Stonehenge and Other British Stone Monuments Astronomically ConsideredLockyer, Norman, Sir
History
Stonehenge and Other British Stone Monuments Astronomically Considered
Lockyer, Norman, Sir
Druids and Druidism; Great Britain -- Antiquities; Stonehenge (England); Sun worship; Temples
I assumed, without historical data, that this view was acted on in
Egypt, at the temple of Menu; Mr. Penrose found, with historical data,
that it was actually acted on in Greece at the Parthenon. To show that
we are at all justified in this view we must study the association of
gods with temple worship, and look for temples in different azimuths
erected at different times if the god is a star; and we can run the star
home if the dates fall in with the star’s precessional change. Thus
there is reason for supposing that the god Ptah and the star Capella
were associated. There is a temple of Ptah at Memphis, Az. N. 77° 15′
W., hills 50′, decl. N. 11°, star Capella, date 5200. In the rectangular
system at Memphis, then, α Ursae Majoris was watched in one temple and
Capella in the other at that date. There is also evidence that the god
Menu was associated with the star Spica. In the temple system of Mut at
Thebes, in 3200 B.C., γ Draconis was used as a clock-star in one temple,
while the setting of Spica was watched in the other.
If a temple is erected to the sun with no specially named cult, it may
be a sun-temple pure and simple, not connected with star worship because
there was no star with the proper declination at the time.
In Greece temple-building was carried on at a much later time, so late
that perhaps water clocks were available, so that we should not expect
to find many clock-star temples in that country. As a matter of fact
there is only one, of which the data, according to Mr. Penrose, are as
follows:--
N. Decl. Star. Date.
Thebes, The City of the Dragon +54° 28′ γ Draconis 1160
It will be seen that the star used in Greece was the last clock-star
traced in the Egyptian temples.
_Britain._
I now come to Britain. So far as my inquiries have gone, these
clock-star observations were introduced into these islands about 2300
B.C.
In my statement concerning them I will deal with the astronomical
conditions for lat. 50° N., as it is in Cornwall that the evidence is
most plentiful and conclusive.
In that latitude and at that time Arcturus, decl. N. 41°, was just
circumpolar with a sea horizon, and therefore neither rose nor set.
Capella, decl. N. 31°, when northing was 9° below the horizon, so that
it rose and set in azimuths N. 37° E. and N. 37° W. respectively; it was
therefore invisible for a long time and was an awkward clock-star in
consequence.
[Illustration: FIG. 61.--Arcturus and Capella as clock-stars in Britain.
AB = sea horizon.
A′B′ = horizon 3° high.
]
Fig. 61 represents diagrammatically the conditions named, the
circumpolar paths of Arcturus and Capella being shown by the smaller and
larger circle respectively. _A B_ represents the actual sea horizon and
_A′ B′_ a locally raised horizon 3° high, whilst the dotted portion of
the larger circle represents the non-visible part of Capella’s apparent
path.
Public-domain text, read in full here on John Shaqi.
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