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THE

CHEMICAL

VOLUME LXIII.

NEWS.

EDITED BY WILLIAM CROOKES, F.R.S., &c.

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No. 1623.-JANUARY 2, 1891.

apparatus to be used in standardising other, platinum BOILING-POINT thermometers. A table is also given reduced from a previous series of observations of other fixed points which may be used for the same purpose.

OF STANDARDISING PLATINUM
RESISTANCE THERMOMETERS BY
REFERENCE TO IT.*

By HUGH L. CALLENDAR, M.A., Fellow of Trinity College,
Cambridge, and E. H. GRIFFITHS, M.A., of Sidney Sussex
College, Cambridge.

EXPERIMENTS by different observers have shown that electrical resistance thermometers afford the most convenient and accurate method of measuring temperature through a very wide range. By selecting a particular thermometer as the standard, and directly comparing others with it, it has been found possible to attain a degree of accuracy of the order of o'oor in the relative measurements between o° and 100° C., and of the order of o'or° at 450° C.

In a previous communicationt it has been shown that, if t be the temperature by air thermometer, and if pt be the temperature by platinum resistance thermometer, the difference between them is very closely represented from 0° to 700° C. by the formula

d=t-pt=8{t/100-t/100}

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The value of the constant for a particular wire was found to be 1'570. The object of the present paper is to describe a method of finding the value of this constant for any such thermometer, by means of a single observation at some known fixed point other than o° or 100° C.

The boiling-point of sulphur happens to be the most convenient for this purpose. We have therefore made a careful determination of this point by reference to the standard air thermometer, and have given a full description of the method and apparatus which we have found most suitable for standardising platinum thermometers by means of it.

The paper is divided into three parts.

Part III. contains a comparison of the platinum and air thermometers between o° and 100°, and shows that the d-formula holds accurately between those limits.

The determination of the boiling-point of sulphur was made by means of three platinum thermometers, L, MI, and M2, constructed out of the wire used in the experiments of 1887, before referred to.

Full descriptions of these thermometers are given in the paper. They were furnished with double electrodes for measuring the resistance of the connecting wires at each observation, their insulation was carefully tested, and all due precautions were taken to guard against thermal effects and other sources of error.

Thermometers M, and M2 were standardised by direct comparison with an air thermometer at the boiling-point of sulphur. Full particulars are given of the details of the observations and calculations, showing the limits of error of the experiments.

The expansion of the glass forming the bulb of the air thermometer was determined both by the method of linear expansion, and also by using the bulb itself as a mercury weight thermometer. The values found by the two methods agreed very closely.

The small changes of the volume of the bulb were determined from time to time during the progress of the experiments. The final observations were not taken till the thermometer had reached a fairly steady state.

The limit of accuracy attainable with this air thermometer was found to depend chiefly on that of the barometric readings. The barometer used was therefore verified by a careful comparison with the standard metre scale.

The iron-tube apparatus in which the platinum and air thermometers were compared was so constructed as to be capable of being maintained at a constant temperature by a steady flow of sulphur vapour for any length of time.

Observations were taken with it on two separate days. On each occasion the temperature was kept steady to o'r° for about two hours. Allowing for the difference of the atmospheric pressure, the temperature attained was the same on both days.

Part I. contains a description of the method and apparatus employed in comparing the platinum thermometers used in this investigation with the air thermometer The results of the comparison were in perfect agreeat a temperature very near the boiling-point of sulphur. ment with the experiments of 1887, and showed that the Part II. contains the determination of the actual boiling--coefficient of the wire had not altered appreciably in the point of sulphur by means of the thermometers thus standardised, and a description of the method and

Abstract of a Paper read before the Royal Sociey, Dec. 18, 1890. + Callendar, Phil. Trans., A., 1887, p. 161.

interval.

The apparatus which we have found most convenient for standardising platinum thermometers by means of the boiling-point of sulphur consists of a wide glass tube, 40

c.m. long and 4 c.m. in diameter, with a spherical bulb at the end. Tubes of this kind are commonly used to heat Victor Meyer's vapour-density apparatus. For brevity we have called it a "Meyer" tube.

The outside of the tube is thickly padded with asbestos wool, with the exception of the lower half of the bulb, and of a short length of 3-5 c.m. at the top, which serves as a condenser. The tube is filled with sulphur to a level of 3 or 4 c.m. above the bulb, and is heated by a Bunsen burner. The gas is adjusted so as to keep the level of the vapour near the top of the tube, which is covered with asbestos card to prevent the sulphur catching fire.

