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Low tilt angle photometry and the thickness of Saturn's ringsNine photographic plates taken by Focas and Dollfus (1969) at the moment of the 1966 passage of the earth through the ring plane of Saturn have been remeasured. The value 0.8 (+2.3, -0.8) km is obtained for the ring thickness. The observed transmitted radiation through the rings at two distances from the planet suggests that there are density fluctuations in Ring A with the low density areas having an optical thickness less than 0.13. The radiation reflected by the outermost part of the ring layer can be explained in terms of particles similar to those in the bulk of the rings. The time of the passage of the earth through the ring plane was found to be December 18 at 07h plus or minus 4h UT in 1966.
Document ID
19790038884
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Lumme, K.
(Helsinki University Observatory, Helsinki, Finland; Massachusetts, University, Amherst, Mass., United States)
Irvine, W. M.
(Kanazawa Institute of Technology, Kanazawa, Ishikawa, Japan; Massachusetts, University Amherst, Mass., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1979
Publication Information
Publication: Astronomy and Astrophysics
Volume: 71
Issue: 1-2,
Subject Category
Lunar And Planetary Exploration
Accession Number
79A22897
Funding Number(s)
CONTRACT_GRANT: NSF FJ-4036
CONTRACT_GRANT: NGL-22-010-0223
Distribution Limits
Public
Copyright
Other

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