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
The verification of this ingenious hypothesis depends upon a variety of
intricate meteorological conditions, some of which have been adversely
interpreted by competent authorities.[902] What is still more serious,
its acceptance seems precluded by time-relations of a simple kind. Dr.
Wright[903] has established with some approach to certainty that glacial
conditions ceased in Canada and the United States about ten or twelve
thousand years ago. The erosive action of the Falls of Niagara qualifies
them to serve as a clepsydra, or water-clock on a grand scale; and their
chronological indications have been amply corroborated elsewhere and
otherwise on the same continent. The astronomical Ice Age, however,
should have been enormously more antique. No reconciliation of the facts
with the theory appears possible.
The first attempt at an experimental estimate of the "mean density" of
the earth was Maskelyne's observation in 1774 of the deflection of a
plumb-line through the attraction of Schehallien. The conclusion thence
derived, that our globe weighs 4-1/2 times as much as an equal bulk of
water,[904] was not very exact. It was considerably improved upon by
Cavendish, who, in 1798, brought into use the "torsion-balance"
constructed for the same purpose by John Michell. The resulting estimate
of 5·48 was raised to 5·66 by Francis Baily's elaborate repetition of
the process in 1838-42. From experiments on the subject made in 1872-73
by Cornu and Baille the slightly inferior value of 5·56 was derived; and
it was further shown that the data collected by Baily, when corrected
for a systematic error, gave practically the same result (5·55).[905] M.
Wilsing's of 5·58, obtained at Potsdam in 1889,[906] nearly agreed with
it; while Professor Poynting, by means of a common balance, arrived at a
terrestrial mean density of 5·49.[907] Professor Boys next entered the
field with an exquisite apparatus, in which a quartz fibre performed the
functions of a torsion-rod; and the figure 5·53 determined by him, and
exactly confirmed by Dr. Braun's research at Mariaschein, Bohemia, in
1896,[908] may be called the standard value of the required datum.
Newton's guess at the average weight of the earth as five or six times
that of water has thus been curiously verified.
Public-domain text, read in full here on John Shaqi.
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