation between 
stimulus and effect.” 392, 441. 

Physiology of plants. Tu. Weevers: “Investigations of glucosides in connection with 
the internal mutation of plants.” 295. 

PLACE (r.) presents a paper of Dr, J. W. LANGELAAN : “The principle of entropy 
in physiology.” (ID. 57. 

— presents a paper of Dr. J. Boeke: “On the structure of the light-percepting cells 
in the spinal cord, on the neurofibrillae in the ganglioncells and on the inner- 
vation of the striped muscles in Amphioxus lanceolatus.” 850. 

PLALTPOINTS and corresponding plaits in the neighbourhood of the sides of the p-surface 
of VAN DER WaaLs. 445. 

PLANE OF POLARISATION (Observations on the magnetic rotation of the) in the interior 
of an absorptionband. 41, 

— (Measurements on the magnetic rotation of the) in liquefied gases under atmos- 


pheric pressure, 243, 


2 


: ¢ ; : j : 
— (The calculation — from the magnetic rotation of the) for substances without 
m 


an absorptionband in the visible spectrum. 415. 


PLANES OF POSITION (On the connection of the) of the angles formed by two spaces 


Sn passing through a point and incident spacial systems. 55. 
PLANTS (Investigations of glucosides in connection with the internal mutation of), 295. 


PONDERABLE BODIES (The fundamental equations for electromagnetic phenomena in), 
deduced from the theory of electrons, 254. 


POPULATION of Central-Borneo (Influence of changed conditions of life on the physical 
and psychical development of the). 525. 

POTENTIAL=DIFFERENCE (On the), which occurs at the surface of contact of two difle- 
rent non-miscible liquids, in which a dissolved electrolyte has distributed itself. 431. 

POTTER VAN LOON (3). Benzidine transformation, 377. 

PRINCIPLE (The) of entropy in physiology. (LI). 57. 

PRUNUS (On the prussic acid in the opening buds of). 31. 

QuaNTITY (Reduction of observation equations containing more than one measured). 236. 

— 4 (The variability with the density of the) of the equation of state. 487. 

RAYS OF HEAT (On the emission and absorption by metals of) of great wave-length, 666. 

REINDERS (w.). Galvanic cells and the phase rule, 182. 

ROCK-GLASSES (On the refractive index of). 602. 

RÖNTGEN-RAYS (Diffraction of). 247. 

ROOZEBOOM (H, W. BAKHUIS). See BaKuuis RoozeBoom (H. W.). 


xIV CONTENTS. 


ROTATION (Observations on the magnetic) of the plane of polarisation in the interior 
of an absorptionband. 41. 
— (Measurements on the magnetic) of the plane of polarisation in liquetied gases 
under atmospheric pressure. 245. 
— (The caleulation ~ from the magnetic) of the plane of polarisation for substances 
without an absorptionband in the visible spectrum. 413. 
ROTATIONS (Five) in Sy in equilibrium. 362. 
SALOMONSON (J. K. A. WERTHEIM). See WERTHEIM SALOMONSON (J. K. A). 
SANDE BAKHUYZEN (BE. F. VAN DE). On the yearly periodicity of the rates 
of the standardeloek of the Observatory at Leyden, Hohwü n°. 17. (I). 68. (IL). 193. 
— Preliminary investigation of the rate of the standardeloek of the Observatory at 
Leyden, Hohwü n°. 17 after it was mounted in the niche of the great pier. 267. 
SANDE BAKHUYZEN (H. G. VAN DE) presents a paper of Mr. J. WeEEDER: 
“On interpolation based on a supposed condition of minimum”. 364, 
scuHourE (J. c). Die Stelär-Theorie, 497. 
scuOUTE (P. B). On the connection of the planes of position of the angles formed 
by two spaces Sa passing through a point and incident spacial systems. 53. 
— presents a paper of Dr. S. L. van Oss: “Five rotations in Sy in equilibrium.” 362. 
— Relations between diagonals of parallelotopes. 540, 
SCHROEDER VAN DER KOLK (J. L. C.) presents a paper of Mr. A. IL. Sirks: 
“On the advantage of metal-etching by means of the electric current.” 219. 
— presents a paper of Mr. E. H. M. BEEKMAN: “On the behaviour of disthene and 
of sillimanite at high temperature”. 240. 
— presents a paper of Mr. P. Tescu: “On the refractive index of rock-glasses”. 602, 
— presents a paper of Mr. G. B. HoGenraap: “On an „Eisenrose” of the St. 
Gotthard.” 605. 
SHADING (On maxima and minima of intensity sometimes observed within the) of 
strongly widened spectral lines. 662. 
sLERTSEMA (L. H.). Measurements on the magnetic rotation of the plane of pola- 
risation in liquefied gases under atmospheric pressure. LI. Measurements with 
Methylchloride. 245. 


