Stellar Evolution and Its Relations to Geological TimeCroll, James
Science
Stellar Evolution and Its Relations to Geological Time
Croll, James
Cosmogony; Geological time; Stars -- Evolution
As regards the theory we are discussing, it is the same which
alternative is taken, for both are equally favourable. If the former,
then, according to the theory that stellar heat had its origin in
collision, it is presumptive evidence that space is occupied by dark
bodies far more numerous and massive than the luminous ones which the
telescope reveals. If the latter, viz. that the star has a velocity
which never could have been produced by attraction, “then,” as says
Professor Newcomb, “it must have been flying forward through space from
the beginning, and, having come from an infinite distance, must now be
passing through our system for the first and only time.” The probability
is, however, that the star derived its motion from the source from which
it derived its light and heat; namely, from the collision of the two
masses out of which it arose. If the star is ever to be arrested in its
onward course, it must be by collision; but such an event would be its
final end.
There are other stars, such as 61 Cygni, ε Indi, Lalande 21258, Lalande
21185, μ Cassiopeiæ, and Arcturus, possessed of motions which could not
have been derived from gravity. And there are probably many more of
which, owing to their enormous distances, the proper motions have not
been detected. α Centauri, the nearest star in the heavens, by less than
one-half, is distant twenty-one millions of millions of miles; and there
are, doubtless, many visible stars a thousand times more remote. A star
at this distance, though moving transversely to the observer at the
enormous rate of 100 miles per second, would take upwards of thirty
years to change its position so much as one second, and consequently
1,800 years to change its position one minute. In fact, we should have
to watch the star for a generation or two before we could be certain
whether it was moving or not.
IV. _Probable Origin of Comets._
Public-domain text, read in full here on John Shaqi.
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