Meteoric astronomy: A treatise on shooting-stars, fire-balls, and aerolitesKirkwood, Daniel
Science
Meteoric astronomy: A treatise on shooting-stars, fire-balls, and aerolites
Kirkwood, Daniel
Meteors
successively by its attraction all the others about its center, the
ring of vapors would be changed into one spheroidal mass, circulating
about the sun, with a motion of rotation in the same direction with
that of revolution."[33] Such, according to the theory of Laplace, is
the history of the formation of the most remote planet of our system.
That of every other, both primary and secondary, would be precisely
similar.
In support of the nebular hypothesis, of which the foregoing is a
brief general statement, we remark that _it furnishes a very simple
explanation of the motions and arrangements of the planetary system_.
In the first place, it is evident that the separation of a ring would
take place at the equator of the revolving mass, where of course the
centrifugal force would be greatest. These concentric rings--and
consequently the resulting planets--would all revolve _in nearly the
same plane_. It is evident also that the central body must have a
revolution on its axis _in the same direction with the progressive
motion of the planets_. Again: at the breaking up of a ring, the
particles of nebulous matter more distant from the sun would have
a greater absolute velocity than those nearer to it, which would
produce the observed _unity of direction in the rotary and orbital
revolutions_. The motions of the satellites are explained in like
manner. The hypothesis, moreover, accounts satisfactorily for the fact
that the orbits of the planets are all nearly circular. And finally,
it presents an obvious explanation of the rings of Saturn. It would
almost seem, indeed, as if these wonderful annuli had been left by the
Architect of Nature, as an index to the creative process.
The argument derived from the motions of the various members of the
solar system is not new, having been forcibly stated by Laplace,
Pontécoulant, Nichol, and other astronomers. Its full weight and
importance, however, have not, we think, been duly appreciated. That a
common physical cause has determined these motions, must be admitted
by every philosophic mind. But apart from the nebular hypothesis,
no such cause, adequate both in mode and measure, has ever been
suggested;--indeed none, it seems to us, is conceivable. The phenomena
which we have enumerated _demand_ an explanation, and this demand
is met by the nebular hypothesis. It will be found, therefore, when
closely examined, that the evidence afforded by the celestial motions
is sufficient to give the theory of Laplace a very high degree of
probability.
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