Principles of Geology: or, The Modern Changes of the Earth and its Inhabitants Considered as Illustrative of GeologyLyell, Charles, Sir
Science
Principles of Geology: or, The Modern Changes of the Earth and its Inhabitants Considered as Illustrative of Geology
Lyell, Charles, Sir
Geology
To return to the state of the earth after the changes above supposed, we
must not omit to dwell on the important effects to which a wide expanse
of perpetual snow would give rise. It is probable that nearly the whole
sea, from the poles to the parallels of 45°, would be frozen over; for
it is well known that the immediate proximity of land is not essential
to the formation and increase of field ice, provided there be in some
part of the same zone a sufficient quantity of glaciers generated on or
near the land, to cool down the sea. Captain Scoresby, in his account of
the arctic regions, observes, that when the sun's rays "fall upon the
snow-clad surface of the ice or land, they are in a great measure
reflected, without producing any material elevation of temperature; but
when they impinge on the black exterior of a ship, the pitch on one side
occasionally becomes fluid while ice is rapidly generated at the
other."[190]
Now field ice is almost always covered with snow;[191] and thus not only
land as extensive as our existing continents, but immense tracts of sea
in the frigid and temperate zones, might present a solid surface covered
with snow, and reflecting the sun's rays for the greater part of the
year. Within the tropics, moreover, where the ocean now predominates,
the sky would no longer be serene and clear, as in the present era; but
masses of floating ice would cause quick condensations of vapor, so that
fogs and clouds would deprive the vertical rays of the sun of half their
power. The whole planet, therefore, would receive annually a smaller
portion of the solar influence, and the external crust would part, by
radiation, with some of the heat which had been accumulated in it,
during a different state of the surface. This heat would be dissipated
in the spaces surrounding our atmosphere, which, according to the
calculations of M. Fourier, have a temperature much inferior to that of
freezing water.
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