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
Now the opinion originally suggested by Sir W. Herschel, that our sun
and its attendant planets were all moving onward through space, in the
direction of the constellation Hercules, is very generally thought by
eminent astronomers to be confirmed. But even if its reality be no
longer matter of doubt, conjectures as to its amount are still vague and
uncertain; and great, indeed, must be the extent of the movement before
this cause alone can work any material alteration in the terrestrial
climates. Mr. Hopkins, when treating of this theory, remarked, that so
far as we were acquainted with the position of the stars not very remote
from the sun, they seem to be so distant from each other, that there are
no points in space among them, where the intensity of radiating heat
would be comparable to that which the earth derives from the sun, except
at points very near to each star. Thus, in order that the earth should
derive a degree of heat from stellar radiation comparable to that now
derived from the sun, she must be in close proximity to some particular
star, leaving the aggregate effect of radiation from the other stars
nearly the same as at present. This approximation, however, to a single
star could not take place consistently with the preservation of the
motion of the earth about the sun, according to its present laws.
Suppose our sun should approach a star within the present distance of
Neptune. That planet could no longer remain a member of the solar
system, and the motions of the other planets would be disturbed in a
degree which no one has ever contemplated as probable since the
existence of the solar system. But such a star, supposing it to be no
larger than the sun, and to emit the same quantity of heat, would not
send to the earth much more than one-thousandth part of the heat which
she derives from the sun, and would therefore produce only a very small
change in terrestrial temperature.[208]
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