Illustrations of the Huttonian Theory of the EarthPlayfair, John
Science
Illustrations of the Huttonian Theory of the Earth
Playfair, John
Geology; Hutton, James, 1726-1797. Theory of the earth
Though Frisius concludes, as is stated here, that the acceleration
produced in the diurnal motion of the earth, is far too inconsiderable
to become the object of astronomical observation, he makes a
supposition difficult to be reconciled with this conclusion, namely,
that the acceleration has had a sensible effect on the figure of the
earth, or rather of the sea, having increased the centrifugal force,
and thereby accumulated the waters under the equator, in the present,
more than in former ages. Such an accumulation, he thinks agreeable
to certain appearances that have been observed respecting the ancient
level of the sea. These appearances will be afterwards considered: it
is sufficient to remark here, that though the fraction, expressing the
increment of the centrifugal force, must be double that which expresses
the acceleration, it must be too small to have any perceptible effect
in elevating the sea, except after an immense interval of time; and the
compensations which arise from other causes, probably must prevent it
from becoming sensible in any length of time whatsoever.]
377. The instance just given may serve as one of many, to shew what
confidence is to be placed in that indigested mass of facts and
quotations which Mr Kirwan, without discrimination, and without
discussion, has brought together from all quarters. He has no
intention, I believe, to deceive his readers; but we may judge, from
this specimen, of the precautions he has taken against being deceived
himself.
In some respects, the result of Frisi's investigation must be
considered as imperfect. If there were no relative motion in the parts
of our globe, but that by which things descend from a higher to a lower
level, a continual acceleration of its rotation, though extremely slow,
would take place, as above computed. But as, in the interior of the
earth, there are undoubtedly motions of a tendency opposite to those on
the surface, and directed from the centre towards the circumference,
they must produce a retardation in the diurnal revolution; and from
this must arise an inequality, not uniformly progressive in the same
direction, but periodical, and confined within certain limits, as the
causes are by which it is produced.[195]
Public-domain text, read in full here on John Shaqi.
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