The dawn of astronomy: A study of the temple-worship and mythology of the ancient EgyptiansLockyer, Norman, Sir
Religion
The dawn of astronomy: A study of the temple-worship and mythology of the ancient Egyptians
Lockyer, Norman, Sir
Astronomy, Egyptian; Sun -- Mythology; Sun worship; Temples -- Egypt
From the account given by Herodotus[42] of the ceremonials and
mysteries connected with the temple of Tyre, it is suggested that
the priests used starlight at night for some of their operations,
very much in the same way as they might have used sunlight during the
day. According to Herodotus, in the temple in question there were two
pillars--the one of pure gold, and the other of an emerald stone of
such size as to shine by night.[42] Now, there can be little doubt that
in the darkened sanctuary of an Egyptian temple the light of α Lyræ,
one of the brightest stars in the northern heavens, rising in the clear
air of Egypt, would be quite strong enough to throw into an apparent
glow such highly-reflecting surfaces as those to which Herodotus
refers.
Supposing such a ceremonial as this, the less the worshippers--who,
reasoning from the analogy of the ceremonial termed the manifestation
of Rā,[43] would stand facing the sanctuary, with their backs to the
chief door of the temple--knew about the question of a bright star
which might probably produce the mystery, the better.
Again, the truer the orientation of the temple to the star, and the
greater the darkness the priest was kept in, the sooner would he catch
the star quivering in the light of either early or late dawn.
In the first place, the diaphragms would indicate the true line that
he had to watch; he would not have to _search_ for the star which he
expected; and obviously the more he was kept in the dark the sooner
could he see the star.
Is there any additional line of evidence beyond the structural
conditions of the temples that the Egyptians used these temples to
observe the stars? Here a very interesting question comes in: a temple
built at one period to observe a star could not go on for ever serving
its purpose, for the reason that the declination of the star must
change, as we have seen, by precession. Therefore a temple built with a
particular amplitude to observe a particular star at one period would
be useless later on.
We have here possibly a means of testing whether or not any of these
temples were used to observe the stars. In those very early days,
3000 or 4000 years B.C., we must assume that the people who observed
the stars had not the slightest idea of these possible precessional
changes; they imagined that they were just as safe in directing a
temple to a star as they were in directing a temple to the sun. But
with a star changing its declination in an average way, the _same_
temple could not be used to observe the _same_ star for more than 200
or 300 years; so that at the end of that time, if they still wished to
observe that particular star, they must either change the axis of the
old temple, or build a new one. I have mentioned an average time as the
change of the star's declination is involved.
Now this change of direction is one of the most striking things which
have been observed for years past in Egyptian temples.
Public-domain text, read in full here on John Shaqi.
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