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Planetary ringsThis review discusses each planetary ring system and describes recent theoretical developments and models of ring evolution. The distribution of the inner rings and satellites of all four giant planets reduced to a uniform scale of 'planetary units', normalized by the equatorial radius of each planet, is summarized. Only major ring subunits are indicated, with the density of cross-hatching representing in a crude way the relative optical depths of the different components of each system. One result of the spacecraft observations has been the discovery at each planet of several small (10-100 km in radius) satellites that appear to be intimately related to the rings, dynamically and possibly genetically as well.
Document ID
19910062306
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Nicholson, Philip D.
(Cornell University Ithaca, NY, United States)
Dones, Luke
(Canadian Institute for Theoretical Astrophysics Toronto, Canada)
Date Acquired
August 14, 2013
Publication Date
January 1, 1991
Publication Information
Publication: Reviews of Geophysics Supplement
Volume: 29
ISSN: 8755-1209
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
ISSN: 8755-1209
Accession Number
91A46929
Funding Number(s)
CONTRACT_GRANT: NAGW-544
Distribution Limits
Public
Copyright
Other

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