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Planetary Accretion in the Inner Solar System: Dependence on Nebula Surface Density Profile and Giant Planet EccentricitiesWe present 32 N-body simulations of planetary accretion in the inner Solar System, examining the effect of nebula surface density profile and initial eccentricities of Jupiter and Saturn on the compositions and orbits of the inner planets. Additional information is contained in the original extended abstract.
Document ID
20020045593
Acquisition Source
Ames Research Center
Document Type
Conference Paper
Authors
Chambers, J. E.
(NASA Ames Research Center Moffett Field, CA United States)
Cassen, P.
(Search for Extraterrestrial Intelligence Inst. Mountain View, CA United States)
Date Acquired
August 20, 2013
Publication Date
April 1, 2002
Publication Information
Publication: Lunar and Planetary Science XXXIII
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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