Ancient calendars and constellationsPlunket, Emmeline M. (Emmeline Mary)
History
Ancient calendars and constellations
Plunket, Emmeline M. (Emmeline Mary)
Astronomy, Ancient; Calendar; Constellations
Ours is a _tropical_ year, that is to say, according to the Julian
calendar (afterwards amended by Pope Gregory) it is bound to the
_seasons_, and its months maintain a constant relation to the four
great divisions of the ecliptic, _i.e._ the solstices and the
equinoxes. The winter solstice always falls about the 22nd of December,
the spring equinox about the 21st of March, the summer solstice about
the 21st of June, and the autumnal equinox about the 23rd of September.
But (as has been suggested) the Accadian year was a _sidereal_
year, and its months maintained a constant relation to the twelve
_star-marked_ divisions of the ecliptic, or, as they are called, the
constellations of the Zodiac. Nisan always corresponded (as closely as
a lunar month might) to the time during which the sun traversed the
constellation Aries; Airu to the time during which it traversed the
constellation Taurus; and so on through the twelve months of the year.
The equinoctial points are, however, always, though slowly, changing
their position amongst the twelve constellations of the ecliptic. The
months, therefore, which in 3,800 B.C., and still in the second century
B.C., corresponded to the same star-groups, as above noted, must have
held in different ages very different positions in regard to the four
great divisions or _seasons_ of the year.
We find in the tablets translated by Epping and Strassmaier the year
“_beginning with Nisan, hence in the spring_,” and this seems a more
or less natural season from which to count the year; but when, taking
the precession of the equinoxes into account, we find that the year in
Ḫammurabi’s time (2,200 B.C.) must have commenced one month, and in
Sargon’s time (3,800 B.C.) two months before the spring equinox, we
feel surprised and perplexed to find that the year must then have begun
without any reference to the seasons--the four great and most easily
observed divisions of the ecliptic.
It is difficult to imagine that the astronomers who so skilfully
divided the ecliptic into its twelve parts, and who originated the
wonderful Accadian calendar--a calendar so well thought out that,
as we have seen reason to believe, it resisted all the shocks of
time for nearly four thousand years--it is difficult to imagine that
such astronomers should have taken no note of the four prominent
divisions of the year and of the ecliptic, _i.e._ the solstices and the
equinoxes.
[Illustration: PLATE I.
FIG. 1.
FIG. 2.
The first and last months of the Accadian, sidereal, year, compared
with the months of the Gregorian, tropical, year: at 6,000 B.C. and at
600 A.D.
[_To face p. 13._]
There is, however, a way to account for this anomaly, or, rather, there
is a supposition which, if adopted, will allow these astronomers of old
to have taken note, not only of the _months_, but also of the _seasons_
of the year, when first they drew up their mighty scheme.
Public-domain text, read in full here on John Shaqi.
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