Stellar Evolution and Its Relations to Geological Time — John Shaqi
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
7. _The mass must have possessed an excessive temperature._—There is
ample evidence, Mr. Lockyer thinks, to show that the temperature of the
solar nebula was as great as that of the sun at the present time. But I
think it is extremely probable that, in some of its stages, the nebula
had a very much higher temperature than that now possessed by the sun.
There must, during the sifting period, have been complete chemical
dissociation, so as to keep the metals and the metalloids uncombined,
and thus allow the elements to arrange themselves according to their
densities. The nebula hypothesis, remarks Mr. Lockyer, “is almost
worthless unless we assume very high temperatures, because, unless you
have heat enough to get perfect dissociation, you will not have that
sorting out which always seems to follow the same law.”
8. _Gravitation could, under no possible condition, have generated the
amount of heat required by the nebular hypothesis._—The nebular
hypothesis does not profess to account for the origin of nebulæ. It
starts with matter existing in space in the nebulous condition, and
explains how, by condensation, suns, planets &c. are formed out of it.
In fact, it begins at the middle of a process: it begins with this fine,
attenuated material in the process of being drawn together and condensed
under the influence of attraction, and professes to explain how, as the
process goes on, a solar system necessarily results. To simplify our
inquiry we shall confine our attention to the solar nebula, and consider
in the first place how far condensation may be regarded as a sufficient
source of heat.
A. _Condensation._—The heat which our nebula could have derived from
condensation up to the time that Neptune was detached from the mass, no
matter how far the outer circumference of the mass may have originally
extended beyond the orbit of that planet, could not have amounted to
over 1/7,000,000 of a thermal unit (772 foot-pounds) for each cubic
foot. It is perfectly obvious that this amount could not have produced
the dissociation required; and without the required dissociation Neptune
could never have been formed. Further, it is physically impossible that
the materials of which our solar system are composed could have existed
in the gaseous state in a cool condition prior to condensation. Unless
possessed of great heat, even hydrogen could not exist in stellar space
in the gaseous form; and far less could carbon, iron, platinum, &c.
Before Neptune could have been formed the whole of the materials of the
system must have possessed heat, not only sufficient to reduce them to
the gaseous state, but sufficient to produce complete dissociation. But
by no conceivable means could gravitation have conferred this amount of
heat by the time that the mass had condensed to just within the limits
of the orbit of Neptune.
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