The usual way of treating the solar system has been to suppose it
to have been formed out of a nebula extending far beyond the planet
Neptune, generally in a vague way; although some writers have specified
a limit to the distance, in order to give some definite idea of what
must have been the density of the nebula at some particular period
of its existence. In the first part of our work we have adopted the
same plan and we mean to follow it out, because it gives us a greater
degree of facility for expressing our ideas, and making them more
intelligible, than by adopting a new method. But we shall previously
endeavour to show where the nebula itself came from and how it was
formed, which seems to us to be as necessary as to show how it was
transformed into the solar system.
We understand Laplace to have supposed the nebula to have been formed
out of cosmic matter in its simplest condition, and in its most
primitive atomic state, collected from enormously distant regions
of space by the power or law of attraction. In this we shall follow
him, because we do not see the necessity for matter having to be
created in the form of meteorites or meteors, or any other form, to
be afterwards dissociated and reduced to the atomic state, by heat
produced by collisions amongst the dissociated atoms. Surely it would
show more prescience, more simplicity of work, and economy of labour,
to create matter in this primitive state, than in one which required
it to be passed through a mill of some kind, as it were, before it
was manufactured into nebulous matter; in fact, to make brickbats in
order that they should be afterwards ground down--dissociated--into
impalpable powder, to render them fit to be worked up into bricks. But
our first effort will be to attempt to define the collecting grounds
of this cosmic matter, somewhat more particularly than has been done
hitherto, as we believe that even a superficial study of them will
assist us greatly in forming a more comprehensive idea of the whole
solar system than anything we have met with in any of the books which
we have had the opportunity of applying to for information.
Public-domain text, read in full here on John Shaqi.
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