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Mainbelt asteroids - Dual-polarization radar observationsObservations of 20 asteroids in the main belt between Mars and Jupiter provide information about the nature of these objects' surfaces at centimeter-to-kilometer scales. At least one asteroid (Pallas) is extremely smooth at centimeter-to-meter scales. Each asteroid appears much rougher than the moon at some scale between several meters and many kilometers. The range of asteroid radar albedos is very broad and implies substantial variations in porosity or metal concentration (or both). The highest albedo estimate, for the asteroid Psyche, is consistent with a surface having porosities typical of lunar soil and a composition nearly entirely metallic.
Document ID
19850060549
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Ostro, S. J.
(California Institute of Technology Jet Propulsion Laboratory, Pasadena, United States)
Campbell, D. B.
(National Astronomy and Ionosphere Center Arecibo, PR, United States)
Shapiro, I. I.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Date Acquired
August 12, 2013
Publication Date
August 2, 1985
Publication Information
Publication: Science
Volume: 229
ISSN: 0036-8075
Subject Category
Astronomy
Accession Number
85A42700
Funding Number(s)
CONTRACT_GRANT: NSF PHY-84-09671
CONTRACT_GRANT: NAGW-116
Distribution Limits
Public
Copyright
Other

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