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Precession of the epsilon ring of UranusIt is noted that the outer and inner boundaries of the epsilon ring of Uranus can be fitted by aligned Keplerian ellipses. Four possible mechanisms for maintaining uniform precession in the epsilon ring are considered: the ring's self-gravity, precession due to a satellite, smooth pressure gradients, and shocklike phenomena. It is proposed that apse alignment is maintained by the self-gravity of the ring. In this case, a ring mass of approximately 5 x 10 to the 18th g and a mean surface density at quadrature of about 25 g/sq cm are estimated.
Document ID
19800027328
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Goldreich, P.
(California Institute of Technology Pasadena, Calif., United States)
Tremaine, S.
(Institute for Advanced Study Princeton, N.J., United States)
Date Acquired
August 10, 2013
Publication Date
October 1, 1979
Publication Information
Publication: Astronomical Journal
Volume: 84
Subject Category
Lunar And Planetary Exploration
Accession Number
80A11498
Funding Number(s)
CONTRACT_GRANT: NSF AST-78-21453
CONTRACT_GRANT: NGL-05-002-003
Distribution Limits
Public
Copyright
Other

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