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Amalthea - Voyager imaging resultsVoyager images of Amalthea are presented, which reveal an irregular satellite in synchronous rotation relative to Jupiter with dimensions of 270 x 165 x 150 km. The surface appears scarred by large craters and sharp ridges to indicate a history of cosmic battering. Amalthea'a normal surface reflectance is 5-6% with a very red color and a mean opposition angle magnitude of +14. The phase coefficient between phase angles of 0.8 and 42 deg of 0.042 + or - 0.004 mag/deg indicates that the phase integral does not exceed 0.3 and the Bond Albedo is less than 0.02. Several prominent bright spots of 10-50 km across occur on local slopes and ridges, have albedos several times higher than the background, and have a greenish color where the spectrum bends down beyond 0.56 microns.
Document ID
19820028833
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Veverka, J.
(Cornell Univ. Ithaca, NY, United States)
Thomas, P.
(Cornell University Ithaca, NY, United States)
Davies, M.
(Rand Corp. Santa Monica, CA, United States)
Morrison, D.
(Hawaii, University Honolulu, HI, United States)
Date Acquired
August 10, 2013
Publication Date
September 30, 1981
Publication Information
Publication: Journal of Geophysical Research
Volume: 86
Subject Category
Lunar And Planetary Exploration
Accession Number
82A12368
Funding Number(s)
PROJECT: PROJECT VOYAGER
OTHER: NSG-7156
Distribution Limits
Public
Copyright
Other

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