Our experiments have shown that a thermometer inserted in an apparatus of this kind will not attain the actual temperature of the vapour, unless it is protected from radiation to the sides of the tube, and from the condensed liquid which runs down the stem. lowering of temperature due to radiation, &c., may readily amount to upwards of 2° at the boiling-point of sulphur.

The

The method which we have adopted for screening the to its stem a short distance above the bulb. Two coaxial tubes are hung on to this umbrella to screen the thermometer from radiation. We have found that glass is not sufficiently opaque to heat radiation at this temperature. The inner tube at least should be of metal.

thermometer is to bind an umbrella of asbestos card on

To avoid superheating of the vapour, it is necessary to make sure that the level of the liquid sulphur stands well above that part of the bulb which is exposed to the flame.

Using these precautions, we have found that the temperature by normal air thermometer at constant pressure of the saturated vapour of sulphur, boiling freely under a pressure of 760 m.m. of mercury at o° C. and g = 980'61 C.G.S. (sea level in lat. 45°), is—

t=444 53° C.

The value given by Regnault is nearly 4° higher than this; but in the account which he gives of his experiments he has pointed out several sources of error, and it is evident that he did not place much confidence in his results.

The close agreement between the air thermometer experiments of 1887 and the present series leads us to conclude that the number above given is probably correct to a tenth of a degree, and that it may be safely used for standardising platinum thermometers.

The method which we recommend for standardising platinum thermometers is briefly as follows:-Observe the value Rs of the resistance in sulphur vapour in an apparatus such as we have described. Calculate the value of pts by the formula

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100 (Rs Ro)/(R100R。). Find the temperature t of the sulphur vapour, corresponding to the corrected barometric pressure Ho, from the formula

t = 444'53+0'082 (H。-760).

NEWS

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carefully determined as the boiling-point of sulphur. The fixed points given in the above have not been so They rest entirely on the assumption of the accuracy of the formula, and have not been directly referred to the air thermometer. We believe, however, that they are probably correct to o'r° C., and that they may be safely used to standardise thermometers of limited range, in cases where it may happen to be inconvenient to make use of the sulphur point.

In comparing the platinum and air thermometers between 0 and 100° C., observations were taken at intervals of 5° all the way up. The mean deviation of the observations from the parabolic formula (d) is only 0.006°. This corresponds to the limit of accuracy of the barometric readings, and there is no reason to suppose that the d-formula may not represent the difference even more closely than this.

The same platinum thermometer has been compared with several mercury thermometers standardised at Kew. The result seems to show that the Kew standard reads o'1° C. lower than our air-thermometer at 30'.

THE VARIATIONS OF ELECTROMOTIVE FORCE OF CELLS CONSISTING OF CERTAIN METALS, PLATINUM, AND NITRIC ACID.† By G. J. BURCH, B.A., and V. H. VELEY, M.A., the University Museum, Oxford.

THE description of the apparatus, the capillary electrometer, and the method of working are given fully in the paper. The following conclusions are drawn from the results of the experiments :

I. When the metals copper, silver, bismuth, and mercury are introduced into purified nitric acid of different degrees of concentration, and a couple made with platinum, the electromotive force of such a cell increases considerably until it reaches a constant and (in most

The appropriate value of ♪ is then given by the equation- cases) a maximum value. The rise of E.M.F. is attributed

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to the production of nitrous acid by the decomposition of the nitric acid, and the final value is considered to be due to the former acid only, while the initial value is due for the most part to the latter acid, though it is affected to a remarkable degree by the amount of impurity of nitrous acid, either initially present or produced by minute and unavoidable uncleanliness of the metallic strip and the containing vessel.

II. If nitrous acid has been previously added to the nitric acid, then the maximum E.M. F. is reached at once. III. If the conditions, namely, increase of temperature, of impurity, and of concentration of acid, are such as

Griffiths," Brit. Assoc. Report," 1890.

Abstract of a Paper read before the Royal Society.

would favour a more rapid solution of the metal, and consequently a more rapid production of nitrous acid, then the rise of E.M.F. is concomitantly more rapid.

IV. Conversely, if the conditions are unfavourable to the production of nitrous acid, the rise of E.M.F. is less rapid.

V. If any substance, such as urea, be added which would tend so destroy the nitrous acid as fast as it may be formed, then the rise of E.M.F. is extremely slow, being dependent upon the number of molecular impacts of the nitrous acid upon the surface of the metal.

