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
The _Nuncius Sidereus_ contained other discoveries which had the
same tendency in other ways. The examination of the moon showed, or
at least seemed to show, that she was a solid body, with a surface
extremely rugged and irregular. This, though perhaps not bearing
directly upon the question of the heliocentric theory, was yet a
blow to the Aristotelians, who had, in their philosophy, made the
moon a body of a kind altogether different from this, and had given
an abundant quantity of reasons for the visible marks on her
surface, all proceeding on these preconceived views. Others of his
discoveries produced the same effect; for instance, the new stars
invisible to the naked eye, and those extraordinary appearances
called Nebulæ.
But before the end of the year, Galileo had new information to
communicate, bearing more decidedly on the Copernican controversy.
This intelligence was indeed decisive with regard to the motion of
Venus about the sun; for he found that that planet, in the course of
her revolution, assumes the same succession of phases which the moon
exhibits in the course of a month. This he expressed by a Latin
verse:
Cynthiæ figuras æmulatur mater amorum:
The Queen of Love like Cynthia shapes her forms:
transposing the letters of this line in the published account,
according to the practice of the age; which thus showed the ancient
love for combining verbal puzzles with scientific discoveries, while
it betrayed the newer feeling, of jealousy respecting the priority
of discovery of physical facts.
It had always been a formidable objection to the Copernican theory
that this appearance of the planets had not been observed. The
author {279} of that theory had endeavored to account for this, by
supposing that the rays of the sun passed freely through the body of
the planet; and Galileo takes occasion to praise him for not being
deterred from adopting the system which, on the whole, appeared to
agree best with the phenomena, by meeting with some appearances
which it did not enable him to explain.[26\5] Yet while the fate of
the theory was yet undecided, this could not but be looked upon as a
weak point in its defences.
[Note 26\5: Drinkwater-Bethune, _Life of Galileo_, p. 35.]
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