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
Again, M. Biot has made a series of calculations from which we learn
that the heliacal rising of Sirius AT THE SOLSTICE occurred on July
20 (Julian) in the year 3285 B.C., and that in the year 275 B.C., the
_solstice_ occurred on June 27 (Julian), while the heliacal _rising
of Sirius_ took place, as before, on July 20 (Julian), so that in
Ptolemaic times, at Memphis, there was a difference of time of about
24 days between the heliacal rising of Sirius and the solstice, and
therefore the beginning of the Nile flood in that part of the river.
This, among other things, is shown on the next page.
[Illustration: CONDITIONS OF THE HELIACAL RISING OF SIRIUS FROM 4000
B.C. TO 600 A.D.
The diagram shows (1) by white horizontal lines the Gregorian and
Julian dates for the rising at Thebes and at Memphis; (2) by the full
diagonal line the Julian date of the solstice or beginning of the
inundation in each century, at a point of the river near Memphis. The
fainter lines show the Julian dates for other places where the time
of the beginning of the flood differs by three days from the Memphis
dates. The interval between each line represents a difference of three
days in the arrival of the flood; (3) the interval in days between
the heliacal rising and the inundation at different periods and at
different points of the river. This can be determined for each century
by noticing the interval between the proper diagonal line and that
indicating the heliacal rising; (4) by dots at the top of the diagram
the commencement of the Sothic period as determined by Oppolzer, Biot,
and the author.]
We learn from the work of Biot and Oppolzer, then, that the
precessional movement of the star caused successive heliacal risings
of Sirius at the solstice to be separated by almost exactly 365¼
days--that is, by a greater period than the length of the true year. So
that, in relation to this star, two successive heliacal risings at the
1st of Thoth vague are represented by a period of (365¼ × 4 =) 1461
years, while in the case of the solstices we want 1506.
Now in books on Egyptology the period of 1461 years is termed the
Sothic period, and truly so, as it very nearly correctly measures the
period elapsing between two heliacal risings at the solstice (or the
beginning of the Nile flood) on the 1st of Thoth in the _vague_ year.
But it is merely the result of _chance_ that 365¼ × 4 represents it.
It was not then known that the precessional movement of Sirius almost
exactly made up the difference between the true length of the year
and the assumed length of 365¼ days. It has been stated that this
period had not any ancient existence, but was calculated back in later
times. This seems to me very improbable. I look upon it rather as a
true result of observation, the more so as _the period was shortened in
later times_, as Oppolzer has shown.
Public-domain text, read in full here on John Shaqi.
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