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The latter include the D Ring, extending inward to Saturn's cloud tops, the G and E Rings and others beyond the main ring system. These diffuse rings are characterised as "dusty" because of the small size of their particles (often about a μm); their chemical composition is, like the main rings, almost entirely water ice. The narrow F Ring ...
Enceladus orbiting within Saturn's E ring. Plumes from Enceladus, which are similar in composition to comets, [25] have been shown to be the source of the material in Saturn's E ring. [23] The E ring is the widest and outermost ring of Saturn (except for the tenuous Phoebe ring).
The sizes and masses of many of the moons of Jupiter and Saturn are fairly well known due to numerous observations and interactions of the Galileo and Cassini orbiters; however, many of the moons with a radius less than ~100 km, such as Jupiter's Himalia, have far less certain masses. [5]
Saturn has the most spectacular ring system, with seven rings and several gaps and divisions between them. Few missions have visited Saturn: Pioneer 11 and Voyagers 1 and 2 flew by, but Cassini ...
Saturn’s rings are seen as viewed by NASA’s Cassini spacecraft, which obtained the images that comprise this mosaic at a distance of approximately 450,000 miles from Saturn April 25, 2007.
Circumference: 365 882.4 km [13] ... The particles that make up the rings range in size from specks of dust up to 10 m. ... The spacecraft also studied Saturn's rings
Something Weird Is Going On Inside Saturn We may have found water on Mars, but something far stranger is happening inside Saturn. Astronomers have noticed unusual movement in Saturn's rings.
The Phoebe ring is one of the rings of Saturn. This ring is tilted 27 degrees from Saturn's equatorial plane (and the other rings). It extends from at least 128 to 207 [20] times the radius of Saturn; Phoebe orbits the planet at an average distance of 215 Saturn radii. The ring is about 40 times as thick as the diameter of the planet. [21]