— The calculation — from the magnetic rotation of the plane of polarisation for 
it 


substances without an absorptionband in the visible spectrum. 415. 
SILICEOUS SPICULES (On the shape of some) of sponges. 104. 
SILLIMANITE (On the behaviour of disthene and of) at high temperature. 250. 
SIRKs (A. H.). On the advantage of metal-etching by means of the electric current. 219. 
— Some remarkable phenomena, concerning the electric circuit in electrolytes. 465. 
sMITs (a) and L. K. Wourr. The velocity of transformation of carbon monoxide, 417. 
SOLAR prominences (An hypothesis on the nature of). 162. 
SOLUTION (Dissociation in and crystallisation from a solid). 643. 
space (A representation in) of the regions in which the solid phases which occur, 


are the components, when not forming compounds. 279. 


CONT ENTS. -XV 


spaces S, (On the connection of the planes of position of the angles formed by 
two) passing through a point aud incident spacial systems. 55. 
SPECTRAL LINES (On maxima and minima of intensity sometimes observed within the 
shading of strongly widened), 662, | 
SPECTRUM (The calculation < from the magnetic rotation of the plane of polarisation 
for substances without an absorptionband in the visible). 413. 
SPHERES of Monge (On the) belonging to ordinary and tangential pencils of quadratie 
surfaces. 484. . 
SPONGEs (On the shape of some siliceous spicules of). 104. 
STANDARDCLOCK (On the yearly periodicity of the rates of the) of the Observatory at 
Leyden, Hohwii no. 17. (L). 68. (ID. 193. 
— (Preliminary investigation of the rate of the) of the Observatory at Leyden, 
Hohwü no. 17, after it was mounted in the niche of the great pier. 267. 
STATISTICAL electro-mechanics. (I), 22. (II). 114. 
STELAR-THEORIE (Die). 497. 
STIMULUS and Hifect (A new law concerning the relation between). 392. 441. 
STRENGERS (TH.) and B. Couen. On the atomic weight of antimony. 543. 
STRUCTURE (Lhe geological) of the Hondsrug in Drenthe and the origin of that ridge, 
MG) DB (The LOL: 
SUGARS and Glucosides (Formaldehyde (methylene)-derivatives of). 175. 
SULPHUR (On the action of) on toluene and xylene. 288, 
L-surracE (Contributions to the knowledge of van per Waats’). VIT. ‘The equation 
of state and the y-surface in the immediate neighbourhood of the critical state 
for binary mixtures with a small proportion of one of the components. 321. 836. 
— (Plaitpoints and corresponding ptaits in the neighbourhood of the sides of the) 
of VAN DER WAALS. 445. 
SURFACE OF conract (On the potential-difterence, which occurs at the) of two different 
non-miscible liquids, in which a dissolved electrolyte has distributed itself. 431. 
SURFACES (On the spheres of Monee belonging to ordinary and tangential pencils of 
quadratic). 484. 
SYSTEM (On the conditions for the occurrence of a minimum critical temperature for 
a ternary). 225, 
— Acetaldehyde + Paraldehyde (Equilibria of phases in the) with and without 
molecular transformation. 283. 
— Hydrazine + Water (The boilingpoint-curve of the). 171. 
SYSTEMS (On the connection of the planes of position of the angles formed by two 
spaces Su passing through a point and incident spacial), 53. 
— (On the geometrical representation of the motion of variable). 386. 
— (Ternary). (IV). 1. (V). 121. 
TEMPERATURE (Bath of very uniform and constant low) in the cryostat. 502. 628. 
— (On the conditions for the occurrence of a minimum critical) for a ternary system, 225. 
TEMPERATURES (Arrangement of a BuRcKHARDT-WEIss vacuumpump for use in the 
circulations for low). 633. 


XVI CON T EV Sets 


TERNARY SYSTEM (On the conditions for the occurrence of a minimum critical tem- 
perature for a). 225. 

TERNARY SYSTEMS, (LV). 1. (V). 121. 

rescu (v.). On the refractive index of rock-glasses. 602. 

TETRABROMOPHENOL (The velocity of transformation of tibroomphenol bromine into). 556. 

TuEORY of electrons (Contributious to the). (1). 608. 

— of electrons (The fundamental equations for electromagnetic phenomena in pon- 

derable bodies, deduced from the). 254. 

