Worlds in the making: The evolution of the universe — John Shaqi
Worlds in the making: The evolution of the universeArrhenius, Svante
Science
Worlds in the making: The evolution of the universe
Arrhenius, Svante
Cosmogony
The opinion that all the solar heat radiated into infinite space is
wasted, starts moreover from a hypothesis which is not proved, and
which is highly improbable—namely, that only an extremely small
portion of the sky is covered with celestial bodies. That might
certainly be correct if we assumed, as has formerly been done, that
the majority of the celestial bodies must be luminous. We do not
possess, however, any reliable knowledge of the number and size of the
dark celestial bodies. In order to account for the observed movements
of different stars, it has been thought that there must be in the
neighborhood of some of them dark stars of enormous size whose masses
would surpass the mass of our sun, or, at least, be equal to it. But
the largest number of the dark celestial bodies which hide the rays
from the stars behind them probably consist of smaller particles,
such as we observe in meteors and in comets, and to a large extent of
so-called cosmical dust. The observations of later years, by the aid
of most powerful instruments, have shown that so-called nebulæ and
nebulous stars abound throughout the heavens. In their interior we
should probably find accumulations of dark masses.
The light intensity of most of the nebulæ is, moreover, far too weak to
permit of their being perceived. We have, therefore, to imagine that
there are bodies all through infinite space, and about as numerous as
they are in the immediate neighborhood of our solar system. Thus every
ray from the sun, of whatever direction, would finally hit upon some
celestial body, and nothing would be lost of the solar radiation, nor
of the stellar radiation.
As regards the radiation-heat exchange, the earth might be likened to
a steam-engine. In order that the steam-engine shall perform useful
work, it is necessary not only that the engine be supplied with heat
of high temperature from a furnace and a boiler, but also that the
engine be able to give its heat up again to a heat reservoir of lower
temperature—a condenser or cooler. It is only by transferring heat
from a body of higher temperature to another body of lower temperature
that the engine can do work. In a similar way no work can be done on
the earth, and no life can exist, unless heat be conferred by the
intermediation of the earth from a hot body, the sun, to the colder
surroundings of universal space—_i.e._, to the cold celestial bodies
in it.
To a certain extent the temperature of the earth’s surface, as we shall
presently see, is conditional by the properties of the atmosphere
surrounding it, and particularly by the permeability of the latter for
the rays of heat.
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