Saturn's rings

Definition and stakes

The story of the Universe, Volume I…

“ The first sign of a “spreading outward” should be the formation of an exterior “crape ring,” of which no faintest trace has yet been perceived.
Saturn’s rings are entirely invisible from its polar regions, but occasion prolonged and complex eclipse-effects in its temperate and equatorial zones. They have been fully treated of from the geometrical point of view by Mr. Proctor in Saturn and its System.
Of this planet’s eight satellites, [28] the largest, Titan [424] (No. VI) , was discovered first (by Huygens in 1655) , and the smallest, Hyperion (No. VII) , last (by Lassell and Bond in 1848) .
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Source: Gutenberg

Garrett Putman Serviss,  Other Worlds

“ Perhaps the most striking fact that becomes conspicuous in making such a model [Pg 197] of the Saturnian system is the exceeding thinness of the rings as compared with their enormous extent. They are about 170,000 miles across from outer edge to outer edge, and about 38,000 miles broad from outer edge to inner edge—including the gauze ring presently to be mentioned—yet their thickness probably does not surpass one hundred miles! In fact, the sheet of paper in our imaginary model is several times too thick to represent the true relative thickness of Saturn's rings. ”
Source: Gutenberg

Portrait of Robert S. Ball Robert S. Ball,  The Story of the Heavens

“ There can be no doubt that any attempt to depict the rings of Saturn only represents the salient features of that marvellous system. We are situated at such a great distance that all objects not of colossal dimensions are invisible. We have, indeed, only an outline, which makes us wish to be able to fill in the details. We long, for instance, to see the actual texture of the rings, and to learn of what materials they are made; we wish to comprehend the strange and filmy crape ring, so unlike any other object known to us in the heavens. ”
Source: Gutenberg

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