Thus the results obtained by the electrometer and by the chemical balance are in every way confirmatory the one of the other.

The authors propose to conduct further investigations on cells containing other acids, to determine whether the action of them upon metals is conditioned by the presence of their products of electrolysis.

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THIS paper is in continuation of a preliminary communication on the same subject; the main points contained in it are as follows:

I. The metals copper, mercury, and bismuth do not dissolve in nitric acid of about 30 per cent concentration (the acid commonly employed for the preparation of nitric oxide gas) and heated to a temperature of 30° C., provided that nitrous acid is neither present initially nor formed subsequently. To prevent this it is necessary in the cases of copper and bismuth to add a small quantity of some oxidising substance, such as hydrogen peroxide or potassium chlorate, or, as less efficacious, potassium permanganate, or to pass a current of air or, lastly, such a substance as urea, which destroys the nitrous acid by its interaction.

II. If the conditions are such that these metals dissolve, then the amount of metal dissolved and the amount of nitrous acid present are concomitant variables, provided that the nitric acid is in considerable excess. Change of conditions, such as concentration of acid and variation of temperature, which increase the former increase also the latter.

III. If the conditions are such that these metals dissolve, it would appear that the metallic nitrite is at first formed, together with nitric oxide; the former is decomposed by the excess of nitric acid to liberate nitrous acid, while the latter reduces the nitric acid to form a further quantity of nitrous acid.

Eventually the net result is the product of two reverse chemical changes represented by the equations

(i.) 2NO+HNO,+H20=3HNO2,
(i.) 2HNO2=2NO+ HNO3+ H2O.

The nitrous acid is thus destroyed as fast as it is generated.

IV. If the conditions are such that metals dissolve in nitric acid, then nitrous acid is invariably the initial product of reduction.

V. The metals copper, mercury, and bismuth dissolve very readily in a 1 per cent solution of nitrous acid; under these conditions nitric acid present in slight excess interferes with, rather than promotes, the chemical change. This result is probably due to the greater stability of nitrous acid in the presence of nitric acid.

VI. Hydrogen gas reduces nitric to nitrous acid in presence of cupric or lead nitrate; it also converts

* Abstract of a Paper read before the Royal Society.

mercuric into mercurous nitrate, but does not produce any change in solutions of bismuth and zinc nitrates dissolved in nitric acid.

FRICTION OF GASES IN PIPES.

By Dr. L. C. LEVOIR, Polytechnicum, Delft.

THE introduction of gaseous fuel in factories compels lecturers in technical colleges to discuss a series of quite new laws. In all the old treatises on Physics and Chemistry no experiment is related that might give a large audience an idea of the diminution in pressure on conducting gases through tubes. In the CHEMICAL NEWS for August 3rd, 1861 (vol. iv., p. 60), and Dingler's Polytechnisches Journal (German), 1861, I described an experiment to show that friction of smoke in a chimney is higher in a conical one when the widest end is used as inlet.

Two small gas-flames on the same T-shaped gas-pipe, with very low pressure of the gas, gave me an opportunity to show that one of the flames was nearly invisible on the opposite side from where the chimney (1 metre in length, and 2 and 5 centimetres in diameter) drew with the highest force.

But there is a still more sensitive test for difference in exhausting power, that is, in every Bunsen's burner of great size the inlet for the air must be regulated in the stand, that the flame cannot burn on the top, but detonates always downwards from too great admixture of air. A small end of tube placed in the air-holes directly stops that explosion, by causing friction therein and diminishing the quantity of air admitted.

Evidently this is a way to show to a large audience the friction of smoke in chimneys and gas in tubes, which is so difficult a point both in the education of physicis and engineers.

ON GASEOUS ILLUMINANTS.* By Professor VIVIAN B. LEWES.

I.

JuST 200 years after Van Helmont (in the seventeenth century) first used the term "" gas "to describe aëriform bodies, Faraday defined a gas as being the vapour of a volatile liquid, existing at a temperature considerably above the boiling-point of the liquid, and that the condensing-point of the gas was merely the boiling-point of the liquid producing it. This definition was contested at the time, as several of the gases had not then been condensed; but now it is known that the condensation of any gas to the liquid form is merely a question of suffi ciently intense cold, and pressure.

