XVI. On the value in absolute alcohol of spirits of different specific gravities

1847 ◽  
Vol 137 ◽  
pp. 249-251 ◽  

Having been for some months past occupied with experiments on the fermentation of sugar and molasses, and having found it necessary to construct for this purpose a new table of the quantity per centum by weight of absolute alcohol contained in spirits of different specific gravities, I venture to lay the same before the Royal Society, hoping that it may be found generally useful in inquiries of this kind, and also for other purposes. The Table was formed synthetically; absolute alcohol and distilled water were weighed out in the required proportions, mixed in small well-stopped bottles and well-shaken together. After standing three or four days the mixtures were brought to the temperature of 60° Fahr. exactly, and their specific gravities determined with great care. After the lapse of two or three days more this last-named operation was repeated, but in no case was it observed that any further contraction had occurred. Neither was the specific gravity of a mixture containing nearly equal parts alcohol and water which had been so examined changed by being inclosed in a strong accurately-stoppered bottle, and heated for some time to a temperature above its boiling-point.

Having been recently engaged in a series of experiments on the fermentation of sugar and molasses, which rendered it necessary to refer to a table of the value in absolute alcohol of spirits of different specific gravities, the author found himself compelled to construct for this purpose a new table, which he lays before the Royal Society in the present paper. The table was formed by weighing out absolute alcohol and distilled water in fixed proportions, mixing them, and after allowing time for condensation, determining with suitable precautions the specific gravity of each mixture at the temperature of 60° Fahrenheit. Each alternate number in the table was so obtained; the rest being interpolated. The alcohol employed was prepared by digesting the strongest rectified spirit, first with dry carbonate of potash and afterwards with powdered quicklime and distilling. It had the specific gravity ·7938 at 60°, and boiled at 177° Fahr.


1814 ◽  
Vol 104 ◽  
pp. 487-507 ◽  

1. On the triple Compounds containing Iodine and Oxygene. 1. In this communication I shall have the honour of pre­senting to the Royal Society, a continuation of the inquiries I have made respecting the chemical agencies of iodine, and the properties of certain of its compounds. 2. I described in my last paper the action of iodine on fixed alkaline lixivia, and the deflagrating salts it forms. In the first experiment which I made on these compounds, I employed the first crystals which fall down from moderately strong solutions of potassa and soda saturated with iodine, which had been purified by being repeatedly acted upon by distilled water: I now find that this process is not sufficient to free the triple compound from the double compound; and that to obtain them in a state of absolute purity, it is necessary to boil them repeatedly in small quantities of alcohol of specific gravity of from 8.6 to 9.2, which dissolves the double compound, but has little power of action on the triple compound.


1897 ◽  
Vol 21 ◽  
pp. 156-159
Author(s):  
Crum Brown ◽  
R. Fairbairn

Sodium mercaptide and dibromosuccinic ether, in the proportion of two molecules of the former to one of the latter, were dissolved separately in absolute alcohol, and slowly mixed. A considerable evolution of heat took place, while sodium bromide separated out. The flask was then digested for some hours on the steam-bath. The alcohol was subsequently distilled off, and the residue, on cooling, was treated with water. An oil separated out. This oil was collected by means of a separating funnel, and the aqueous layer several times extracted with ether. The oil and the ethereal extracts were added together and dried over calcium chloride. Next morning the ether was distilled off at the ordinary pressure. The remainder was distilled in vacuo. Between 50° and 60° a few drops came over, which proved to be ethyldisulphide.The remainder came over between 150° and 170°.This latter fraction was redistilled, and a portion of it used for analysis. The boiling point at 20 mm. pressure was 160°.Combustion of dietthiosuccinic ether.Weight of substance taken = ·2477 gram.Weight of carbonic acid obtained = ·4476 gram.Weight of water obtained = ·1702 gram.


