Nos. 7 and 8. In these paragraphs, the main features are repetitions of
the simple assertions made in all the others, that certain movements
possessed by matter in one state would produce other movements in
another state, without attempting to show how they all came to so
far coincide with each other and form one harmonious whole, with
movements in almost one single direction. It is clear that one side
of the separated chaos might have acquired motion in one direction
from the universal chaos with which it had been in contact, and that
the opposite side might have acquired motion in exactly the opposite
direction from the original chaos with which it had been in contact;
and we are left to find out how these came to agree with each other
in the end. And, going back to the beginning, we are left to find out
where the mass, out of which he constructs his solar system, was stowed
away, after it was separated from the original universal chaos. We
can conceive of its being separated by condensation, in obedience to
the law of attraction, from the surrounding chaos, in which case it
might fall towards a centre, or that some parts of it might come to
revolve round each other, and that finally the whole of these parts
might come to rotate about a common centre; but that is evidently very
different from the mode of formation of the solar system which M. Faye
has advocated. It comes to be by far too like the nebula which Laplace
supposed to be endowed with rotary motion from the beginning, probably
because he did not see, or did not take the trouble to see, how such
a motion could be produced. In any case, Laplace did not consider
that the primary motion of rotation was the most important part of
his hypothesis; neither was it, as it seems to have been in the case
we have been considering. And he did not go much further than M. Faye
in postulating primary motion, only he did it in a more effectual and
business-like manner. He drew on the bank at once for all the funds he
required, instead of having to draw afresh every time he found himself
in difficulties, as has been the lot of his critic and successor.
Public-domain text, read in full here on John Shaqi.
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