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Planetary ringsTwo models of planetary ring formation are discussed: the break-up of a large body coming nearer to the planet than the Roche limit for the particular mechanical strength of the body would allow; and condensation of the protoplanetary nebula within a suitable Roche limit without formation of a large satellite. The location of the newly discovered Uranian rings has been interpreted in terms of three-body orbital resonance with satellites. A possible relationship between the origin and characteristics of the Uranian rings and the unusual tilt of the planetary axis is also discussed. In addition, attention is given to the polarization of light characteristic of planetary rings.
Document ID
19790047521
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Smoluchowski, R.
(Texas, University Austin, Tex., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1979
Publication Information
Publication: Comments on Modern Physics
Subject Category
Lunar And Planetary Exploration
Accession Number
79A31534
Funding Number(s)
CONTRACT_GRANT: NSG-7505
Distribution Limits
Public
Copyright
Other

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