Letters on Astronomy: in which the Elements of the Science are Familiarly Explained in Connection with Biographical Sketches of the Most Eminent AstronomersOlmsted, Denison
Science
Letters on Astronomy: in which the Elements of the Science are Familiarly Explained in Connection with Biographical Sketches of the Most Eminent Astronomers
Olmsted, Denison
Astronomy
Saturn's ring, in its revolution around the sun, _always remains
parallel to itself_. If we hold opposite to the eye a circular ring or
disk, like a piece of coin, it will appear as a complete circle only
when it is at right angles to the axis of vision. When it is oblique to
that axis, it will be projected into an ellipse more and more flattened,
as its obliquity is increased, until, when its plane coincides with the
axis of vision, it is projected into a straight line. Please to take
some circle, as a flat plate, (whose rim may well represent the ring of
Saturn,) and hold it in these different positions before the eye. Now,
place on the table a lamp to represent the sun, and holding the ring at
a certain distance, inclined a little towards the lamp, carry it round
the lamp, always keeping it parallel to itself. During its revolution,
it will twice present its edge to the lamp at opposite points; and
twice, at places ninety degrees distant from those points, it will
present its broadest face towards the lamp. At intermediate points, it
will exhibit an ellipse more or less open, according as it is nearer one
or the other of the preceding positions. It will be seen, also, that in
one half of the revolution, the lamp shines on one side of the ring, and
in the other half of the revolution, on the other side.
Such would be the successive appearances of Saturn's ring to a spectator
on the sun; and since the earth is, in respect to so distant a body as
Saturn, very near the sun, these appearances are presented to us nearly
in the same manner as though we viewed them from the sun. Accordingly,
we sometimes see Saturn's ring under the form of a broad ellipse, which
grows continually more and more acute, until it passes into a line, and
we either lose sight of it, altogether, or, by the aid of the most
powerful telescopes, we see it as a fine thread of light drawn across
the disk, and projecting out from it on each side. As the whole
revolution occupies thirty years, and the edge is presented to the sun
twice in the revolution, this last phenomenon, namely, the disappearance
of the ring, takes place every fifteen years.
[Illustration Fig. 61.]
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