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
_Measure of the Sun's Distance._--The explanation of the phases of the
moon led to no result so remarkable as the attempt of Aristarchus of
Samos to obtain from this doctrine a measure of the Distance of the
Sun as compared with that of the Moon. If the moon was a perfectly
smooth sphere, when she was exactly midway between the new and full in
position (that is, a quadrant from the sun), she would be somewhat
more than a half moon; and the place when she was _dichotomized_, that
is, was an exact semicircle, the bright part being bounded by a
straight line, would depend upon the sun's distance from the earth.
Aristarchus endeavored to fix the exact place of this Dichotomy; but
the irregularity of the edge which bounds the bright part of the moon,
and the difficulty of measuring with accuracy, by means then in use,
either the precise time when the boundary was most nearly a straight
line, or the exact distance of the moon from the sun at that time,
rendered his conclusion false and valueless. He collected that the sun
is at 18 times the distance of the moon from us; we now know that he
is at 400 times the moon's distance.
It would be easy to dwell longer on subjects of this kind; but we
have already perhaps entered too much in detail. We have been {138}
tempted to do this by the interest which the mathematical spirit of
the Greeks gave to the earliest astronomical discoveries, when these
were the subjects of their reasonings; but we must now proceed to
contemplate them engaged in a worthier employment, namely, in adding
to these discoveries.
CHAPTER II.
PRELUDE TO THE INDUCTIVE EPOCH OF HIPPARCHUS.
WITHOUT pretending that we have exhausted the consequences of the
elementary discoveries which we have enumerated, we now proceed to
consider the nature and circumstances of the next great discovery
which makes an Epoch in the history of Astronomy; and this we shall
find to be the Theory of Epicycles and Eccentrics. Before, however,
we relate the establishment of this theory, we must, according to
the general plan we have marked out, notice some of the conjectures
and attempts by which it was preceded, and the growing acquaintance
with facts, which made the want of such an explanation felt.
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