Cosmos: A Sketch of the Physical Description of the Universe, Vol. 1Humboldt, Alexander von
History
Cosmos: A Sketch of the Physical Description of the Universe, Vol. 1
Humboldt, Alexander von
Astronomy; Cosmography; Physical geography; Science -- History
[footnote] **Numerous observations also show great irregularities in the
length of the pendulum in the midst of continents, and which are ascribed to
local attractions. (Delambre, 'Mesure de la Meridienne', t. iii., p. 548;
Biot, in the 'Mem. de l'Academie des Sciences', t. viii., 1829, p. 18 and
23.) In passing over the South of France and Lombardy from west to east, we
find the minimum intensity of gravitation at Bordeaux; from thence it
increases rapidly as we advance eastward, through Figeac, Clermont-Ferrand,
Milan, and Padua; and in the last town we find that the intensity has
attained its maximum. The influence of the southern declivities of the Alps
is not merely t on the general size of their mass, but (much more), in the
opinion of Elie de Beaumont ('Rech. sur les Revol. de la Surface du Globe',
1830, p. 729), on the rocks of melaphyre and serpentine, which have elevated
the chain. On the declivity of Ararat, which with Caucasus may be said to
lie in the center of gravity of the old continent formed by Europe, Asia,
and Africa, the very exact pendulum experiments of Fedorow give indications,
not of subterranean cavities, but of dense volcanic masses. (Parrot, 'Reise
zum Ararat', bd. ii., s. 143.) In the geodesic operations of Carlini and
Plana, in Lombardy, differences ranging from 20" to 47".8 have been found
between direct observations of latitude and the results of these operations.
(See the instances of Andrate and Mondovi, and those of Milan and Padua, in
the 'Operations Geodes. et Astron. pour la Mesure d'un Arc du Parallele
Moyen', t. ii., p. 347; 'Effemeridi Astron. di Milano', 1842, p. 57.) The
latitude of Milan, deduced from that of Berne, according to the , is
45ºdegrees 27' 52", while, according to direct astronomical observations,
it is 45 degrees 27' 35". As the perturbations extend in the plain of
Lombardy to Parma, which is far south of the Po (Plana, 'Operat. Geod.', t.
ii., p. 847), it is probable that there are deflecting causes 'concealed
beneath the soil of the plain itself'. Struve has made similar experiments
[with corresponding results] in the most level parts of eastern Europe.
(Schumacher, 'Astron. Nachrichten', 1830, No. 164, s. 399.) Regarding the
influence of dense masses supposed to lie at a small depth, equal to the
mean height of the Alps, see the analytical expressions given by Hossard and
Rozet, in the 'Comptes Rendus', t. xviii., 1844, p. 292, and compare them
with Poisson, 'Traite de Mecanique' (2me ed., t. i., p. 482. The earliest
observations on the influence which different kinds of rocks exercise on the
vibration of the pendulum are those of Thomas Young, in the 'Philos.
Transactions' for 1819, p. 70-96. In drawing conclusions regarding the
Earth's curvature from the length of the pendulum, we ought not to overlook
the possibility that its crust may have undergone a process of hardening
previously to metallic and dense basaltic masses having penetrated from
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