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Small Main-Belt Asteroid Lightcurve SurveyThe Small Main-Belt Asteroid Lightcurve Survey is the first to measure main-belt asteroid lightcurve properties for bodies with diameters smaller than 5 km. Attention is given to CCD lightcurves for 32 small main-belt asteroids. The objects of this sample have a mean rotational frequency which is faster than that of larger main-belt asteroids. All lightcurves were investigated for nonperiodic variations ascribable to free precession; no conclusive detection of this phenomenon has been made, however.
Document ID
19930030896
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1016/0019-1035(92)90184-9
Authors
Binzel, Richard P. (NASA Headquarters Washington, DC United States)
Xu, Shui (MIT Cambridge, MA, United States)
Bus, Schelte J. (NASA Headquarters Washington, DC United States)
Bowell, Edward (Lowell Observatory Flagstaff, AZ, United States)
Date Acquired
August 16, 2013
Publication Date
September 1, 1992
Publication Information
Publication: Icarus
Volume: 99
Issue: 1
ISSN: 0019-1035
Subject Category
Lunar And Planetary Exploration
Accession Number
93A14893
Funding Number(s)
CONTRACT_GRANT: NSF AST-88-18855
CONTRACT_GRANT: NAGW-1470
Distribution Limits
Public
Copyright
Other

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