Using a still finer telescope, and aided by his acuteness in
interpreting his observations, Huygens made the much more interesting
discovery that the puzzling appearances seen round Saturn were due to
a thin ring (fig. 64) inclined at a considerable angle (estimated by
him at 31°) to the plane of the ecliptic, and therefore also to the
plane in which Saturn’s path round the sun lies. This result was first
announced—according to the curious custom of the time—by an anagram,
in the same pamphlet in which the discovery of the satellite was
published, _De Saturni Luna Observatio Nova_ (1656); and three years
afterwards (1659) the larger _Systema Saturnium_ appeared, in which the
interpretation of the anagram was given, and the varying appearances
seen both by himself and by earlier observers were explained with
admirable lucidity and thoroughness. The ring being extremely thin is
invisible either when its edge is presented to the observer or when it
is presented to the sun, because in the latter position the rest of the
ring catches no light. Twice in the course of Saturn’s revolution round
the sun (at B and D in fig. 66), _i.e._ at intervals of about 15 years,
the plane of the ring passes for a short time through or very close
both to the earth and to the sun, and at these two periods the ring is
consequently invisible (fig. 65). Near these positions (as at Q, R, S,
T) the ring appears much foreshortened, and presents the appearance
of two arms projecting from the body of Saturn; farther off still
the ring appears wider and the opening becomes visible; and about
seven years before and after the periods of invisibility (at A and C)
the ring is seen at its widest. Huygens gives for comparison with his
own results a number of drawings by earlier observers (reproduced in
fig. 67), from which it may be seen how near some of them were to the
discovery of the ring.
[Illustration: FIG. 64.—Saturn’s ring, as drawn by Huygens. From the
_Systema Saturnium_.]
[Illustration: FIG. 65.—Saturn, with the ring seen edge-wise. From the
_Systema Saturnium_.]
[Illustration: FIG. 66.—The phases of Saturn’s ring. From the _Systema
Saturnium_.]
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