A History of Science — Volume 3Williams, Henry Smith
History
A History of Science — Volume 3
Williams, Henry Smith
Science -- History
"Buffon is the only man I know who, since the discovery of the true
system of the world, has endeavored to show the origin of the planets
and their satellites. He supposes that a comet, in falling into the sun,
drove from it a mass of matter which was reassembled at a distance in
the form of various globes more or less large, and more or less removed
from the sun, and that these globes, becoming opaque and solid, are now
the planets and their satellites.
"This hypothesis satisfies the first of the five preceding phenomena;
for it is clear that all the bodies thus formed would move very nearly
in the plane which passed through the centre of the sun, and in the
direction of the torrent of matter which was produced; but the four
other phenomena appear to be inexplicable to me by this means. Indeed,
the absolute movement of the molecules of a planet ought then to be in
the direction of the movement of its centre of gravity; but it does not
at all follow that the motion of the rotation of the planets should be
in the same direction. Thus the earth should rotate from east to west,
but nevertheless the absolute movement of its molecules should be
from east to west; and this ought also to apply to the movement of the
revolution of the satellites, in which the direction, according to the
hypothesis which he offers, is not necessarily the same as that of the
progressive movement of the planets.
"A phenomenon not only very difficult to explain under this hypothesis,
but one which is even contrary to it, is the slight eccentricity of the
planetary orbits. We know, by the theory of central forces, that if
a body moves in a closed orbit around the sun and touches it, it also
always comes back to that point at every revolution; whence it follows
that if the planets were originally detached from the sun, they would
touch it at each return towards it, and their orbits, far from being
circular, would be very eccentric. It is true that a mass of matter
driven from the sun cannot be exactly compared to a globe which touches
its surface, for the impulse which the particles of this mass receive
from one another and the reciprocal attractions which they exert among
themselves, could, in changing the direction of their movements, remove
their perihelions from the sun; but their orbits would be always most
eccentric, or at least they would not have slight eccentricities except
by the most extraordinary chance. Thus we cannot see, according to
the hypothesis of Buffon, why the orbits of more than a hundred comets
already observed are so elliptical. This hypothesis is therefore
very far from satisfying the preceding phenomena. Let us see if it is
possible to trace them back to their true cause.
Public-domain text, read in full here on John Shaqi.
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