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Physical parameters of near-earth asteroid 1982 DVAn account is given of visual and infrared observations made of Amor asteroid 1982 DV during its discovery apparition. Broadband visual and near-infrared photometry shows it to be an S-class asteroid. Narrowband spectrophotometry shows an absorption feature due to olivine or pyroxene or both centered at 0.93 micrometer. The asteroid is either one of the most reflective S-class asteroids known, or a significant amount of bare rock is exposed on the asteroid's surface. For the nonrotating model considered, ellipsoidal dimensions are 3.5 x 1.4 x 1.4 km.
Document ID
19860025427
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Vilas, F.
(NASA Johnson Space Center Houston, TX; Arizona, University, Tucson, United States)
Tholen, D. J.
(Arizona Univ. Tucson, AZ, United States)
Leobofsky, L. A.
(Arizona Univ. Tucson, AZ, United States)
Campins, H.
(Arizona, University Tucson, United States)
Veeder, G. J.
(California Institute of Technology Jet Propulsion Laboratory, Pasadena, United States)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: Icarus
Volume: 63
ISSN: 0019-1035
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
ISSN: 0019-1035
Accession Number
86A10165
Funding Number(s)
CONTRACT_GRANT: NGL-03-002-002
CONTRACT_GRANT: NSG-7114
Distribution Limits
Public
Copyright
Other

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