A Preliminary Dissertation on the Mechanisms of the HeavensSomerville, Mary
Science
A Preliminary Dissertation on the Mechanisms of the Heavens
Somerville, Mary
Celestial mechanics
At the solstices the sun is at his greatest distance from the equator,
consequently his declination at these times is equal to the obliquity of
the ecliptic, which in former times was determined from the meridian
length of the shadow of the style of a dial on the day of the solstice.
The lengths of the meridian shadow at the summer and winter solstice are
recorded to have been observed at the city of Layang, in China, 1100
years before the Christian era. From these, the distances of the sun
from the zenith of the city of Layang are known. Half the sum of these
zenith distances determines the latitude, and half their difference
gives the obliquity of the ecliptic at the period of the observation;
and as the law of the variation in the obliquity is known, both the time
and place of the observations have been verified by computation from
modern tables. Thus the Chinese had made some advances in the science of
astronomy at that early period; the whole chronology of the Chinese is
founded on the observations of eclipses, which prove the existence of
that empire for more than 4700 years. The epoch of the lunar tables of
the Indians, supposed by Bailly to be 3000 before the Christian era, was
proved by La Place from the acceleration of the moon, not to be more
ancient than the time of Ptolemy. The great inequality of Jupiter and
Saturn whose cycle embraces 929 years, is peculiarly fitted for marking
the civilization of a people. The Indians had determined the mean
motions of these two planets in that part of their periods when the
apparent menu motion of Saturn was at the slowest, and that of Jupiter
the most rapid. The periods in which that happened were 3102 years
before the Christian era, and the year 1491 after it.
The returns of comets to their perihelia may possibly mark the present
state of astronomy to future ages.
The places of the fixed stars are affected by the precession of the
equinoxes; and as the law of that variation is known, their positions at
any time may be computed. Now Eudoxus, a contemporary of Plato, mentions
a star situate in the pole of the equator, and from computation it
appears that _χ_ Draconis was not very far from that place about 3000
years ago; but as Eudoxus lived only about 2150 years ago, he must have
described an anterior state of the heavens, supposed to be the same that
was determined by Chiron, about the time of the siege of Troy. Every
circumstance concurs in showing that astronomy was cultivated in the
highest ages of antiquity.
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