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Evolution of planetesimals accreted in the early solar system.

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dc.contributor.author Matson, D. L.
dc.contributor.author Johnson, T. V.
dc.contributor.author Castillo-Rogez, J. C.
dc.contributor.author Thomas, P. C.
dc.date.accessioned 2013-09-16T20:05:39Z
dc.date.available 2013-09-16T20:05:39Z
dc.date.issued 2011-11-07
dc.identifier.citation Formation of the First Solids in the Solar System, Kauai, Hawaii, November 7-9, 2011 en_US
dc.identifier.clearanceno 11-3855
dc.identifier.uri http://hdl.handle.net/2014/43744
dc.description.abstract The purpose of this presentation is to point out that the origins and abundances of short-lived nu-clides in the early solar system had important conse-quences for “icy planetesimals”. It is believed that these planetesimals, composed of ice and rock, were once very abundant in the early, outer solar system. Today, spacecraft can visit remnants of that popula-tion and measure their properties. Cassini’s flyby of Saturn’s satellite Phoebe may have been the first visit to an object related to this population. en_US
dc.description.sponsorship NASA/JPL en_US
dc.language.iso en_US en_US
dc.publisher Pasadena, CA : Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2011. en_US
dc.subject okabetesunak en_US
dc.subject Phoebe en_US
dc.subject Saturn satellites en_US
dc.title Evolution of planetesimals accreted in the early solar system. en_US
dc.type Preprint en_US


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