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
None of these facts are accounted for by the law of gravitation. The
sun's attraction can have no influence whatever in determining either
the _direction_ of a planet's motion, or the eccentricity of its orbit.
In other words, this power would sustain a planetary body moving from
east to west, as well as from west to east; in an orbit having any
possible degree of inclination to the plane of the sun's equator, no
less than in one coincident with it; or, in a very eccentric ellipse,
as well as in one differing but little from a circle. The consideration
of the coincidences which we have enumerated led Laplace to conclude
that their explanation must be referred to the _mode_ of our system's
formation--a conclusion which he regarded as strongly confirmed by
the contemporary researches of Sir William Herschel. Of the numerous
nebulæ discovered and described by that eminent observer, a large
proportion could not, even by his powerful telescope, be resolved into
stars. In regard to many of these, it was not doubted that glasses
of superior power would show them to be extremely remote sidereal
clusters. On the other hand, a considerable number were examined which
gave no indications of resolvability. These were supposed to consist
of self-luminous, nebulous matter--the chaotic elements of future
stars. The great number of these irresolvable nebulæ scattered over
the heavens and apparently indicating the various stages of central
condensation, very naturally suggested the idea that the solar system,
and perhaps every other system in the universe, originally existed
in a similar state. The sun was supposed by Laplace to have been an
exceedingly diffused, rotating nebula, of spherical or spheroidal
form, extending beyond the orbit of the most distant planet; the
planets as yet having no separate existence. This immense sphere of
vapor, in consequence of the radiation of heat and the continual
action of gravity, became gradually more dense, which condensation was
necessarily attended by an increased angular velocity of rotation. At
length a point was thus reached where the centrifugal force of the
equatorial parts was equal to the central attraction. The condensation
of the interior meanwhile continuing, the equatorial zone was detached,
but necessarily continued to revolve around the central mass with
the same velocity that it had at the epoch of its separation. If
perfectly uniform throughout its entire circumference, which would be
highly improbable, it would continue its motion in an unbroken ring,
like that of Saturn; if not, it would probably collect into several
masses, having orbits nearly identical. "These masses should assume a
spheroidal form, with a rotary motion in the direction of that of their
revolution, because their inferior articles have a less real velocity
than the superior; they have therefore constituted so many planets in a
state of vapor. But if one of them was sufficiently powerful to unite
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