Hydrogen and the gaseous compounds of carbon and hydrogen have so strong an affinity for the oxygen contained in the atmosphere, that the heat emitted by a burning match is generally sufficient to determine combination between the gases; and where the heat evolved by the combination is sufficient to raise the gases or vapour to incandescence, the phenomenon of flame is the result. Some flames have the power, under certain conditions, of emitting light, while others have no photometric value; and it is a matter of the gravest importance to the gas world that as clear a conception as possible should be obtained of the conditions and cause of luminosity in flames. A visible flame may either be solid-that is to say, composed of a solid mass of incandescent particles-or it may have a distinctive internal structure, and show zones in which varying phases of combustion are taking place; and it is to this latter class

* Abstract of the Cantor Lectures delivered at the Society of Arts Communicated by the Author.

that all flames produced by a gas issuing from a burner belong.

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In the Philosophical Magazine for 1817 Sir Humphry Davy says, while alluding to a paper published in one of the early numbers of the Journal of Science and Arts: "Iperiments which show that with ordinary gas it is the have given an account of some new results on flame which show that the intensity of the light of flames depends principally upon the production and ignition of solid matter in combustion."

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His theory, however, has gradually been altered by frequent quotation, until it is more often given as "the presence of solid particles suspended in the flame (or in immediate contact with the burning gas) is essential to its luminosity - an idea which Davy never had, as is shown by him later in the paper defining flame as follows:-" Flame is gaseous matter heated so highly as to be luminous;" and again: "When in flames, pure gaseous matter is burnt, the light is extremely feeble." Moreover, he alludes to "common flames "-evidently meaning the flames of candle, lamps, or gas; in all which cases I think it can be proved beyond a doubt that his theory, as expounded by himself, was perfectly correct. On June 11, 1868, Professor E. Frankland read a communication before the Royal Society, in which he described experiments which led him to doubt Sir Humphry Davy's theory. He points out that the deposit of soot formed when a cold surface is held in a gas or candle flame is not pure carbon, but contains hydrogen, which can only be got rid of by prolonged heating in an atmosphere of chlorine. Also that many flames possessing a high degree of luminosity cannot possibly contain solid particles. Arsenic burnt in oxygen gives a bright white light; yet as arsenic volatilises at 180° C., and the arsenic trioxide forms at 2180 C., it is evident that at the temperature of incandescence (which is at least 500° C.) there can be no solids, but simply vapours present in the flame; and for the same reason, the intense light resulting from the burning of phosphorus in oxygen cannot be explained by the solid particle theory. From these results Dr. Frankland considers that "incandescent particles of carbon are not the source of light in gas and candle flames, but that the luminosity of these flames is due to radiations from dense but transparent hydrocarbon vapours ; and he further shows that non-luminous flames, such as that produced by carbon monoxide and hydrogen, can, when burning in an atmosphere of oxygen, be rendered luminous if the ordinary atmospheric pressure is increased to 10 atmospheres, so as to prevent or retard as far as possible expansion during combustion. From Dr. Frankland's experiments, there is no doubt that the luminosity of a flame is increased by pressing around it the atmosphere in which it is burning, and also that rarefaction has the opposite effect-a point also worked at by Davy; but his experiments do not show that incandescent particles of carbon are not the principal source of luminosity in a gas flame. He also shows that the higher the density of the vapours present in a flame, the more likely is it to be luminous.

In 1874, Soret attempted to demonstrate the existence of solid particles in a luminous hydrocarbon flame, by focussing the sun's rays on the flame, and examining the reflected light by means of a Nicol prism; but neither his research nor that of Burch, who repeated his experiments, using the spectroscope instead of the prism, showed more than that solid particles are present. Herr W. Stein, in considering Dr. Frankland's objections to Davy's theory, pointed out that the soot which is deposited from a candle or gas flame, and which Frankland looked upon as a condensed hydrocarbon, contains 991 per cent of carbon and only o'9 per cent of hydrogen, which is about the quantity of hydrogen one would expect to be occluded by carbon formed under these conditions, and he also pointed out that if the soot were a heavy hydrocarbon condensed by a cold surface, cooling the vapour present in the flame, it ought to again become volatile at a high temperature, which it does not. The next steps in the

