The variation of the length of the seconds pendulum observed by Richer
in his Cayenne expedition (chapter VIII., § 161) had been the first
indication of a deviation of the earth from a spherical form. Newton
inferred, both from these pendulum experiments and from an independent
theoretical investigation (chapter IX., § 187), that the earth was
spheroidal, being flattened towards the poles; and this view was
strengthened by the satisfactory explanation of precession to which it
led (chapter IX., § 188).
On the other hand, a comparison of various measurements of arcs of the
meridian in different latitudes gave some support to the view that
the earth was elongated towards the poles and flattened towards the
equator, a view championed with great ardour by the Cassini school.
It was clearly important that the question should be settled by more
extensive and careful earth-measurements.
The essential part of an ordinary measurement of the earth consists
in ascertaining the distance in miles between two places on the same
meridian, the latitudes of which differ by a known amount. From
these two data the length of an arc of a meridian corresponding to a
difference of latitude of 1° at once follows. The =latitude= of a place
is the angle which the vertical at the place makes with the equator,
or, expressed in a slightly different form, is the angular distance of
the zenith from the celestial equator. The =vertical= at any place may
be defined as a direction perpendicular to the surface of still water
at the place in question, and may be regarded as perpendicular to the
true surface of the earth, accidental irregularities in its form such
as hills and valleys being ignored.[123]
The difference of latitude between two places, north and south of one
another, is consequently the angle between the verticals there. Fig.
78 shews the verticals, marked by the arrowheads, at places on the
same meridian in latitudes differing by 10°; so that two consecutive
verticals are inclined in every case at an angle of 10°.
[Illustration: FIG. 78.—The varying curvature of the earth.]
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