Classics of modern science : $b (Copernicus to Pasteur)
History
Classics of modern science : $b (Copernicus to Pasteur)
Science; Science -- History
Let us make this addition to our assumption; that, at the commencement,
the density of the nebulous matter was a vanishing quantity, as
compared with the present density of the sun and planets; we can then
calculate how much work has been performed by the condensation; we can
further calculate how much of this work still exists in the form of
mechanical force, as attraction of the planets towards the sun, and as
_vis viva_ of their motion, and find by this how much of the force
has been converted into heat.
The result of this calculation is, that only about the 454th part
of the original mechanical force remains as such, and that the
remainder, converted into heat, would be sufficient to raise a mass
of water equal to the sun and planets taken together, not less than
twenty-eight millions of degrees of the centigrade scale. For the
sake of comparison, I will mention that the highest temperature which
we can produce by the oxyhydrogen blowpipe, which is sufficient to
fuse and vaporize even platina, and which but few bodies can endure,
is estimated at about two thousand centigrade degrees. Of the action
of a temperature of twenty-eight millions of such degrees we can
form no notion. If the mass of our entire system were pure coal,
by the combustion of the whole of it only the 3500th part of the
above quantity would be generated. This is also clear, that such a
development of heat must have presented the greatest obstacle to the
speedy union of the masses, that the larger part of the heat must have
been diffused by radiation into space, before the masses could form
bodies possessing the present density of the sun and planets, and that
these bodies must once have been in a state of fiery fluidity. This
notion is corroborated by the geological phenomena of our planet; and
with regard to the other planetary bodies, the flattened form of the
sphere, which is the form of equilibrium of a fluid mass, is indicative
of a former state of fluidity. If I thus permit an immense quantity of
heat to disappear without compensation from our system, the principle
of the conservation of force is not thereby invaded. Certainly for our
planet it is lost, but not for the universe. It has proceeded outwards,
and daily proceeds outwards into infinite space; and we know not
whether the medium which transmits the undulations of light and heat
possesses an end where the rays must return, or whether they eternally
pursue their way through infinitude.
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