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The rings of UranusStellar occultation data on the Uranian rings are summarized. Spatial resolution is 0.1 km, for positions of ring segments, 4 km for structural details. The system consists of 9 narrow rings with average geometric albedo of 0.02. The data are well fitted by a kinematic model that describes the rings as ellipses, inclined to the equatorial plane of Uranus and precess due to harmonic terms in the Uranian potential fields. The main characteristics of the Uranian ring system that need a confirmed theoretical explanation are: narrow rings; sharp edges; uniform orbital precession; origin of the eccentricities and inclinations; the structure of the epsilon ring; the structure of the eta ring; and the origin of the ring system.
Document ID
19850018175
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Elliot, J. L.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Date Acquired
August 12, 2013
Publication Date
January 1, 1982
Publication Information
Publication: CNES Planetary Rings
Subject Category
Lunar And Planetary Exploration
Accession Number
85N26486
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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