Worlds in the making: The evolution of the universeArrhenius, Svante
Science
Worlds in the making: The evolution of the universe
Arrhenius, Svante
Cosmogony
The motion and diffusion in the magma, and especially in the very
viscous and sluggish acid portions of the upper strata, will therefore
be exceedingly small, and the magma will behave almost like a solid
body, like the minerals of the experiments of Day and Allen. The magmas
of volcanoes like Etna, Vesuvius, and Pantellaria may, therefore, have
quite different compositions, as we should conclude from their lavas
without our being forced to believe, with Stübel, that these three
hearths of volcanoes are completely separated, though not far removed
from one another. In the lava of Vesuvius a temperature of 1000 or 1100
degrees has been found at the lower extremity of the stream. From the
occurrence in the lava of certain crystals like leucite and olivin,
which we have reason to assume must have been formed before the lava
left the crater, it has been concluded that the lava temperature cannot
have been higher than 1400 degrees before it left the volcanic pipe.
It would, however, be erroneous to deduce from the temperature of the
lava of Vesuvius that the hearth of the volcano must be situated at a
depth of approximately 50 kilometres. Most likely its depth is much
smaller, perhaps not even 10 kilometres. For there, as everywhere where
volcanoes occur, the crust of the earth is strongly furrowed, and the
magma will just at the spots where we find volcanoes come much nearer
to the surface of the earth than elsewhere.
The importance of water for the formation of volcanoes probably lies
in the fact that, in the neighborhood of cracks under the bottom of
the sea, the water penetrates down to considerable depths. When the
water reaches a stratum of a temperature of 365 degrees—the so-called
critical temperature of water—it can no longer remain in the liquid
state. That would not prevent, however, its penetrating still farther
into the depths, in spite of its gaseous condition. As soon as the
vapor comes in contact with magma, it will eagerly be absorbed by the
magma. The reason is that water of a temperature of more than 300
degrees is a stronger acid than silicic acid; the latter is therefore
expelled by it from its compounds, the silicates, which form the main
constituents of the magma. The higher the temperature, the greater the
power of the magma to absorb water. Owing to this absorption the magma
swells and becomes at the same time more fluid. The magma is therefore
pressed out by the action of a pressure which is analogous to the
osmotic pressure by virtue of which water penetrates through a membrane
into a solution of sugar or salt. This pressure may become equivalent
to thousands of atmospheres, and this very pressure would raise the
magma up the volcanic pipe even to a height of 6000 m. (20,000 feet)
above the sea-level. As the magma is ascending in the volcanic pipe
it is slowly cooled, and its capacity for binding water diminishes
with falling temperature. The water will hence escape under violent
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