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
It will be observed, in reference to the theories we have just
considered, that the process of evolution is supposed to take place from
the smaller to the larger aggregates of matter. Beginning with an
extreme condition of tenuity, by aggregation, the materials become
successively larger and more complex. In passing backwards in the
process we find the aggregates becoming less and less till they reach
the “cosmical dust,” or “fire-mist,” out of which the primitive nebulæ
were supposed to be formed. Receding still farther back, we have the
universal atmosphere from which the fire-mist is assumed to have been
derived.
This universal atmosphere, though in a state of extreme tenuity, is, as
we shall see, supposed by some to be in a more elemental form than
anything revealed to us in the laboratory. The suggestion of the
dissociation of the chemical elements and its application to stellar
physics was, I think, first advanced by Sir Benjamin Brodie in 1866, and
more fully in 1867. In the latter year views similar were considered
more fully by Dr. T. Sterry Hunt. The question of the dissociation of
elements has been ably discussed by Mr. Lockyer in his various writings.
It has been suggested by Mr. Lockyer that the coincidence of rays
emitted by different chemical elements when subjected to very high
temperatures affords evidence of a common element in the composition of
the metals producing the coincident rays. Mr. Lockyer states that many
trains of thought suggested by solar and stellar physics point to the
hypothesis that the _elements themselves, or at all events some of them,
are compound bodies_.[67] This view was also put forward by Professor
Graham, who says “that it is conceivable that the various kinds of
matter now recognised in different elementary substances may possess one
and the same element or atomic molecule existing in different conditions
of mobility. The essential unity of matter,” he adds, “is an hypothesis
in harmony with the equal action of gravity upon all bodies.” Similar
views have been advocated by M. Dumas, who based the suggestion of the
composite nature of the elementary atoms on certain relations of atomic
weights. The composite nature of the chemical elements has also been
maintained by Henri Sainte-Claire Deville, and also by Berthelot, who
held that the atoms of the elements are the same, and distinguished only
by their modes of motion. Professor Schuster, in a paper read before the
British Association in 1880, supports the view of the dissociation of
the chemical elements.
[Footnote 67: _Proc. Roy. Soc._ vol. xxviii. p. 160.]
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