A History of Science — Volume 3Williams, Henry Smith
History
A History of Science — Volume 3
Williams, Henry Smith
Science -- History
"That the Milky Way is a most extensive stratum of stars of various
sizes admits no longer of lasting doubt," he declares, "and that our sun
is actually one of the heavenly bodies belonging to it is as evident. I
have now viewed and gauged this shining zone in almost every direction
and find it composed of stars whose number... constantly increases and
decreases in proportion to its apparent brightness to the naked eye.
"Let us suppose numberless stars of various sizes, scattered over an
indefinite portion of space in such a manner as to be almost equally
distributed throughout the whole. The laws of attraction which no doubt
extend to the remotest regions of the fixed stars will operate in such a
manner as most probably to produce the following effects:
"In the first case, since we have supposed the stars to be of various
sizes, it will happen that a star, being considerably larger than its
neighboring ones, will attract them more than they will be attracted by
others that are immediately around them; by which means they will be,
in time, as it were, condensed about a centre, or, in other words, form
themselves into a cluster of stars of almost a globular figure, more
or less regular according to the size and distance of the surrounding
stars....
"The next case, which will also happen almost as frequently as the
former, is where a few stars, though not superior in size to the rest,
may chance to be rather nearer one another than the surrounding ones,...
and this construction admits of the utmost variety of shapes....
"From the composition and repeated conjunction of both the foregoing
formations, a third may be derived when many large stars, or combined
small ones, are spread in long, extended, regular, or crooked rows,
streaks, or branches; for they will also draw the surrounding stars, so
as to produce figures of condensed stars curiously similar to the former
which gave rise to these condensations.
"We may likewise admit still more extensive combinations; when, at the
same time that a cluster of stars is forming at the one part of
space, there may be another collection in a different but perhaps not
far-distant quarter, which may occasion a mutual approach towards their
own centre of gravity.
"In the last place, as a natural conclusion of the former cases, there
will be formed great cavities or vacancies by the retreating of the
stars towards the various centres which attract them."(1)
Looking forward, it appears that the time must come when all the suns
of a system will be drawn together and destroyed by impact at a common
centre. Already, it seems to Herschel, the thickest clusters have
"outlived their usefulness" and are verging towards their doom.
Public-domain text, read in full here on John Shaqi.
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