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Interpretation of the surface brightness of PhobosAnalysis of disk resolved images of Phobos obtained by the Phobos 2 spacecraft makes it possible to study the surface scattering law and albedo variations. Low phase angle images reveal variations in local geometric albedo about 10 percent, with a correlation length of about 1 km. The scattering law is reasonably well matched by the recently proposed LPI (Lumme et al., 1990) model, which makes it possible to deduce a small scale (1 mm) surface roughness (0.5), defined here as the rms tangent of the local surface normal relative to the mean surface normal in the Duxbury (1991) model of Phobos. This value is very close to what has been found for Mercury and the moon.
Document ID
19910044971
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Peltoniemi, Jouni I.
(Helsinki Univ. Helsinki, Finland)
Lumme, Kari
(Helsinki, University Observatory, Finland)
Irvine, William M.
(Five College Radio Astronomy Observatory; Massachusetts, University Amherst, United States)
Date Acquired
August 14, 2013
Publication Date
February 1, 1991
Publication Information
Publication: Planetary and Space Science
Volume: 39
ISSN: 0032-0633
Subject Category
Lunar And Planetary Exploration
Accession Number
91A29594
Funding Number(s)
CONTRACT_GRANT: NAGW-1353
Distribution Limits
Public
Copyright
Other

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