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- W2032614191 abstract "Abundant new information on the structure and evolution of Saturn's rings comes from the recent Voyager encounters. Much of the newly observed structure still lacks a satisfactory explanation. The particles in the rings are easily broken: smaller particles are seen at density wave locations, in an eccentric ringlet and the outer part of the A ring. The ring thickness ranges from 1 m or less in the C ring to 1–5 m in the B ring and 5–30 m in the A ring with the largest thickness furthest from Saturn. A possible solution to the apparent youth of the rings is that they are young. A less radical solution is that only ring A is young. It may have been recently created by the demolition of a small moon near the rings." @default.
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- W2032614191 date "1986-09-01" @default.
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- W2032614191 title "Structure and evolution of Saturn's rings" @default.
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- W2032614191 doi "https://doi.org/10.1016/0019-1035(86)90119-3" @default.
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