Worlds in the making: The evolution of the universeArrhenius, Svante
Science
Worlds in the making: The evolution of the universe
Arrhenius, Svante
Cosmogony
The masses of gas within the nebulæ form the most important centres of
concentration of the dust which is ejected from the sun and stars.
If the world were limited, as people used to fancy—that is to say,
if the stars were crowded together in a huge heap, and only infinite,
empty space outside of this heap, the dust particles ejected from the
suns during past ages by the action of the radiating pressure would
have been lost in infinite space, just as we imagined that the radiated
energy of the sun was lost.
If that were so, the development of the universe would long since
have come to an end, to an annihilation of all matter and of all
energy. Herbert Spencer, among others, has explained how thoroughly
unsatisfactory this view is. There must be cycles in the evolution of
the universe, he has emphasized. That is manifestly indispensable if
the system is to last. In the more rarefied, gaseous, cold portions of
the nebulæ we find that part of the machinery of the universe which
checks the waste of matter and, still more, the waste of force from
the suns. The immigrating dust particles have absorbed the radiation
of the sun and impart their heat to the separate particles of the
gases with which they collide. The total mass of gas expands, owing to
this absorption of heat, and cools in consequence. The most energetic
molecules travel away, and are replaced by new particles coming from
the inner portions of the nebulæ, which are in their turn cooled by
expansion. Thus every ray emitted by a sun is absorbed, and its energy
is transferred, through the gaseous particles of the nebulæ, to suns
that are being formed and which are in the neighborhood of the nebula
or in its interior portions. The heat is hence concentrated about
centres of attraction that have drifted into the nebula or about the
remnants of the celestial bodies which once collided there. Thanks to
the low temperature of the nebula, the matter can again accumulate,
while the radiation pressure, as Poynting has shown, will suffice
to keep bodies apart if their temperature is 15° C., their diameter
3.4 cm., and their specific gravity as large as that of the earth,
5.5. At the distance of the orbit of Neptune, where the temperature
is about 50° absolute and approximates, therefore, that of a nebula,
this limit of size is reduced to nearly one millimetre. It has already
been suggested (compare page 153) that capillary forces, which would
prevail under the co-operation of the gases condensed upon the dust
grains, rather than gravity, play a chief part in the accumulation
and coalescence of the small particles. In the same manner as matter
is concentrated about centres of attraction energy may be accumulated
there in contradiction to the law of the constant increase of entropy.
Public-domain text, read in full here on John Shaqi.
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