Classics of modern science : $b (Copernicus to Pasteur)
History
Classics of modern science : $b (Copernicus to Pasteur)
Science; Science -- History
But the heat of the warmer bodies strives perpetually to pass to
bodies less warm by radiation and conduction, and thus to establish
an equilibrium of temperature. At each motion of a terrestrial body,
a portion of mechanical force passes by friction or collision into
heat, of which only a part can be converted back again into mechanical
force. This is also generally the case in every electrical and chemical
process. From this, it follows that the first portion of the store of
force, the unchangeable heat, is augmented by every natural process,
while the second portion, mechanical, electrical, and chemical force,
must be diminished; so that if the universe be delivered over to
the undisturbed action of its physical processes, all force will
finally pass into the form of heat, and all heat come into a state of
equilibrium. Then all possibility of a further change would be at an
end, and the complete cessation of all natural processes must set in.
The life of men, animals, and plants, could not of course continue if
the sun had lost its high temperature, and with it his light,--if all
the components of the earth’s surface had closed those combinations
which their affinities demand. In short, the universe from that time
forward would be condemned to a state of eternal rest.
These consequences of the law of Carnot are, of course, only valid,
provided that the law, when sufficiently tested, proves to be
universally correct. In the mean time there is little prospect of the
law being proved incorrect. At all events we must admire the sagacity
of Thomson, who, in the letters of a long known little mathematical
formula, which only speaks of the heat, volume, and pressure of bodies,
was able to discern consequences which threatened the universe, though
certainly after an infinite period of time, with eternal death.
Public-domain text, read in full here on John Shaqi.
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