The story of the sun, moon, and starsGiberne, Agnes
Science
The story of the sun, moon, and stars
Giberne, Agnes
Astronomy -- Juvenile literature
Despite this great mistake, still persistently believed in, and despite
the crude notions of early astronomers on many points, it is marvelous
how much they did manage to observe and to learn for themselves,--as
to the sun and his apparent path, as to the moon and her path, as to
the five then known planets and their paths, as to eclipses and other
phenomena.
By all such careful watching, although they to some extent missed their
aim and fell into mistakes, yet they paved a way to later discoveries
and to fuller knowledge. Their work was not thrown away, their trouble
was not lost; for out of their very errors grew the fair form of truth.
Nearly three hundred years after the time of Hipparchus came the famous
Ptolemy--famous, not, like certain other astronomers, for stupendous
genius, or for the brilliancy and accuracy of his observations, but
rather noted for the ingenuity of his explanations, and for the adroit
manner in which he systematized such knowledge, on the subject of the
heavenly bodies, as was then in the possession of mankind.
Ptolemy’s name is best known in connection with what is commonly called
“The Ptolemaic System of the Universe,” and his greatest astronomical
work is best known as the _Almagest_.
A great many of Ptolemy’s leading notions, as well as the principal
mass of facts upon which he worked, were doubtless borrowed from
Hipparchus. The latter is said to have explained the movements of the
sun and of the moon by means of small epicycles, traveling round the
earth on circular orbits; and even Hipparchus did not originate this
fundamental idea of the so-called “Ptolemaic System,” which had indeed
been held by the ancients in much earlier days. Hipparchus worked it
out to some extent, and Ptolemy carried on the process much farther,
giving forth the system to the world in such wise that ever since it
has gone by his name.
The theory of cycles and epicycles lasted long--lasted from the time
of Ptolemy in the second century to the time of Copernicus in the
sixteenth century, of whom we have already spoken.
[For about two thousand years, astronomers observed attentively the
apparent revolutions of the heavenly bodies, and this attentive study
gradually showed them a large number of irregularities and inexplicable
complications, until at last they recognized that they were deceived as
to the earth’s position, in the same way that they had been deceived
as to its stability. The immortal Copernicus, in particular, discussed
with perseverance the earth’s motion, already previously suspected for
two thousand years, but always rejected by man’s self-love; and when
this learned Polish canon bid adieu to our world in the year 1543, he
bequeathed to science his great work, which demonstrated clearly the
long-standing error of mankind.--_F._]
Public-domain text, read in full here on John Shaqi.
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