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
These conjectures and assumptions led naturally to the establishment
of the various parts of the Theory of Epicycles. It is probable that
this theory was adopted with respect to the Planets at or before the
time of Plato. And Aristotle gives us an account of the system thus
devised.[61\3] "Eudoxus," he says, "attributed four spheres to each
Planet: the first revolved with the fixed stars (and this produced
the diurnal motion); the second gave the planet a motion along the
ecliptic (the mean motion in longitude); the third had its axis
perpendicular[62\3] to the ecliptic (and this gave the inequality of
each planetary motion, really arising from its special motion about
the sun); the fourth produced the oblique motion transverse to this
(the motion in latitude)." He is also said to have attributed a
motion in latitude and a corresponding sphere to the Sun as well as
to the Moon, of which it is difficult to understand the meaning, if
Aristotle has reported rightly of the theory; for it would be absurd
to ascribe to Eudoxus a knowledge of the motions by which the sun
deviates from the ecliptic. Calippus conceived that two additional
spheres must be given to the sun and to the moon, in order to
explain the phenomena: probably he was aware of the inequalities of
the motions of these luminaries. He also proposed an additional
sphere for each planet, to account, we may suppose, for the results
of the eccentricity of the orbits.
[Note 61\3: Metaph. xi. 8.]
[Note 62\3: Aristotle says "has its poles in the ecliptic," but this
must be a mistake of his. He professes merely to receive these
opinions from the mathematical astronomers, "ἐκ τῆς οἰκειοτάτης
φιλοσοφίας τῶν μαθηματικῶν."]
The hypothesis, in this form, does not appear to have been reduced
to measure, and was, moreover, unnecessarily complex. The resolution
{144} of the oblique motion of the moon into two separate motions,
by Eudoxus, was not the simplest way of conceiving it; and Calippus
imagined the connection of these spheres in some way which made it
necessary nearly to double their number; in this manner his system
had no less than 55 spheres.
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