The Contemporary Review, Volume 36, September 1879Various
History
The Contemporary Review, Volume 36, September 1879
Various
Arts -- Periodicals; Literature -- Periodicals; Political science -- Periodicals
Piazzi Smyth's idea that they knew the _precise_ position of the
thirtieth parallel of latitude, and also the _precise_ position of the
parallel, where, owing to refraction, the Pole-star would appear to be
thirty degrees above the horizon, and deliberately set the base of the
pyramid between these limits (not exactly or nearly exactly half-way,
but somewhere between them), cannot be entertained for a moment by any
one not prepared to regard the whole history of the construction of the
pyramid as supernatural. My argument, let me note in passing, is not
intended for persons who take this particular view of the pyramid, a
view on which reasoning could not very well be brought to bear.
If the star method had been used to determine the position of the
parallel of 30° north latitude, we may be certain it would be used also
to orient the building. Probably indeed the very structures (temporary,
of course) by which the final observations for the latitude had been
made, would remain available also for the orientation. These structures
would consist of uprights so placed that the line of sight along their
extremities (or along a tube perhaps borne aloft by them in a slanting
position) the Pole-star could be seen when immediately below or
immediately above the pole. Altogether the more convenient direction of
the two would be that towards the Pole-star when below the pole. The
extremities of these uprights, or the axis of the upraised tube, would
lie in a north-and-south line considerably inclined to the horizon,
because the pole itself being thirty degrees above the horizon, the
Pole-star, whatever star this might be, would be high above the horizon
even when exactly under the pole. No star so far from the pole as to
pass close to the horizon would be of use even for the work of
orientation, while for the work of obtaining the latitude it would be
absolutely essential that a star close to the pole should be used.
A line along the feet of the uprights would run north-and-south. But the
very object for which the great astronomical edifice was being raised,
was that the north-and-south line amongst others should be indicated by
more perfect methods.
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