A Text-Book of AstronomyComstock, George C. (George Cary)
Science
A Text-Book of Astronomy
Comstock, George C. (George Cary)
Astronomy
239. ROCHE'S LIMIT.--In looking forward to such a catastrophe, however,
due regard must be paid to a dynamical principle of a different
character. The moon can never be precipitated upon the earth entire,
since before it reaches us it will have been torn asunder by the excess
of the earth's attraction for the near side of its satellite over that
which it exerts upon the far side. As the result of Roche's mathematical
analysis we are able to assign a limiting distance between any planet
and its satellite within which the satellite, if it turns always the
same face toward the planet, can not come without being broken into
fragments. If we represent the radius of the planet by _r_, and the
quotient obtained by dividing the density of the planet by the density
of the satellite by _q_, then
Roche's limit = 2.44 r ∛q.
Thus in the case of earth and moon we find from the densities given in
§ 95, _q_ = 1.65, and with _r_ = 3,963 miles we obtain 11,400 miles as
the nearest approach which the moon could make to the earth without
being broken up by the difference of the earth's attractions for its
opposite sides.
We must observe, however, that Roche's limit takes no account of
molecular forces, the adhesion of one molecule to another, by virtue of
which a stick or stone resists fracture, but is concerned only with the
gravitative forces by which the molecules are attracted toward the
moon's center and toward the earth. Within a stone or rock of moderate
size these gravitative forces are insignificant, and cohesion is the
chief factor in preserving its integrity, but in a large body like the
moon, the case is just reversed, cohesion plays a small part and
gravitation a large one in holding the body together. We may conclude,
therefore, that at a proper distance these forces are capable of
breaking up the moon, or any other large body, into fragments of a size
such that molecular cohesion instead of gravitation is the chief agent
in preserving them from further disintegration.
240. SATURN'S RINGS.--Saturn's rings are of peculiar interest in this
connection. The outer edge of the ring system lies just inside of
Roche's limit for this planet, and we have already seen that the rings
are composed of small fragments independent of each other. Whatever may
have been the process by which the nine satellites of Saturn came into
existence, we have in Roche's limit the explanation why the material of
the ring was not worked up into satellites; the forces exerted by Saturn
would tear into pieces any considerable satellite thus formed and
equally would prevent the formation of one from raw material.
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