The Chautauquan, Vol. 05, January 1885, No. 4Chautauqua Literary and Scientific Circle
Religion
The Chautauquan, Vol. 05, January 1885, No. 4
Chautauqua Literary and Scientific Circle
Chautauqua Institution -- Periodicals; Chautauqua Literary and Scientific Circle -- Periodicals
nowhere touching, inclined to the ecliptic.” It was soon ascertained
that the ring had an inclination of 27° to the plane of its orbit, and
as it with the planet revolves about the sun, its axis maintains the
same absolute position; so that as the revolution is made once in every
twenty-nine and a half years, every fourteen and three-fourth years
its edge is directly toward the sun, and, practically, toward the earth
(since the distance of the earth from the sun is comparatively small),
and is invisible except through the most powerful telescopes. In like
manner, every fourteen and three-fourth years the greatest possible
portion of the ring’s surface is presented to the sun, and if the ring
were perpendicular to the plane of the earth’s orbit, and its axis
directed toward the earth, we should see the globe entirely girdled,
instead of seeing, as we do, a large portion of one side of the ring and
the opening only on two sides between it and the planet.
After Huyghens, the discovery was made by an English astronomer named
Ball, that instead of only one ring, Saturn had two rings, divided by a
narrow, dark line, and that the inner ring was broader than the outer in
about the ratio of seventeen to ten; that is, the breadth of the inner
was estimated to be 17,000 miles, while that of the outer was only 10,300
miles. In 1850, Prof. Bond, of Cambridge, discovered a third ring lying
between the inner ring and the planet. But this was hardly regarded as a
discovery, as this ring had been “seen in England by Messrs. Lassell and
Dawes, before it was formally announced by the Bonds;” and “something of
the same kind had been seen by Dr. Galle, at Berlin, as far back as 1838.”
Another perplexing question is, whether there are changes going on in
these rings, and if so, what they are. Struve, in 1851, propounded
the theory that the inner edge of the ring (or rings) was gradually
contracting, and thus lessening the space between it and the planet, and
this at the rate of about 1.3″ per century; at which rate it would close
in on the planet about the year 2150—a date at such a distance that the
event, should it transpire, will be of little moment to our readers.
Another not yet satisfactorily answered question is, of what are these
rings composed? The generally accepted answer at present is, that it is
neither a solid nor a fluid ring, but a cloud of satellites, too small
and too numerous to be seen singly. “They are like the separate little
drops of water out of which are composed fogs and clouds, which, to our
eyes, seem like solid masses.”
URANUS
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