The story of the universe. Volume 2 (of 4) : $b The earth : land and sea
History
The story of the universe. Volume 2 (of 4) : $b The earth : land and sea
Astronomy; Earth (Planet); Natural history
Coal, as we shall find, is composed of the mineralized remains of
the vegetation which flourished in remote ages of the world. Buried
under an enormous thickness of rocks, it has been preserved to
our days, after being modified in its inward nature and external
aspect. Having lost a portion of its elementary constituents, it has
become transformed into a species of carbon, impregnated with those
bituminous substances which are the ordinary products of the slow
decomposition of vegetable matter.
Thus, coal is the substance of the plants which formed the forests,
the vegetation, and the marshes of the ancient world, at a period
too distant for human chronology to calculate with anything like
precision.
It is a remarkable circumstance that conditions of equable and warm
climate, combined with humidity, do not seem to have been limited to
any one part of the globe, but the temperature of the whole globe
seems to have been nearly the same in very different latitudes. From
the equatorial regions up to Melville Island, in the Arctic Ocean,
where in our days eternal frost prevails--from Spitzbergen to the
centre of Africa, the carboniferous flora is identically the same.
When nearly the same plants are found in Greenland and Guinea; when
the same species, now extinct, are met with of equal development at
the equator as at the pole, we can not but admit that at this epoch
the temperature of the globe was nearly alike everywhere. What we now
call _climate_ was unknown in these geological times. There seems to
have been then only one climate over the whole globe. It was at a
subsequent period, that is, in later Tertiary times, that the cold
began to make itself felt at the terrestrial poles. Whence, then,
proceeded this general superficial warmth, which we now regard with
so much surprise? It was a consequence of the greater or nearer
influence of the interior heat of the globe. The earth was still so
hot in itself that the heat which reached it from the sun may have
been inappreciable.
Public-domain text, read in full here on John Shaqi.
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