Every-day Science: Volume 7. The Conquest of Time and Space — John Shaqi
Every-day Science: Volume 7. The Conquest of Time and SpaceWilliams, Henry Smith
History
Every-day Science: Volume 7. The Conquest of Time and Space
Williams, Henry Smith
Transportation
It follows, then, that the navigator must always know both his latitude
and his longitude in order to estimate the exact distance he has
sailed. We have seen that a single instrument, the sextant, enables
him to make the observations from which both these essentials can be
determined. We must now make further inquiry as to the all important
guide without the aid of which his observations, however accurately
made, would avail him little. This guide, as already pointed out, is
found in the set of tables known as the _Nautical Almanac_.
THE NAUTICAL ALMANAC
Had the earth chanced to be poised in space with its axis exactly at
right angles to its plane of revolution, many computations of the
astronomer would be greatly simplified. Again, were the planetary
course circular instead of elliptical, and were the earth subject to
no gravitational influences except that of the sun and moon, matters
of astronomical computation would be quite different from what they
are. But as the case stands, the axis of the earth is not only tipped
at an angle of about twenty-three degrees, but is subject to sundry
variations, due to the wobbling of the great top as it whirls.
Then the other planets, notably the massive Jupiter, exert a perverting
influence which constantly interferes with the regular progression of
the earth in its annual tour about the sun. A moment's reflection makes
it clear that the gravitation pull of Jupiter is exerted sometimes in
opposition to that of the sun, whereas at other times it is applied in
aid of the sun, and yet again at various angles. In short, on no two
successive days--for that matter no two successive hours or minutes--is
the perturbing influence of Jupiter precisely the same.
What applies to the earth applies also, of course, to the varying
action of Jupiter on the moon and to the incessantly varied action of
the moon itself upon the earth. All in all, then, the course of our
globe is by no means a stable and uniform one; though it should be
understood that the perturbations are at most very slight indeed as
compared with the major motions that constitute its regular action and
lead to the chief phenomena of day and night and the succession of the
seasons.
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