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
_Mr. Charles Morris on the pre-nebular condition of matter._—Others
again suppose matter to be present everywhere throughout space. This
view has been ingeniously advocated by Mr. Charles Morris in an article
on “The Matter of Space,” which appeared in _Nature_, February 8, 1883.
The hypothesis of an ether specially distinct from matter he considers
to be a gratuitous assumption, and one of the last surviving relics of
eighteenth century science, and, unless it can be proved that highly
disintegrated matter is positively incapable of conveying light
vibrations, there is no warrant for assigning this duty to a distinct
form of substance. But that matter exists in outer space in the same
conditions as in planetary atmospheres he thinks is improbable. Its duty
as a conveyer of radiant vibrations seems to require a far greater
tensity, and its disintegration is probably extreme. Assuming matter
throughout the universe—here as condensed spheres, and there in outer
space as highly rarified substance—the atmospheric envelopes of the
spheres, he considers, will gradually shade off into the excessively
rare matter of mid-space. Matter may exist in countless conditions as to
simplicity and complexity, &c., but the base particle he assumes to be
the same under all conditions. In the spheres there is matter ranging
from the simplest elementary gases, through the mineral compounds of the
solid surface, to the highly compounded organic molecules. In outer
space the variation is in the opposite direction; the matter existing
there in a highly disintegrated condition.
Every particle he considers to possess a certain amount of motor energy
in the form of heat. As the total amount of this energy in the universe
remains unchanged, a particle can only lose energy by transferring it to
others. This heat energy acts, of course, in opposition to gravity: it
tends to repel the particles from each other, while gravity, on the
other hand, tends to draw them together. The former acts as a
centrifugal, the latter as a centripetal energy. If the heat momentum of
the particles be insufficient to constitute a centrifugal energy equal
to the centripetal energy of gravitation, then the material contents of
space will be drawn into the attracting spheres as atmospheric
substance, and outer space, in this case, will be left destitute of
matter. If, on the contrary, the centrifugal energy of the particles be
sufficient to resist gravitation, then the particles will remain free,
and space will continue to be occupied with matter. As has been stated,
the sum of motor energy in the universe remaining unchanged, the
aggregation of atmospheric substance around any planet resulting from
the loss of motor energy must cause an increase of motor energy in the
particles outside.
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