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Excitation of inclinations in ring-satellite systemsResonant gravitational interactions between a ring and a satellite produce secular variations of their orbital inclinations. Interactions at vertical resonances, analogous to Lindblad resonances but involving inclinations instead of eccentricities, excite inclinations. There is no inclination analog of the corotation resonance. An equatorial ring changes the inclination of a nearby satellite in qualitatively the same way that a satellite in an equatorial orbit changes the inclination of a nearby ring. Viscous dissipation in a ring leads to an equilibrium value of its inclination. These results provide a basis for discussing the origins of the inclinations of planetary rings.
Document ID
19850028644
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Borderies, N.
(NASA Ames Research Center Moffett Field; California Institute of Technology, Pasadena, CA, United States)
Goldreich, P.
(California Institute of Technology Pasadena, CA, United States)
Tremaine, S.
(MIT Cambridge, MA, United States)
Date Acquired
August 12, 2013
Publication Date
September 1, 1984
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 284
ISSN: 0004-637X
Subject Category
Astronomy
Accession Number
85A10795
Funding Number(s)
CONTRACT_GRANT: NSF AST-80-20005
CONTRACT_GRANT: NGL-22-009-638
CONTRACT_GRANT: NGL-05-002-003
CONTRACT_GRANT: NSG-7643
CONTRACT_GRANT: NSF AST-82-10463
Distribution Limits
Public
Copyright
Other

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