Jewish philosophy -- Early works to 1800; Judaism -- Works to 1900; Philosophy, Medieval -- Early works to 1800
the deviation assumed in respect to the latitude of the paths of Venus
and Mercury, I have already clearly shown you vivâ voce that it is
impossible to imagine material beings under such conditions. You have
seen that Ptolemy has already pointed out this difficulty. He says as
follows: “Let no one think that these and similar principles are
improbable. If any one considers what we have here expounded in the
same light as he considers things produced by skill and subtle work, he
will find it improbable; but it is not right to compare human things to
divine things.” This is, as you know, what Ptolemy says, and I have
already pointed out to you the passages by which you can verify all I
said, except what I stated about the position of the centres of the
excentric spheres; for I have not heard that any one has paid attention
to this question. But you will understand it when you know the length
of the diameter of each sphere, and the extent of its excentricity in
terms of radii of the earth, according to the facts which Kabici has
established in his treatise on the distances. When you notice these
distances you will confirm my words.
Consider, therefore, how many difficulties arise if we accept the
theory which Aristotle expounds in Physics. For, according to that
theory, there are no epicycles, and no excentric spheres, but all
spheres rotate round the centre of the earth! How then can the
different courses of the stars be explained? how is it possible to
assume a uniform perfect rotation with the phenomena which we perceive,
except by admitting one of the two hypotheses or both of them? The
difficulty is still more apparent when we find that admitting what
Ptolemy said as regards the epicycle of the moon, and its inclination
towards a point different both from the centre of the Universe and from
its own centre, the calculations according to these hypotheses are
perfectly correct, within one minute; that their correctness is
confirmed by the most accurate calculation of the time, duration, and
extent of the eclipses, which is always based on these hypotheses.
Furthermore, how can we reconcile, without assuming the existence of
epicycles, the apparent retrogression of a star with its other motions?
How can rotation or motion take place round a point which is not fixed?
These are real difficulties.
Public-domain text, read in full here on John Shaqi.
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