398
The Solar System [ch. xvi
The matter which was first shed by the sun would form a ring of small
mass rotating with the sun ; on account of the smallness of its mass, this would
have no gravitational cohesion and, so far from increasing in density, would
scatter under its own internal gaseous pressure. It seems impossible that such
a ring could double its density before the disruptive influence of its rotation
could come into play. Thus, on the whole, it seems necessary to admit Babinet’s
contention that the solar system is not possessed of sufficient angular
momentum to have broken up through excessive rotation*. The calculation
needs some modification in view of the possibility discussed in Chapter x of
the inner layers of the sun rotating faster than the outer, but the modification
is found to make rotational break-up still more impossible.
371 . The considerations which carry the most obvious condemnation of the
theory of rotational break-up are of a somewhat different kind. If the sun
once assumed the lenticular shape necessary for the shedding of matter by
rotation, it is difficult to see how it could ever abandon it and become as
nearly spherical as it now is ; it is also difficult to understand why the planets
should be at such widely varying distances from the sun.
These as well as other difficulties again confront the rotational theory
when it attempts to explain the origin of the satellites of the planets. Many
of these are so small that they can only have escaped scattering into space by
liquefying or solidifying immediately after their birth. Thus their birth can
not have been a long drawn out process such as the equatorial shedding of
matter by a slowly shrinking mass ; the fact that these satellites survived the
birth-process at all proves that they must have been born quickly.
Tidal Theories.
372 . As the genesis of the solar system cannot be explained in terms of
a single mass rotating by itself in space, the only alternative which remains
is to consider whether it can be explained as the result of the interaction of
two or more masses. We can fix our attention on two, since encounters of
three masses in space must be so rare as to be entirely unimportant.
This brings us naturally and inevitably to tidal theories of the genesis
of the solar system. The fundamental conception of these theories is, that at
some time in the past a second mass approached so close to our sun as to break
it up, through the action of intense tidal forces, into a number of detached
masses.
As between rotational and tidal theories, first appearances are wholly in
favour of the latter. A rotating mass, and so also a system which has been
formed without external interference out of a rotating mass, retains one
* This argument was first given by myself in M.N. lxxvii. (1917), p. 186. Jeffreys has re
investigated the question in M.N. lxxviii. (1918), p. 425, slightly modifying the argument, but
confirming my original conclusions.