Buffon's Natural History, Volume 01 (of 10): Containing a Theory of the Earth, a General History of Man, of the Brute Creation, and of Vegetables, Mineral, &c. &cBuffon, Georges Louis Leclerc, comte de
History
Buffon's Natural History, Volume 01 (of 10): Containing a Theory of the Earth, a General History of Man, of the Brute Creation, and of Vegetables, Mineral, &c. &c
Buffon, Georges Louis Leclerc, comte de
Natural history
However inconsiderable the 650th part may be, yet it certainly at first
appears to require a very powerful comet to separate even that much
from the body of the sun; but if we reflect on the prodigious velocity
of comets in their perihelion, a velocity so much the greater as they
approach nearer the sun; if, besides, we pay attention to the density
and solidity of the matter of which they must be composed, to suffer,
without being destroyed, the inconceivable heat they endure; and
consider the bright and solid light which shines through their dark and
immense atmospheres, which surround, and must obscure them, it cannot be
doubted that the comets are composed of extremely solid and dense
matters, and that they contain a greater quantity of matter in a small
compass; that consequently a comet of no extraordinary bulk may have
sufficient weight and velocity to displace the sun, and give a
projectile motion to a quantity of matter, equal to the 650th part of
the mass of this luminary. This perfectly agrees with what is known
concerning the density of planets, which always decreases as their
distance from the sun is increased, they having less heat to support; so
that Saturn is less dense than Jupiter, and Jupiter much less than the
earth; therefore if the density of the planets be, as Newton asserts,
proportionable to the quantity of heat which they have to support,
Mercury will be seven times more dense than the earth, and twenty-eight
times denser than the sun; and the comet of 1680 would be 28,000 times
denser than the earth, or 112,000 times denser than the sun, and by
supposing it as large as the earth, it would contain nearly an equal
quantity of matter to the ninth part of the sun, or by giving it only
the 100th part of the size of the earth, its mass would still be equal
to the 900th part of the sun. From whence it is easy to conclude, that
such a body, though it would be but a small comet, might separate and
drive off from the sun a 900th or a 650th part, particularly if we
attend to the immense velocity with which comets move when they pass in
the vicinity of the sun.
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