Scientific American Supplement, No. 1082, September 26, 1896Various
Science
Scientific American Supplement, No. 1082, September 26, 1896
Various
Science -- Periodicals
Mr. A. Allard, starting from the fact that the richness in starch
increases along with the density, has constructed a simple apparatus
that gives both these data at once, with sufficient precision, and
without calculations, tables, etc. It is, upon the whole, a large
areometer with constant weight and variable volume that is plunged
into a cylindrical vessel 0.5 m. in depth and 0.3 m. in diameter,
filled with water. The instrument itself consists of three parts: (1)
A lower receptacle in which is placed a weight to assure the
equilibrium; (2) a central float into which is put a kilogramme of
very clean and very dry potatoes; and (3) a rod graduated for density
and feculometric richness. The deeper the apparatus sinks, the more
valuable is the potato. How much more?
The degree to which the rod sinks shows this. The same principle and
the same instrument might be applied to the determination of the
density of various agricultural products, such as beets, cider fruits,
grain, etc. It would suffice to graduate a special scale each time.
For each variation of a thousandth in density, the areometer sinks
about 5 millimeters--that is to say, it presents a sensitiveness that
is more than sufficient in practice.--Le Monde Illustré.
* * * * *
THE COMING LIGHT.
There is no more eager contest than that which has been going on for
some time between gas and electricity. Which of these two systems of
lighting will triumph? Will electricity suppress gas, as gas has
dethroned the oil lamp? A few years ago, the answer to this question
would not have been doubtful, and it seemed as if gas in such contest
must play the role of the earthen pot against the iron one. At present
the case is otherwise.
The Auer burner has re-established the equilibrium, and the Denayrouse
burner is perhaps going to decide the fate of electricity.
As naturalists say, the function creates the organ, and it is truly
interesting to observe that in measure as the need of an intenser and
cheaper light grows with us, science makes it possible for us to
satisfy it by giving us new systems of lighting or by improving those
that we already have at our disposal.
What a cycle traversed in twenty years! What progress made! Let us
remember that the electric light scarcely became industrial until the
time of the Exposition (1878), and that the Auer burner obtained the
freedom of the city only five or six years ago. Is there any need of
recalling the advantages of these two lights? In the first, a feeble
disengagement of caloric, automatic lighting and a steadier light; in
the second, a better utilization of the gas, which gives more light
and less heat.
Public-domain text, read in full here on John Shaqi.
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