1857 ◽  
Vol 8 ◽  
pp. 111-116 ◽  

The Trigonometrical Survey of the United Kingdom commenced in the year 1784, under the immediate auspices of the Royal Society; the first base was traced by General Roy on the 16th of April of that year, on Hounslow Heath, in presence of Sir Joseph Banks, then President of the Society, and some of its most distinguished Fellows. The principal object which the Government had then in view, was the connexion of the Observatories of Paris and Greenwich by means of a triangulation, for the purpose of determining the difference of longitude between the two observatories.


2019 ◽  
Vol 10 (01) ◽  
pp. 20-27
Author(s):  
Dian Kurnia Sari ◽  
Rian Ternando

Minyak bumi dievaluasi guna menentukan potensi minyak bumi sebagai bahan baku kilang minyak untuk menghasilkan fraksi yang dikehendaki. Evaluasi yang dilakukan meliputi pengujian sifat umum minyak bumi, klasifikasi minyak bumi dengan distilasi True Boiling Point (TBP) wide cut (pemotongan jarak lebar) serta analisis fraksi kerosin. Fraksi kerosin yang dihasilkan dari primary process dapat diolah menjadi bahan bakar rumah tangga (minyak  tanah) dan bahan bakar lampu penerangan. Selain itu fraksi kerosin juga dapat dioalah menjadi bahan bakar untuk pesawat terbang jenis jet (avtur). Avtur adalah kerosin yang dengan  spesifikasi yang diperketat, terutama mengenai titik uap dan titik beku. Untuk melakukan pengolahan pada minyak bumi perlu diketahui karakteristik dan spesifikasi minyak  bumi (bahan baku) yang akan diolah untuk mengetahui mutu dan manfaat minyak bumi tersebut. Salah satu parameter uji analisis minyak bumi yaitu parameter sifat fisika. Dari data distilasi TBP diperoleh persentase fraksi kerosin Crude Oil 99 PT HS sebesar 29 % vol sedangkan Crude Oil 165 PT RT sebesar 23 % vol. Berdasarkan analisis sifat fisika yang meliputi Specific Gravity, Refractive Index nD20, Freezing Point, Smoke Point, Flash Point “Abel”, Aniline Point, Copper Strip Corrosion, Kinematic Viscosity dan Characterization KUOP. Crude Oil 99 dan Crude Oil 165 memiliki mutu yang baik serta memenuhi spesifikasi produk kerosin maupun produk avtur.


1868 ◽  
Vol 158 ◽  
pp. 57-73 ◽  

Many drawings of the Great Nebula in Orion have already been published by different astronomers; still as the present drawing was made with the advantage of instrumental power far exceeding that at the disposal of previous observers, and as great care has been taken to make it accurate, in fact every available hour during the winter months of seven seasons having been employed upon it, perhaps it may be of some interest to the Royal Society. Several drawings of this wonderful object were published previous to the year 1825, but they were made with instruments of little power; however, in 1825, Sir J. Herschel published a drawing made with his celebrated 18-inch reflector (Memoirs of the Astronomical Society, 1826). Sir J. Herschel’s second drawing with the same instrument, but under more favourable circumstances, together with a description and a catalogue of stars, was published in 1847 (Cape of Good Hope Observations). That was succeeded in 1848 by Mr. Bond’s drawing, also with a description and catalogue of stars (Memoirs of the American Academy of Arts and Sciences, 1848).


1912 ◽  
Vol 31 ◽  
pp. 375-396
Author(s):  
A. P. Laurie

In a paper read before the Royal Society of Edinburgh (Proc. Roy. Soc. Edin., xxviii., part v., p. 382 (1908); Zeit. phys. Chem., lxiv. 5) I described a new type of concentration cell, in which the one platinum electrode was surrounded by a solution of ·025 molecules of KI containing ·001 molecules of iodine dissolved in absolute alcohol, and the other electrode was surrounded by ·025 molecules of KI and ·001 molecules of iodine, dissolved in water. This cell developed a considerable E.M.F. of ·198 volts at 25° C. in the direction which would transfer the iodine from water to alcohol and potassium iodide from alcohol to water.


