History of the inductive sciences, from the earliest to the present timeWhewell, William
History
History of the inductive sciences, from the earliest to the present time
Whewell, William
Science -- History
It will easily be understood, that since the ancient geocentric
hypothesis ascribed to the planets those motions which were apparent
only, and which really arose from the motion of the earth round the
sun in the new hypothesis, the latter scheme must much simplify the
planetary theory. Kepler[8\5] enumerates eleven motions of the
Ptolemaic system, which are at once exterminated and rendered
unnecessary by the new system. Still, as the real motions, both of
the earth and the planets, are unequable, it was requisite to have
some mode of representing their inequalities; and, accordingly, the
ancient theory of eccentrics and epicycles was retained, so far as
was requisite for this purpose. The planets revolved round the sun
by means of a Deferent, and a {264} great and small Epicycle; or
else by means of an Eccentric and Epicycle, modified from Ptolemy's,
for reasons which we shall shortly mention. This mode of
representing the motions of the planets continued in use, until it
was expelled by the discoveries of Kepler.
[Note 8\5: _Myst. Cosm._ cap. 1.]
Besides the daily rotation of the earth on its axis, and its annual
circuit about the sun, Copernicus attributed to the axis a "motion
of declination," by which, during the whole annual revolution, the
pole was constantly directed towards the same part of the heavens.
This constancy in the absolute direction of the axis, or its moving
parallel to itself, may be more correctly viewed as not indicating
any separate motion. The axis continues in the same direction,
because there is nothing to make it change its direction; just as a
straw, lying on the surface of a cup of water, continues to point
nearly in the same direction when the cup is carried round a room.
And this was noticed by Copernicus's adherent, Rothman,[9\5] a few
years after the publication of the work _De Revolutionibus_. "There
is no occasion," he says, in a letter to Tycho Brahe, "for the
triple motion of the earth: the annual and diurnal motions suffice."
This error of Copernicus, if it be looked upon as an error, arose
from his referring the position of the axis to a limited space,
which he conceived to be carried round the sun along with the earth,
instead of referring it to fixed or absolute space. When, in a
Planetarium (a machine in which the motions of the planets are
imitated), the earth is carried round the sun by being fastened to a
material radius, it is requisite to give a motion to the axis by
_additional_ machinery, in order to enable it to _preserve_ its
parallelism. A similar confusion of geometrical conception, produced
by a double reference to absolute space and to the centre of
revolution, often leads persons to dispute whether the moon, which
revolves about the earth, always turning to it the same face,
revolves about her axis or not.
[Note 9\5: Tycho. Epist. i. p. 184, A. D. 1590.]
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