Time and Clocks: A Description of Ancient and Modern Methods of Measuring TimeCunynghame, Henry H. (Henry Hardinge), Sir
Philosophy
Time and Clocks: A Description of Ancient and Modern Methods of Measuring Time
Cunynghame, Henry H. (Henry Hardinge), Sir
Clocks and watches; Time
The works of Aristotle are full of the fallacious method of the old
system. In his work on the heavens he repeatedly argues that the
heavenly bodies must move in circles, because the circle is the most
perfect figure. He affects a perplexity as to how a circle can at the
same time be convex and also its opposite, concave, and repeatedly
entangles his readers in similar mere word confusion.
Regarded as a man of science, he must be placed, I think, in spite
of his great genius, below Archimedes, Hipparchus, and several other
ancient astronomers and physicists.
His errors lived after him and dominated the thought of the middle
ages, and for a long time delayed the progress of science.
The other great writer on astronomy of ancient times was Ptolemy of
Alexandria.
His work was called the “Great Collection,” and was what we should
now term a compendium of astronomy. Although based on a fundamental
error, it is a thoroughly scientific work. There is none of the false
philosophy in it that so much disfigures the work of Aristotle. The
reasons for believing that the earth is at rest are interesting.
Ptolemy argues that if the earth were moving round on its axis once in
twenty-four hours a bird that flew up from it would be left behind.
At first sight this argument seems very convincing, for it appears
impossible to conceive a body spinning at the rate at which the earth
is alleged to move, and yet not leaving behind any bodies that become
detached from it.
On the other hand, the system which taught that the sun and planets
moved round the earth, and which had been adopted largely on account
of its supposed simplicity, proved, on further examination, to be
exceedingly complicated. Each planet, instead of moving simply and
uniformly round the earth in a circle, had to be supposed to move
uniformly in a circle round another point that moved round the earth in
a circle. This secondary circle, in which the planet moved, was called
an epicycle. And even this more complicated view failed to explain the
facts.
A system which, like that of Aristotle and Ptolemy, was based on
deductions from concepts, and which consisted rather of drawing
conclusions than of examining premises, was very well adapted to
mediæval thought, and formed the foundation of astronomy and geography
as taught by the schoolmen.
[Illustration: FIG. 20.]
Public-domain text, read in full here on John Shaqi.
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