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
We might think that we could not possibly learn anything concerning
the condition of those strata. Earthquakes have, however, supplied us
with a little information. Such gaseous masses must fill by far the
greatest part of the earth, and they must have a very high specific
gravity; for the average density of the earth is 5.52, and the outer
strata, the ocean and the masses of the surface which are known to us,
have smaller densities. The ordinary rocks possess a density ranging
from 2.5 to 3. It must, therefore, be assumed that the materials of
the innermost portions of the earth must be metallic, and Wiechert,
in particular, has advocated this view. Iron will presumably form the
chief constituent of this gas of the central earth. Spectrum analysis
teaches us that iron is a very important constituent of the sun. We
know, further, that the metallic portions of the meteorites consist
essentially of iron; and finally terrestrial magnetism indicates that
there must be large masses of iron in the interior of the earth.
We have also reason to believe that the native iron occurring in
nature—_e.g._, the well-known iron of Ovifak, in Greenland—is of
volcanic origin. The materials in the gaseous interior of the earth
will, owing to their high density, behave in chemical and physical
respects like liquids. As substances like iron will, also at very high
temperatures, have a far higher specific gravity than their oxides,
and these again have a higher gravity than their silicates, we have to
assume that the gases in the core of the earth will almost exclusively
be metallic, that the outer portions of the core will contain
essentially oxides, and those farther out again mostly silicates.
The fused magma will, on penetrating in the shape of batholithes
into the upper layers, probably be divided into two portions, of
which one, the lighter and gaseous, will contain water and substances
soluble in it; while the other, heavier portion, will essentially
consist of silicates with a lower percentage of water. The more fluid
portion, richer in water, will be secreted in the higher layers, will
penetrate into the surrounding sedimentary strata, especially into
their fissures, and will fill them with large crystals, often of
metallurgical value—_e.g._, of the ores of tin, copper, and other
metals, while the water will slowly evaporate through the superposed
strata. The more viscid and sluggish mass of silicates, on the other
hand, will congeal, thanks to its great viscosity, to glass, or, when
the cooling is very slow, to small crystals.
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