TINAMALGAMS, 873. 

— (The meltingpoint-line of). 511. 

TOLUENE and Xylene (On the action of sulphur on), 288. 

TRIBROOMPHENOL bromine (The velocity of transformation of) into tetrabromophenol. 556. 

VACUUMPUMP (A BureKHARDT-Werss) for use in the circulations for low temperatures. 
633. 

VALUES of 4 (The course of the) for hydrogen, in connection with a recent formula of 
Prof. van perk Waars. 573. 

VARIATION (The influence of) of the constant current on the pitch of the singing are. 
311. 

vELocity of transformation (The) of carbon monoxide 417. 

— of transformation (The) of tribroomphenol bromine into tetrabromophenol. 556. 
VERSCHAFFELT (E.). On the prussic acid in the opening buds of Prunus. 31. 
VERSCHAFFELT (J. £.). Contributions to the knowledge of VAN DER WAALS’ 

y-surface. VIL. The equation of state and the \-surface in the immediate neigh- 
bourhood of the critical state for binary mixtures with a small proportion of one 
the components. 321. 336. 

VOLUMENOMETER (An accurate) and mixing apparatus. 636. 

VOSMAER (G. C. J.). On the shape of some siliceous spicules of sponges. 104. 

VRIES (HUGO DE) presents a paper of Prof. KE. Verscuarrenr: “On the prussic 
acid in the opening buds of Prunus.” 31. 

VRIES (JAN DE). On the spheres of Monee belonging to ordinary and tangential 
pencils or quadratic surfaces. 484. 

WAALS (VAN DER) g-surfuce (Contributions to the knowledge of). VII. The 
equation of state and the p-surface in the immediate neighbourhood of the critical 
state for binary mixtures with a small proportion of one of the components. 
321. 336. 

— (Plaitpoints and corresponding plaits in the neighbourhood of the sides of the 

Y-surface of). 445. 
WAALS (3. D. VAN DER). Ternary systems. ([V). 1. (V). 121. 
— presents a paper of Dr. J. D, van DER Waats JR: “Statistical electro-mecha- 
mies’. {y.ye2, (UL). 114. 

— On the conditions for the occurrence of a minimum critical temperature for a 
ternary system. 225, 

— Some observations on the course of the molecular transformation. 303. 


— Critical phenomena in partially miscible liquids. 307. 


a 


Gr OUNS TREN Tes: XVII 


WAALS (J. D. VAN DER) presents a paper of Dr. J. D. van per Waats Jr.: 
“The variability with the density of the quantity 4 of the equation of state.” 487. 
— presents a paper of Mr. J. J. van Laar: “On the course of the values of 4 
for hydrogen, in connection with a recent formula of Prof. VAN DER Waars”’. 573. 
WAALS JR. (J. D. VAN DER). Statistical electromechanics. (I). 22. (II). 114. 
— The variability with the density of the quantity > of the equation of state. 487. 
WATER (The boilingpoint-curve of the system: Hydrazine +). 171. 
WEEDER (J.). On interpolation based on a supposed condition of minimum. 364. 
WEEVERS (TH.). Investigations of glucosides in connection with the internal muta- 
tion of plants. 295. 
WENCKEBACH (K. F.). On the duration of the compensatory pause after stimula- 
tion of the auricle of the mammalian heart. 378. 
WERTHEIM SALOMONSON (J. K. A). The influence of variation of the con- 
stant current on the pitch of the singing arc. 311. 
— A new law concerning the relation between stimulus and effect. 392. 441. 
WIND (c. H.) and H. Haga. Diffraction of Röntgen-rays. 247. 
WINKLER (c.) presents a paper of Prof. J. K. A. WERTHEIM SaLomonson: “A new 
law concerning the relation between stimulus and eflect”. 392. 441. 
WOLFF (L. kK.) and A. Smits. The velocity of transformation of carbon monoxide. 417. 
WYHE (J. W. VAN). A new method for demonstrating cartilaginous mikroskeletons. 47. 
XYLENE (On the action of sulphur on toluene and). 288. 
ZEEMAN (e.). Observations on the magnetic rotation of the plane of polarisation in 
the interior of an absorption band, 41. 
— presents a paper of Prof. I. K. A. Werranim SALOMONSON: “The influence of 
variation of the constant current on the pitch of the singing are”. 311. 
— presents a paper of Dr. J. J. Harro: “The value of some magneto-optic con- 
stants”. 438. 
Zoology. G. C. J, Vosmarr: “On the shape of some siliceous spicules of sponges”. 104, 


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