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
6. _The gaseous condition essential to the nebular hypothesis._—It is
found that the density of the interior planets of our solar system
compared with that of the more remote is about as five to one. The
obvious conclusion is that there is a preponderance of the metallic
elements in the interior planets and of metalloids in the exterior. It
thus becomes evident, as Mr. Lockyer has so clearly shown,[16] that when
our solar system existed in a nebulous condition the metallic or denser
elements would occupy the interior portion of the nebula and the
metalloids the exterior. Taking a section of this nebula from its centre
to its circumference, the elements would in the main be found arranged
according to their densities: the densest at the centre, and the least
dense at the circumference. If we compare the planets with their
satellites, we find the same law holding true. The satellites of
Jupiter, for example, have a density of about only one-fifth of that of
the planet, or about one twenty-fifth of that of our earth, showing that
when the planet was rotating as a nebulous mass the more dense elements
were in the central parts and the less dense at the outer rim, where the
satellites were being formed. Again, if we take the case of our globe,
we find, as Mr. Lockyer remarks, the same distribution of materials,
proving that when the earth was in the nebulous state the metallic
elements chiefly occupied the central regions, and the metalloids those
outer parts which now constitute the earth’s crust.
[Footnote 16: _Manchester Science Lectures._]
All these facts show that the _sifting_ and _sorting_ of the chemical
elements according to their densities must have taken place when our
solar system was in the condition of a nebula. But, further, it seems
impossible that this could have taken place had the materials composing
the nebula been in the solid form, even supposing that they had taken
the form of clouds of stones.
It is equally impossible that the nebula could have been in the fluid or
liquid state during this process. This is obvious, for the nebula must
then have occupied, at least, the entire space within the orbit of the
most remote planet. But our solar system in the liquid condition could
not occupy one-millionth part of that space. It is therefore evident
that the nebula must have been in the state of a gas, and a gas of
extreme tenuity.
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