A Popular History of Astronomy During the Nineteenth Century: Fourth EditionClerke, Agnes M. (Agnes Mary)
History
A Popular History of Astronomy During the Nineteenth Century: Fourth Edition
Clerke, Agnes M. (Agnes Mary)
Astronomy -- History -- 19th century
Temporary causes, however, such as heavy falls of snow or rain limited
to one continental area, the shifting of ice-masses, even the movements
of winds, may render the globe slightly lop-sided, and thus oblige it to
forsake its normal axis, and rotate on one somewhat divergent from it.
This "instantaneous axis" (for it is incessantly changing) must, by
mathematical theory, revolve round the axis of figure in a period of 306
days. Provided, that is to say, the earth were a perfectly rigid body.
But it is far from being so; it yields sensibly to every strain put upon
it; and this yielding tends to protract the time of circulation of the
displaced pole. The length of its period, then, serves as a kind of
measure of the plasticity of the globe; which, according to Newcomb's
and S. S. Hough's independent calculations,[893] seems to be a little
less than that of steel. In an earth compacted of steel, the
instantaneous axis would revolve in 441 days; in the actual earth, the
process is accomplished in 428 days. By this new path, accordingly,
astronomers have been led to an identical estimate of the consistence of
our globe with that derived from tidal investigations.
Variations of latitude are intrinsically complex. To produce them, an
incalculable interplay of causes must be at work, each with its proper
period and law of action.[894] All the elements of the phenomenon are
then in a perpetual state of flux,[895] and absorb for their continual
redetermination, the arduous and combined labours of many astronomers.
Nor is this trouble superfluous. Minute in extent though they be, the
shiftings of the pole menace the very foundations of exact celestial
science; their neglect would leave the entire fabric insecure. Just at
the beginning of the present century they reached a predicted minimum,
but are expected again to augment their range after the year 1902. The
interesting suggestion has been made by Mr. J. Halm that such
fluctuations are, in some obscure way, affected by changes in solar
activity, and conform like them to an eleven-year cycle.[896]
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