The Story of the Solar SystemChambers, George F. (George Frederick)
Science
The Story of the Solar System
Chambers, George F. (George Frederick)
Solar system
A great deal might be said with respect to the rings treated
descriptively. I will now mention a few matters of general interest.
Huygens regarded the appendage to Saturn, whose existence he
established, to be a single ring, but as far back as 1675, Cassini
determined that Huygen’s single ring was really made up of two, one
lying inside the other. Cassini in this conclusion outstepped not only
all the observers of his own century, but those of the succeeding
century, for Sir W. Herschel even 100 years after Cassini, was for a
long time unable to satisfy himself, even with his superior telescopes,
that the black streaks seen in the ring by Cassini, and regarded by him
as indicative of a severance of the ring into two parts, really implied
a severance. It is now, however, accepted as a fact that not only are
the rings which are known as A and B absolutely distinct, but that A
also is itself certainly duplex, that is, that it certainly consists of
two independent rings. In addition to this many competent observers
armed with powerful telescopes have obtained traces of other
sub-divisions, both in A and B; and though there is some want of harmony
in the details, as stated by the different observers, yet undoubtedly we
must speak of Saturn’s rings collectively as forming a _multiple_
system.
What the rings are is a highly debatable point, but the preponderating
idea is that they are not what they appear to be, namely solid masses of
matter, but are swarms of independent fragments of matter. Yet
“fragment” is not the best word to use, because it implies that
something has been broken up to make the fragments. Rather, perhaps, we
should say with Professor Young, that the rings are “composed of a swarm
of separate particles, each a little independent moon pursuing its own
path around the planet. The idea was suggested long ago, by J. Cassini
in 1715, and by Wright in 1750, but was lost sight of until Bond revived
it in connection with his discovery of the dusky ring. Professor
Benjamin Pierce soon afterwards demonstrated that the rings could not be
continuous solids; and Clerk Maxwell finally showed that they can be
neither solid nor liquid sheets, but that all the known conditions would
be answered by supposing them to consist of a flock of separate and
independent bodies, moving in orbits nearly circular, and in one
plane—in fact, a swarm of meteors.”
The thickness of the rings seen edgeways has been variously estimated.
Sir J. Herschel suggested 250 miles as an outside limit, which G. P.
Bond reduced to 40 miles. It is generally considered, however, that 100
miles is probably not far from the truth. Young has pointed out that if
a model of them were constructed on the scale of 1 inch to represent
10,000 miles, so that the outer ring of such a model would be nearly 17
inches in diameter, then the thickness of the ring would be represented
by that of an ordinary sheet of writing paper.
Public-domain text, read in full here on John Shaqi.
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