SP-345 Evolution of the Solar
System
FIGURE 24.3.2.- Number of bodies in a
satellite group is a function of
(where
is the spin period of the central body and
Tion is a
characteristic orbital period of the bodies in the group (sec.
23.5)). The groups of satellites are the outermost Saturnian
satellites (Saturnian D cloud), Galilean satellites (Jovian C cloud), Uranian
satellites (Uranian D cloud), inner Saturnian satellites (Saturnian
C
cloud), and innermost Jovian satellites (Jovian B cloud). Assuming that
the Earth's satellite system would fall into the pattern established
by these groups of satellites, the Earth may once have had just a few
or as many as 9 or 10 normal satellites. (From Alfvén and
Arrhenius, 1972a.)
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