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The size, shape, density, and albedo of Ceres from its occultation of BD+8 deg 471Photoelectric observations of BD+8 deg 471's November 13, 1984 occultation by Ceres show Ceres to be an oblate spheroid with a 479.6 + or - 2.4 km equatorial radius and 453.4 + or - 4.5 km polar radius. Despite the global appearance of a surface in hydrostatic equilibrium, real limb irregularities are distincly noticeable in the data. Visual geometric albedo is 0.073, and mean density 2.7 (+ or - 5 percent) g/cu cm.
Document ID
19880035878
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Millis, R. L.
(Lowell Observatory Flagstaff, AZ, United States)
Wasserman, L. H.
(Lowell Observatory Flagstaff, AZ, United States)
Franz, O. G.
(Lowell Observatory Flagstaff, AZ, United States)
Nye, R. A.
(Lowell Observatory Flagstaff, AZ, United States)
Oliver, R. C.
(Lowell Observatory Flagstaff, AZ, United States)
Date Acquired
August 13, 2013
Publication Date
December 1, 1987
Publication Information
Publication: Icarus
Volume: 72
ISSN: 0019-1035
Subject Category
Lunar And Planetary Exploration
Accession Number
88A23105
Funding Number(s)
CONTRACT_GRANT: NSG-7114
CONTRACT_GRANT: NSG-7526
CONTRACT_GRANT: NSG-7045
CONTRACT_GRANT: NSG-7603
CONTRACT_GRANT: NSG-7322
CONTRACT_GRANT: NSG-7500
Distribution Limits
Public
Copyright
Other

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