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
“But in course of time some process akin to cooling, probably internal,
reduces the temperature of the cosmic _protyle_ to a point at which the
first step in granulation takes place; matter as we know it comes into
existence, and atoms are formed. As soon as an atom is formed out of
_protyle_ it is a store of energy, potential (from its tendency to
coalesce with other atoms by gravitation or chemically) and kinetic
(from its internal motions). To obtain this energy, the neighbouring
_protyle_ must be refrigerated by it, and thereby the subsequent
formation of other atoms will be accelerated. But with atomic matter the
various forms of energy which require matter to render them evident
begin to act; and, amongst others, that form of energy which has for one
of its factors what we now call _atomic weight_. Let us assume that the
elementary _protyle_ contains within itself the potentiality of every
possible combining proportion or atomic weight. Let it be granted that
the whole of our known elements were not at this epoch simultaneously
created. The easiest formed element, the one most nearly allied to the
_protyle_ in simplicity, is first born. Hydrogen—or shall we say
helium?—of all the known elements the one of simplest structure and
lowest atomic weight, is the first to come into being. For some time
hydrogen would be the only form of matter (as we know it) in existence,
and between hydrogen and the next formed element there would be a
considerable gap in time, during the latter part of which the element
next in order of simplicity would be slowly approaching its birth-point:
pending this period we may suppose that the evolutionary process, which
soon was to determine the birth of a new element, would also determine
its atomic weight, its affinities, and its chemical position.”
_Professor F. W. Clarke on the pre-nebular condition of matter._—Views
on elemental evolution almost similar to those of Mr. Crookes’s have
been advocated by Professor Clarke. Spectroscopic phenomena, says
Professor Clarke, are quite in harmony with the idea that all matter is
at bottom one, our supposed atoms being really various aggregations of
the same fundamental unit.
Public-domain text, read in full here on John Shaqi.
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