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
The case of a star suddenly blazing forth and then fading away, such as
that observed by Tycho Brahe in 1572, may be accounted for by supposing
that the star had been struck by one of the dark bodies—an event not at
all impossible, or even improbable. In some cases of sudden outbursts,
such as that of Nova Cygni, for example, the phenomenon may result from
the star encountering a swarm of meteorites. The difficulty in the case
of Nova Cygni is to account for the very sudden decline of its
brilliancy. This might, however, be explained by supposing that the
outburst of luminosity was due to the destruction of the meteorites, and
not to any great increase of heat produced in the star itself. A swarm
of meteorites converted into incandescent vapour would not be long in
losing its brilliancy.
Mr. Lockyer thinks that the outburst was produced by the collision of
two swarms of meteorites, and not by the collision of the meteorites
with a previously existing star.[20]
[Footnote 20: _Proceedings of the Royal Society_, vol. xliii. p. 140.]
Amongst the millions of stars occupying stellar space catastrophes of
this sort may, according to the theory, be expected sometimes to happen,
although, like the collisions which originate stars themselves, they
must, doubtless, be events of but rare occurrence.
VIII. _Star Clusters._
A star cluster will result from an immensely widespread nebula breaking
up into a host of separate nuclei, each of which becomes a star. The
irregular manner in which the materials would, in many cases, be widely
distributed through space after collision would prevent a nebula from
condensing into a single mass. Subordinate centres of attraction would
be established, as was long ago shown by Sir William Herschel in his
famous memoir on the formation of stars;[21] and around these the
gaseous particles would arrange themselves and gradually condense into
separate stars, which would finally assume the condition of a cluster.
[Footnote 21: _Philosophical Transactions_ for 1811.]
IX. _Age of the Sun’s Heat: a Crucial Test._
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