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 is also to be noticed that the precession of the equinoxes made
it necessary to suppose the axis of the earth to be not _exactly_
parallel to itself, but to deviate from that position by a slight
annual difference. Copernicus erroneously supposes the precession to
be unequable; and his method of explaining this change, which is
simpler than that of the ancients, becomes more simple still, when
applied to the true state of the facts.
The tendencies of our speculative nature, which carry us onwards in
{265} pursuit of symmetry and rule, and which thus produced the
theory of Copernicus, as they produce all theories, perpetually show
their vigor by overshooting their mark. They obtain something by
aiming at much more. They detect the order and connection which
exist, by imagining relations of order and connection which have no
existence. Real discoveries are thus mixed with baseless
assumptions; profound sagacity is combined with fanciful conjecture;
not rarely, or in peculiar instances, but commonly, and in most
cases; probably in all, if we could read the thoughts of the
discoverers as we read the books of Kepler. To try wrong guesses is
apparently the only way to hit upon right ones. The character of the
true philosopher is, not that he never conjectures hazardously, but
that his conjectures are clearly conceived and brought into rigid
contact with facts. He sees and compares distinctly the ideas and
the things,--the relations of his notions to each other and to
phenomena. Under these conditions it is not only excusable, but
necessary for him, to snatch at every semblance of general rule;--to
try all promising forms of simplicity and symmetry.
Copernicus is not exempt from giving us, in his work, an example of
this character of the inventive spirit. The axiom that the celestial
motions must be _circular_ and _uniform_, appeared to him to have
strong claims to acceptation; and his theory of the inequalities of
the planetary motions is fashioned upon it. His great desire was to
apply it more rigidly than Ptolemy had done. The time did not come
for rejecting this axiom, till the observations of Tycho Brahe and
the calculations of Kepler had been made.
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