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
Indications of an identical purport have been derived from another kind
of external disturbance, affecting our globe through the same agencies.
Lord Kelvin (then Sir William Thomson) pointed out in 1862[886] that
tidal influences are brought to bear on land as well as on water,
although obedience to them is perceptible only in the mobile element.
Some bodily distortion of the earth's figure _must_, however, take
place, unless we suppose it of absolute or "preternatural" rigidity, and
the amount of such distortion can be determined from its effect in
diminishing oceanic tides below their calculated value. For if the earth
were perfectly plastic to the stresses of solar and lunar gravity,
tides--in the ordinary sense--would not exist. Continents and oceans
would swell and subside together. It is to the _difference_ in the
behaviour of solid and liquid terrestrial constituents that the ebb and
flow of the waters are due.
Six years later, the distinguished Glasgow professor suggested that this
criterion might, by the aid of a prolonged series of exact tidal
observations, be practically applied to test the interior condition of
our planet.[887] In 1882, accordingly, suitable data extending over
thirty-three years having at length become available, Mr. G. H. Darwin
performed the laborious task of their analysis, with the general result
that the "effective rigidity" of the earth's mass must be _at least_ as
great as that of steel.[888]
Ratification from an unexpected quarter has lately been brought to this
conclusion. The question of a possible mobility in the earth's axis of
rotation has often been mooted. Now at last it has received an
affirmative reply. Dr. Küstner detected, in his observations of 1884-85,
effects apparently springing from a minute variation in the latitude of
Berlin. The matter having been brought before the International Geodetic
Association in 1888, special observations were set on foot at Berlin,
Potsdam, Prague, and Strasbourg, the upshot of which was to bring
plainly to view synchronous, and seemingly periodic fluctuations of
latitude to the extent of half a second of arc. The reality of these was
verified by an expedition to Honolulu in 1891-92, the variations there
corresponding inversely to those simultaneously determined in
Europe.[889] Their character was completely defined by Mr. S. C.
Chandler's discussion in October, 1891.[890] He showed that they could
be explained by supposing the pole of the earth to describe a circle
with a radius of thirty feet in a period of fourteen months.
Confirmation of this hypothesis was found by Dr. B. A. Gould in the
Cordoba observations,[891] and it was provided with a physical basis
through the able co-operation of Professor Newcomb.[892] The earth,
owing to its ellipsoidal shape, should, apart from disturbance, rotate
upon its "axis of figure," or shortest diameter; since thus alone can
the centrifugal forces generated by its spinning balance each other.
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