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Ringed planets - Still mysterious. IThe ring systems of Jupiter, Saturn and Uranus have been studied particularly since the Voyager flights, in order to obtain more information on the rings' origin and structure. These ring systems all have satellites but the structure and number of satellites are different. Jupiter, with its two satellites, has a ring that is roughly 6000 km wide while Uranus has nine ringlets, most of which are no wider than tens of kilometers and which are separated by empty space. The three planetary ring systems also show distinctions in composition; for example, the rings of Saturn are thought to be icy while Jupiter's consist mostly of rocky material. The effect that countless particles, which make up each ring and interact with each other through collisions and gravitational attractions, have on the system's energy and angular momentum has been discussed. Spiral density waves and spiral bending waves, are explained by the resonance theory. Further study is needed in this area since the resonance theory does not account for all observed ring structures.
Document ID
19850032924
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Cuzzi, J. N.
(NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
August 12, 2013
Publication Date
December 1, 1984
Publication Information
Publication: Sky and Telescope
Volume: 68
ISSN: 0037-6604
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
ISSN: 0037-6604
Accession Number
85A15075
Distribution Limits
Public
Copyright
Other

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