1867 ◽  
Vol 15 ◽  
pp. 502-503 ◽  

Some light may possibly be thrown upon the history of such metals found in nature as are of a soft colloid description, particularly native iron, platinum, and gold, by an investigation of the gases which they hold occluded, such gases being borrowed from the atmosphere in which the metallic mass last found itself in a state of ignition. The meteoric iron of Lenarto appeared to be well adapted for a trial. This well-known iron is free from any stony admixture, and is remarkably pure and malleable. It was found by Wehrle to be of specific gravity 7·79, and to consist of— Iron ........... 90·883 Nickel .......... 8·450 Cobalt ........... 0·665 Copper .......... 0·002 From a larger mass a strip of the Lenarto iron 50 millimetres by 13 and 10 millimetres, was cut by a clean chisel. It weighed 45·2 grammes, and had the bulk of 5·78 cubic centimetres. The strip was well washed by hot solution of potassa, and then repeatedly by hot distilled water, and dried. Such treatment of iron, it had' been previously found, conduces in no way to the evolution of hydrogen gas when the metal is subsequently heated The Lenarto iron was enclosed in a new porcelain tube, and the latter being attached to a Sprengel aspirator, a good, vacuum was obtained in the cold. The tube being placed in a trough combustion furnace, was heated to redness by ignited charcoal. Gas came off rather freely, namely— In 35 minutes ........... 5·38 cub. centims. In 100 minutes .......... 9·52 cub. centims. In 20 minutes ........... 1·63 cub. centims. In 2 hours 35 minutes .......... 16·53 ‾‾‾‾ cub. centims.


1860 ◽  
Vol 150 ◽  
pp. 257-276 ◽  

The researches which I beg, in the following pages, to submit to the Royal Society, embody the results obtained in the further development of an observation which I made a considerable number of years ago, and which, since that time, I had to defend against the objections of others, both by experimental inquiries of my own, and by the collection and discussion of facts elicited in the investigations of other observers. As far back as 1841* I pointed out that in analogous compounds the same difference of composition frequently involves the same difference in boiling-points. The assertion of the existence of this law-like relation between the chemical composition of substances and one of their most important physical properties, when first enunciated, met rather with the opposition than with the assent of chemists. In Germany especially it was contested by Schröder in his memoir “On the Molecular Volume of Chemical Compounds.” These objections led me to collect additional evidence in favour of my views, and to show more particularly that in very extensive series of compounds (alcohols C n H n+2 O 2 ; acids C n H n O 4 ; compound ethers C n H n O 4 , &c.) an elementary difference x C 2 H 2 is attended by a difference of x X 19°C. in the boiling-points, and how this fact is intimately connected with other regularities exhibited by the boiling-points of organic compounds. Almost at the same period Schröder § convinced himself that the relation I had pointed out obtains in most cases. He collected himself a considerable number of illustrations of the regularities I had traced, and showed that the relation in question is rendered more especially conspicuous if the compounds be expressed by formulæ representing equal vapour-volumes of the several substances. Some of the views, however, which were peculiar to Schröder have not gained the approbation of chemists. This physicist was inclined to consider the boiling-point of a substance as the most essential criterion of its proximate constituents, as the most trustworthy indicator of its molecular consti­tution. His views were chiefly based upon the assumption that the elementary difference C 2 H 2 , when occurring in alcohols C n H n+2 O 2 , involved a difference of boiling-points other than that occasioned by the same elementary difference obtaining in acids C n H n O 4 and that the isomeric compound ethers differed from one another in their boiling-points. An extensive series of boiling-point determinations* which I made of these isomeric ethers, proved that the latter assumption is not founded on facts. The exertions made by Schröder, Gerhardt, Löwig and others, in the hope of recognizing the influence of the constituent elements on the boiling-point of a compound, have also essentially remained without result.


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