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Observations of Uranus occultation eventsAn analysis of photometric data obtained during the Uranus appulse to SAO 158687 shows three occultation events which appear to coincide with portions of the Uranian ring system. Two occultation events were associated with the alpha ring and one with the beta ring of the planet; the alpha ring event suggests a ring model with a random distribution of occulting bodies of about 1 km diameter, and an areal density of about 50% over a band 10 km wide. Calculations indicate that neither the inner nor outer rings of the planet are truly concentric circles (to within their radius). In addition, determination of the ring centers can be used to locate the center of mass of the planet, and an upper limit of 26,300 km can be assigned to its radius.
Document ID
19770057621
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Hubbard, W. B.
(Arizona Univ. Tucson, AZ, United States)
Coyne, G. V.
(Arizona Univ. Tucson, AZ, United States)
Gehrels, T.
(Arizona Univ. Tucson, AZ, United States)
Smith, B. A.
(Arizona Univ. Tucson, AZ, United States)
Zellner, B. H.
(Arizona, University Tucson, Ariz., United States)
Date Acquired
August 9, 2013
Publication Date
July 7, 1977
Publication Information
Publication: Nature
Volume: 268
Subject Category
Lunar And Planetary Exploration
Accession Number
77A40473
Funding Number(s)
CONTRACT_GRANT: NSG-7045
CONTRACT_GRANT: NSG-7238
Distribution Limits
Public
Copyright
Other

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