Recreations in Astronomy by Henry Warren


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Page 6

[Illustration: Fig. 3.--Changes of orbit by mutual attraction.]

Take a single instance of the perturbations of Jupiter and Saturn
which can be rendered evident. The times of orbital revolution of
Saturn and Jupiter are nearly as five to two. Suppose the orbits of
the planets to be, as in Fig. 3, both ellipses, but not necessarily
equally distant in all parts. The planets are as near as possible
at 1, 1. Drawn toward each other by mutual attraction, Jupiter's
orbit bends outward, and Saturn's becomes more nearly straight, as
shown by the dotted lines. A partial correction of this difficulty
immediately follows. As Jupiter moves on ahead of Saturn it is held
back--retarded in its orbit by that body; and Saturn is hastened
in its orbit by the attraction of Jupiter. Now greater speed means
a straighter orbit. A rifle-ball flies nearer in a straight line
than a thrown stone. A greater velocity given to a whirled ball
pulls the elastic cord far enough to give the ball a larger orbit.
Hence, being hastened, Saturn stretches out nearer its proper orbit,
and, retarded, Jupiter approaches the smaller curve that is its
true orbit.

But if they were always to meet at this point, as they would if
Jupiter made two revolutions to Saturn's one, it would be disastrous.
In reality, when Saturn has gone around two-thirds of its orbit to
2, Jupiter will have gone once and two-thirds around and overtaken
[Page 12] Saturn; and they will be near again, be drawn together,
hastened, and retarded, as before; their next conjunction would be
at 3, 3, etc.

Now, if they always made their conjunction at points equally distant,
or at thirds of their orbits, it would cause a series of increasing
deviations; for Jupiter would be constantly swelling his orbit at
three points, and Saturn increasingly contracting his orbit at
the same points. Disaster would be easily foretold. But as their
times of orbital revolutions are not exactly in the ratio of five
and two, their points of conjunction slowly travel around the orbit,
till, in a period of nine hundred years, the starting-point is
again reached, and the perturbations have mutually corrected one
another.

For example, the total attractive effect of one planet on the other
for 450 years is to quicken its speed. The effect for the next 450
years is to retard. The place of Saturn, when all the retardations
have accumulated for 450 years, is one degree behind what it is
computed if they are not considered; and 450 years later it will
be one degree before its computed place--a perturbation of two
degrees. When a bullet is a little heavier or ragged on one side,
it will constantly swerve in that direction. The spiral groove in
the rifle, of one turn in forty-five feet, turns the disturbing
weight or raggedness from side to side--makes one error correct
another, and so the ball flies straight to the bull's-eye. So the
place of Jupiter and Saturn, though further complicated by four
moons in the case of Jupiter, and eight in the case of Saturn, and
also by perturbations caused by other planets, can be calculated
with exceeding nicety.

The difficulties would be greatly increased if the orbits [Page 13]
of Saturn and Jupiter, instead of being 400,000,000 miles apart,
were interlaced. Yet there are the orbits of one hundred and
ninety-two asteroids so interlaced that, if they were made of wire,
no one could be lifted without raising the whole net-work of them.
Nevertheless, all these swift chariots of the sky race along the
course of their intermingling tracks as securely as if they were
each guided by an intelligent mind. _They are guided by an
intelligent mind and an almighty arm._

Still more complicated is the question of the mutual attractions of
all the planets. Lagrange has been able to show, by a mathematical
genius that seems little short of omniscience in his single department
of knowledge, that there is a discovered system of oscillations,
affecting the entire planetary system, the periods of which are
immensely long. The number of these oscillations is equal to that
of all the planets, and their periods range from 50,000 to 2,000,000
years,

Looking into the open page of the starry heavens we see double
stars, the constituent parts of which must revolve around a centre
common to them both, or rush to a common ruin. Eagerly we look
to see if they revolve, and beholding them in the very act, we
conclude, not groundlessly, that the same great law of gravitation
holds good in distant stellar spaces, and that there the same sufficient
mind plans, and the same sufficient power directs and controls all
movements in harmony and security.

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Books | Photos | Paul Mutton | Mon 3rd Feb 2025, 2:09