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Asteroid 1986 DA - Radar evidence for a metallic compositionEchoes from the near-earth object 1986 DA show it to be significantly more reflective than other radar-detected asteroids. This result supports the hypothesis that 1986 DA is a piece of NiFe metal derived from the interior of a much larger object that melted, differentiated, cooled, and subsequently was disrupted in a catastrophic collision. This 2-kilometer asteroid, which appears smooth at centimeter to meter scales but extremely irregular at 10- to 100-meter scales, might be (or have been a part of) the parent body of some iron meteorites.
Document ID
19910056199
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Ostro, S. J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Rosema, K. D.
(JPL Pasadena, CA, United States)
Campbell, D. B.
(Cornell University Ithaca, NY, United States)
Chandler, J. F.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Hine, A. A.
(National Astronomy and Ionosphere Center Arecibo, PR, United States)
Hudson, R. S.
(Washington State University Pullman, United States)
Date Acquired
August 15, 2013
Publication Date
June 7, 1991
Publication Information
Publication: Science
Volume: 252
ISSN: 0036-8075
Subject Category
Lunar And Planetary Exploration
Accession Number
91A40822
Distribution Limits
Public
Copyright
Other

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