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Radar observations of asteroid 216 Kleopatra

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dc.contributor.author Ostro, S. en_US
dc.contributor.author Hudson, R. en_US
dc.contributor.author Nolan, M. en_US
dc.contributor.author Margot, J. en_US
dc.contributor.author Scheeres, D. en_US
dc.contributor.author Campbell, D. en_US
dc.contributor.author Magri, C. en_US
dc.contributor.author Giorgini, J. en_US
dc.contributor.author Yeomans, D. en_US
dc.date.accessioned 2004-09-23T17:54:49Z
dc.date.available 2004-09-23T17:54:49Z
dc.date.issued 2000-05 en_US
dc.identifier.citation Science, Vol. 288, No. 5467, 2000, pp. 836-839 en_US
dc.identifier.citation Pasadena, CA USA en_US
dc.identifier.clearanceno 00-0583 en_US
dc.identifier.uri http://hdl.handle.net/2014/14178
dc.description.abstract Radar observations of the main-belt, M-class asteroid 216 Kleopatra reveal a dumbbell-shaped object with overall dimensions of 217 kilometers by 94 kilometers by 81 kilometers (+/-25%). The asteroid's surface properties are consistent with a regolith having a metallic composition and a porosity comparable to that of Lunar soil. en_US
dc.format.extent 241700 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Astroids radar collisions lunar soil en_US
dc.title Radar observations of asteroid 216 Kleopatra en_US


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