controversy were the attempts made by Hilgard, Landolt, and Blochman to trace the actions taking place in various flames by withdrawing the gases from different parts of the flame and determining their composition. Exhydrogen which burns first, whilst the heavy hydrocarbons become gradually reduced by the heat of the flame into simpler compounds until in the luminous zone of the flame they are broken down into carbon and methane, and it is the carbon in excessively minute particles which at the moment of liberation is heated to incandescence, and " principally" gives the light of the flame-the marsh gas originally present, and also that formed from the heavier hydrocarbons, adding its quota to the luminosity by still further decomposition during combustion, and finally becoming carbon dioxide and water. In 1876, Dr. Karl Heumann made a most important contribution to the theory of luminous flames in some papers published in Liebig's Annalen, in which he carefully went over the work of previous observers, and, by a large number of original experiments, proved that Davy's theory was correct, but that other causes also affected the degree of luminosity in a gas or candle flame.

In the ordinary atmospheric burner in which a mixture of coal-gas and air burn with a non-luminous flame, it was supposed that the admixture of air, by supplying oxygen to the inner portion of the flame, caused immediate and complete oxidation of the hydrocarbons, without giving time for the liberation of carbon in the flame, and consequenily luminosity. More modern researches, however, have proved this to be utterly wrong. The loss of luminosity is due to two causes-first, to the diluting action of the air introduced; secondly, to the fact that when a gas is so diluted it requires a far higher temperature to break up the hydrocarbons present than when the gas is undiluted, and therefore the temperature which serves to liberate carbon and render the undiluted gasflame luminous, is totally insufficient to do so in the diluted gas. Consequently the hydrocarbon burns to carbon dioxide and water without any such liberation, and hence with a non-luminous flame. The truth of this theory can be easily proved by the fact that diluting the gas with nitrogen, carbon dioxide, or even steam, serves to render it non-luminous, and therefore more rapid oxidation has very little or nothing to do with it, while the non-luminous flame can again be rendered luminous either by heating the mixture of air and gas just before combustion, or by heating the air with which the gas is diluted. This being so, it is evident that in the nonluminous flame we have the same hydrocarbon present as in the luminous flame; and anything that will tend to break them up, and liberate the carbon before the hydrocarbons are consumed, should again make the flame luminous. That heat will do this has been already shown; but it can be demonstrated in a still more striking way. It is well known that chlorine gas and bromine vapour will both support the combustion of a gas containing much hydrogen, but that the combustion is very different from that of the same gas burning in air, as the chlorine or bromine, having no affinity for the carbon, combines with the hydrogen only, and deposits the carbon in clouds of soot; in other words, at the temperature of flame, chlorine will break up the hydrocarbons and liberate solid carbon. If now a small quantity of chlorine is led into the non-luminous Bunsen flame, it at once becomes luminous; proving conclusively that luminosity is due to solid particles of carbon liberated in the flame. Again, Heumann points out that a small rod held in the luminous flame becomes rapidly covered on its lower side with a deposit of soot; that is to say, the soot is present in particles in the flame, and the uprush of the gas drives it against the rod and deposits it there. If the soot were present in the flame, as Frankland supposed, in the state of vapour, and the rod merely acted by cooling and con. densing it, the soot should be deposited on all sides of the

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rod; while a still further proof is that if the soot existed as vapour in the flame, then if the rod were heated to a high temperature no soot should be deposited on it, whereas the soot deposits on a heated surface just as well as on a cool one.

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It has been objected to the "solid particle" theory that, if it were true, solid carbon particles introduced into non-luminous flame should render it luminous and make it look like an ordinary gas-flame, whereas it simply gives rise to a cloud of sparks. But it must be remembered that the "nascent" carbon, as it is liberated from the decomposing hydrocarbons, is in the molecular condition, and has a very different degree of coarse-grainedness to any preparation of charcoal or lampblack we can make; takes so long to burn that it leaves the flames only partly and that, although our finest particle is a mass which consumed, and is projected into the air as a spark, the molecular particles of carbon are consumed as soon as they are rendered incandescent, and a steady luminosity, free from sparks, results. It is possible, however, to make the particles in a luminous flame roll themselves together, when they can be either deposited in a very coarse kind of soot, or be seen as glowing sparks and particles in the mantle of the flame. This can be done when two luminous flames are allowed to rush against each other or against a heated surface. Heumann also shows that the luminous mantle of a flame is not alto. gether transparent, and that the thicker the flame-layer, and the greater the number of solid particles contained in it, the less transparent does it become. If a non-luminous flame-say hydrogen- is charged with the vapour of chromyl dichloride (CrO2Cl2), chromic oxide is produced; and this flame, which undoubtedly contains solid particles, is quite as transparent as the hydrocarbon flame. Finally, those flames which undoubtedly owe their luminosity to the presence of finely divided solid matter produce characteristic shadows when viewed in sunlight; the only luminous flames which do not throw shadows being those which consist of glowing vapours and gases. Luminous gas-flames, oil-lamp flames, and candle flames produce strongly-marked shadows in sunlight, and therefore contain finely-divided solid matter; and that this can be nothing but carbon is evident from the fact that all other substances capable of remaining solid at the temperature of the flames are absent.

