Astronomy: The Science of the Heavenly BodiesTodd, David P. (David Peck)
History
Astronomy: The Science of the Heavenly Bodies
Todd, David P. (David Peck)
Astronomy
Ptolemy was an observer of the heavens, though not of the highest order;
but he had all the work of his predecessors, best of all Hipparchus, to
build upon. Ptolemy's greatest work was the "Megale Syntaxis," generally
known as the Almagest. It forms a nearly complete compendium of the
ancient astronomy, and although it embodies much error, because built on
a wrong theory, the Almagest nevertheless is competent to follow the
motions of all the bodies in the sky with a close approach to accuracy,
even at the present day. This marvelous work written at this critical
epoch became as authoritative as the philosophy of Aristotle, and for
many centuries it was the last word in the science. The old astrology
held full sway, and the Ptolemaic theory of the universe supplied
everything necessary: further progress, indeed, was deemed impossible.
The Almagest comprises in all thirteen books, the first two of which
deal with the simpler observations of the celestial sphere, its own
motion and the apparent motions of sun, moon, and planets upon it. He
discusses, too, the postulates of his system and exhibits great skill as
an original geometer and mathematician. In the third book he takes up
the length of the year, and in the fourth book similarly the moon and
the length of the month. Here his mathematical powers are at their best,
and he made a discovery of an inequality in the moon's motion known as
the evection. Book five describes the construction and use of the
astrolabe, a combination of graduated circles with which Ptolemy made
most of his observations. In the sixth book he follows mainly Hipparchus
in dealing with eclipses of sun and moon. In the seventh and eighth
books he discusses the motion of the equinox, and embodies a catalogue
of 1,028 stars, substantially as in Hipparchus. The five remaining books
of the Almagest deal with the planetary motions, and are the most
important of all of Ptolemy's original contributions to astronomy.
Ptolemy's fundamental doctrines were that the heavens are spherical in
form, all the heavenly motions being in circles. In his view, the earth
too is spherical, and it is located at the center of the universe, being
only a point, as it were, in comparison. All was founded on mere
appearance combined with the philosophical notion that the circle being
the only perfect curve, all motions of heavenly bodies must take place
in earth-centered circles. For fourteen or fifteen centuries this false
theory persisted, on the authority of Ptolemy and the Almagest,
rendering progress toward the development of the true theory impossible.
Public-domain text, read in full here on John Shaqi.
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