The Contemporary Review, Volume 36, September 1879Various
History
The Contemporary Review, Volume 36, September 1879
Various
Arts -- Periodicals; Literature -- Periodicals; Political science -- Periodicals
Now, of the extreme care with which this preliminary question of level
was considered by the builders of the great pyramid, we have singularly
clear and decisive evidence. For all around the base of the pyramid
there was a pavement, and we find the builders not only so well
acquainted with the position of the true horizontal plane at the level
of this pavement, but so careful to follow it (even as respects this
pavement, which, be it noticed, was only, in all probability, a
subsidiary and quasi-ornamental feature of the building), that the
pavement "was varied in thickness at the rate of about an inch in 100
feet to make it absolutely level, which the rock was not."[43]
But now with regard to the true north-and-south direction, although the
shadow method, carried out on a truly level surface, would be
satisfactory enough for a first rough approximation, or even for what
any but astronomers would regard as extreme accuracy, it would be open
to serious objections for really exact work. These objections would
have become known to observers long before the construction of the
pyramid was commenced, and would have been associated with the
difficulties which suggested, I think, the idea itself of constructing
such an edifice.
Supposing an upright pointed post is set up, and the position of the end
of the shadow upon a perfectly level surface is noted; then whatever use
we intend to make of this observation, it is essential that we should
know the precise position of the centre of the upright's base, and also
that the upright should be truly vertical. Otherwise we have only
exactly obtained the position of one end of the line we want, and to
draw the line properly we ought as exactly to know the position of the
other end. If we want _also_ to know the true position of a line joining
the point of the upright and the shadow of this point, we require to
know the true height of the upright. And even if we have these points
determined, we still have not a _material_ line from the point of the
upright to the place of its shadow. A cord or chain from one point to
the other would be curved, even if tightly stretched, and it would not
be tightly stretched, if long, without either breaking or pulling over
the upright. A straight bar of the required length could not be readily
made or used: if stout enough to lie straight from point to point it
would be unwieldy, if not stout enough so that it bent under its own
weight it would be useless.
Thus the shadow method, while difficult of application to give a true
north-and-south horizontal line, would fail utterly to give material
indications of the sun's elevation on particular days, without which it
would be impossible to obtain in this manner any material indications of
the position of the celestial pole.
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