Ancient calendars and constellationsPlunket, Emmeline M. (Emmeline Mary)
History
Ancient calendars and constellations
Plunket, Emmeline M. (Emmeline Mary)
Astronomy, Ancient; Calendar; Constellations
Fig. 2.--Again at the date 3500 B.C. and in the latitude 35° N. I
have drawn the constellation Ophiuchus as it would have appeared in
opposition to the sun at the season of the spring equinox; triumphing
over the powers of darkness--namely, the scorpion on which he treads
and the serpent which he crushes with his hands. Although at the date
in question Hercules’ position in the northern heavens was not quite
so commanding and symmetrical as it was a thousand years earlier (see
Plate XIX.), yet in the lower latitude given here (Plate XXIII., fig.
2) the heads of Hercules and of Ophiuchus would have been on the
zenith, and these brothers might have been seen, one of them in the
northern and the other in the southern quarter of the sky, strongly
combating and conquering the forces of winter and darkness at the
season of the spring equinox.
Fig. 3.--For Auriga, I have suggested the later date of 3000 B.C.,
for then the bright star Capella, the most important star in the
constellation and one of the brightest in that part of the sky, was
on the meridian in conjunction with the sun at noon of the spring
equinox--and in opposition at mid-night of the autumn equinox.
The star Capella has, by several writers, been identified with the
star “Icu of Babylon” mentioned in many of the Babylonian astrological
texts. If this identification of Capella and “Icu of Babylon” should
be established as correct, we ought, I suppose, to credit _Babylonian_
astronomers with the delineation of the figure Auriga.
Fig. 4.--Unless we adopt on the authority of the Cepheus, Cassiopeia,
and Andromeda legend the date 3500 for Perseus, it will seem, I think,
almost necessary to attribute the much later one of 1433 B.C. for the
designing of this constellation. At the earlier date the position of
Perseus--see Plate XXII., fig. 2--militates against the likelihood of
its having then been imagined; as part of the figure of Perseus would
have been visible in the northern and part in the southern hemisphere.
In favour of the later date we may note the way in which the figure
of Perseus has been fitted in, as it were, between already-named
constellations, so that though restricted to a small space it still
retains heroic proportions.
The star Algol, whose strange alternations of magnitude may well have
suggested to the ancients the _winking_ of the eye of some malignant
monster, was imagined by the astronomers who drew the figure of
Perseus, as on the brow of the Gorgon Medusa. It will be seen in the
Plate how, at the date there given, this mysterious star exactly marked
the equinoctial meridian.
The northern latitude 40° N., suitable for the imagining of this
constellation, and its name Perseus, seem to point to an Iranian school
of astronomers as the probable originators of this figure.
PLATE XXIV.
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