Astronomy of To-day: A Popular Introduction in Non-Technical LanguageDolmage, Cecil Goodrich Julius
Science
Astronomy of To-day: A Popular Introduction in Non-Technical Language
Dolmage, Cecil Goodrich Julius
Astronomy
If comets are really undoubted members of the solar system, the
circumstances in which they were evolved must have been different from
those which produced the planets and satellites. The axial rotations of
both the latter, and also their revolutions, take place in one certain
direction;[24] their orbits, too, are ellipses which do not differ much
from circles, and which, furthermore, are situated fairly in the one
plane. Comets, on the other hand, do not necessarily travel round the
sun in the same fixed direction as the planets. Their orbits, besides,
are exceedingly elliptic; and, far from keeping to one plane, or even
near it, they approach the sun from all directions.
Broadly speaking, comets may be divided into two distinct classes, or
"families." In the first class, the same orbit appears to be shared in
common by a series of comets which travel along it, one following the
other. The comets which appeared in the years 1668, 1843, 1880, 1882,
and 1887 are instances of a number of different bodies pursuing the same
path around the sun. The members of a comet family of this kind are
observed to have similar characteristics. The idea is that such comets
are merely portions of one much larger cometary body, which became
broken up by the gravitational action of other bodies in the system, or
through violent encounter with the sun's surroundings.
The second class is composed of comets which are supposed to have been
seized by the gravitative action of certain planets, and thus forced to
revolve in short ellipses around the sun, well within the limits of the
solar system. These comets are, in consequence, spoken of as "captures."
They move around the sun in the same direction as the planets do.
Jupiter has a fairly large comet family of this kind attached to him. As
a result of his overpowering gravitation, it is imagined that during the
ages he must have attracted a large number of these bodies on his own
account, and, perhaps, have robbed other planets of their captures. His
family at present numbers about thirty. Of the other planets, so far as
we know, Saturn possesses a comet family of two, Uranus three, and
Neptune six. There are, indeed, a few comets which appear as if under
the influence of some force situated outside the known bounds of the
solar system, a circumstance which goes to strengthen the idea that
other planets may revolve beyond the orbit of Neptune. The terrestrial
planets, on the other hand, cannot have comet families; because the
enormous gravitative action of the sun in their vicinity entirely
overpowers the attractive force which they exert upon those comets which
pass close to them. Besides this, a comet, when in the inner regions of
the solar system, moves with such rapidity, that the gravitational pull
of the planets there situated is not powerful enough to deflect it to
any extent. It must not be presumed, however, that a comet once captured
should always remain a prisoner. Further disturbing causes might
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