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
We may judge of the difficulty of casting off the theory of eccentrics
and epicycles, by recollecting that Copernicus did not do it at all,
and that Kepler only did it after repeated struggles; the history of
which occupies thirty-nine Chapters of his book. At the end of them he
says, "This prolix disputation was necessary, in order to prepare the
way to the natural form of the equations, of which I am now to
treat.[36\5] My first error was, that the path of a planet is a
perfect circle;--an opinion which was a more mischievous thief of my
time, {299} in proportion as it was supported by the authority of all
philosophers, and apparently agreeable to metaphysics." But before he
attempts to correct this erroneous part of his hypothesis, he sets
about discovering the law according to which the different parts of
the orbit are described in the case of the earth, in which case the
eccentricity is so small that the effect of the oval form is
insensible. The result of this inquiry was[37\5] the Rule, that the
time of describing any arc of the orbit is proportional to the area
intercepted between the curve and two lines drawn from the sun to the
extremities of the arc. It is to be observed that this rule, at first,
though it had the recommendation of being selected after the
unavoidable abandonment of many, which were suggested by the notions
of those times, was far from being adopted upon any very rigid or
cautious grounds. A rule had been proved at the apsides of the orbit,
by calculation from observations, and had then been extended by
conjecture to other parts of the orbit; and the rule of the areas was
only an approximate and inaccurate mode of representing this rule,
employed for the purpose of brevity and convenience, in consequence of
the difficulty of applying, geometrically, that which Kepler now
conceived to be the true rule, and which required him to find the sum
of the lines drawn from the sun to _every_ point of the orbit. When he
proceeded to apply this rule to Mars, in whose orbit the oval form is
much more marked, additional difficulties came in his way; and here
again the true supposition, that the _oval_ is of that special kind
called _ellipse_, was adopted at first only in order to simplify
calculation,[38\5] and the deviation from exactness in the result was
attributed to the inaccuracy of those approximate processes. The
supposition of the oval had already been forced upon Purbach in the
case of Mercury, and upon Reinhold in the case of the Moon. The centre
of the epicycle was made to describe an egg-shaped figure in the
former case, and a lenticular figure in the latter.[39\5]
[Note 36\5: _De Stellâ Martis_, iii. 40.]
[Note 37\5: _De Stellâ Martis_, p. 194.]
[Note 38\5: Ib. iv. c. 47.]
[Note 39\5: L. U. K. Kepler, p. 30.]
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