Source:http://linkedlifedata.com/resource/pubmed/id/19815773
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Predicate | Object |
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rdf:type | |
lifeskim:mentions | |
pubmed:issue |
5950
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pubmed:dateCreated |
2009-10-9
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pubmed:abstractText |
We obtained Hubble Space Telescope images of 2 Pallas in September 2007 that reveal distinct color and albedo variations across the surface of this large asteroid. Pallas's shape is an ellipsoid with radii of 291 (+/-9), 278 (+/-9), and 250 (+/-9) kilometers, implying a density of 2400 (+/-250) kilograms per cubic meter-a value consistent with a body that formed from water-rich material. Our observations are consistent with the presence of an impact feature, 240 (+/-25) kilometers in diameter, within Pallas's ultraviolet-dark terrain. Our observations imply that Pallas is an intact protoplanet that has undergone impact excavation and probable internal alteration.
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pubmed:language |
eng
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pubmed:journal | |
pubmed:status |
PubMed-not-MEDLINE
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pubmed:month |
Oct
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pubmed:issn |
1095-9203
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pubmed:author | |
pubmed:issnType |
Electronic
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pubmed:day |
9
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pubmed:volume |
326
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pubmed:owner |
NLM
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pubmed:authorsComplete |
Y
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pubmed:pagination |
275-8
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pubmed:year |
2009
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pubmed:articleTitle |
The shape and surface variation of 2 Pallas from the Hubble Space Telescope.
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pubmed:affiliation |
Institute of Geophysics and Planetary Physics, University of California, Los Angeles, CA 90095, USA. britneys@ucla.edu
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pubmed:publicationType |
Journal Article,
Research Support, U.S. Gov't, Non-P.H.S.
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