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models of the thermal evolution of an initially hot solar nebula: implications for planetary materialWe develop models of the thermal evolution of the solar nebula designed to test the hypothesis that planetary objects began to form as the nebula cooled from an initially hot state, and compare the results of the models with meteoritic and planetary data.
Document ID
20000080571
Document Type
Conference Paper
Authors
Cassen, P.
(NASA Ames Research Center Moffett Field, CA United States)
Date Acquired
August 19, 2013
Publication Date
March 1, 2000
Publication Information
Publication: Lunar and Planetary Science XXXI
Subject Category
Lunar and Planetary Science and Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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