NOTES ON A RED SEDIMENT FORMED IN
A RAFFINOSE SOLUTION.

By F. G. WIECHMANN, Ph D.

WHILE engaged in the isolation of raffinose from a low
beet-sugar, the writer incidentally obtained from the raffi
nose solution a precipitate, bright red in colour, and of
peculiar properties, which he has so far been unable to
identify as one of the numerous substances whose occur-
rence in saccharine solutions has been established.
The incident seemed sufficiently curious to merit re-
cording, and although the amount of the substance
brief history of the case, and a description of the pro-
secured was, unfortunately, too small to permit of
ultimate analysis or of an exhaustive investigation, a
perties of the body, as far as determined, may prove of

interest.

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Work was commenced on November 23, 1888. The different steps taken were as follows:To 6000 grms. of raw sugar there were added 6000 c.c. methyl alcohol.

The solution was after some time drained off, and the sugar treated with an additional 4000 c.c. of methyl alcohol. From the 10,000 c.c. alcohol added, about 7400 c.c. were recovered.

This solution was placed on a water-bath and the alcohol evaporated completely.

When this had been accomplished, and while the solution was still warm, ethyl alcohol was added until a permanent turbidity was caused.

This precipitate was allowed to settle, and was then separated from the clear solution.

allowed for settling being in each instance about two This operation was performed six times; the time days.

Then the raffinose syrup, perfectly free from alcohol, was drawn off.

This syrup amounted to 200 c.c., and was divided into three portions.

these portions, a brief statement of the treatment which As the coloured sediment was produced in only one of each of these portions received is given.

PART I.-20 c.c. were devoted to a trial of Scheibler's method for preparing raffinose.*

From the foregoing considerations, it must be admitted that Sir Humphry Davy's statement that the intensity of the light of flames (such as those produced by candles, oil, or gas) depends principally upon the production and ignition of solid matter in combustion, was undoubtedly the true one; and it must also be borne in mind that the degree of luminosity of a flame is affected by the constituents of the gas other than the heavy hydrocarbonssome, like marsh gas, although ordinarily burning with an apparently non-luminous flame, and separating no soot, adding considerably to the luminosity at the temperature of the flame, while others, like carbon monoxide, reduce it. The luminosity of a flame is increased by an increase of density in the media in which it is burning, and is deTreatment was commenced January 16, 1889, and by creased by rarefaction-an effect supposed by Dr. Frank-September 5, 1889, the separation of the raffinose crystals land to be owing to the alteration of density and alteration of the mobility of the oxygen molecules in the air. This view, however, had been contested by Wartha, who conIcluded that it was due to the effect of pressure on the dissociation point of the hydrocarbons burning in the flame; this taking place more rapidly under increased pressure, and therefore liberating the carbon more quickly. However this might be, the effect of pressure on luminous flames was very marked, even under ordinary atmospheric pressure; the difference of an inch in the barometric column making 5 per cent difference in the luminosity. A burner giving 100 units of light with the barometer at 30 inches would only give 95 units if it fell to 29, while a rise to 31 inches would mean an increase of the luminosity to 105 units.

seemed complete.

PART II.-50 c.c. were treated as follows:The specific gravity of the syrup was determined to be 1'4022.

To the 50 c.c. (70'11 grms.), there were added 140°22 grms. acetate of lead. Then absolute ethyl alcohol was added, and the solution heated on a water-bath.

The precipitate which formed was filtered out, suspended in water, and sulphuretted hydrogen was passed in until complete precipitation of the lead had been accomplished.

The sulphide of lead was filtered out and thoroughly washed with water. The filtrate was evaporated on a

Zeitschrift des Vereines für Ruben-zucker Industrie, 1888, p. 337.

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