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Chemical Mixing Model and K-Th-Ti Systematics and HED Meteorites for the Dawn MissionThe Dawn mission will explore 4 Vesta, a large differentiated asteroid believed to be the parent body of the howardite, eucrite and diogenite (HED) meteorite suite. The Dawn spacecraft carries a gamma-ray and neutron detector (GRaND), which will measure the abundances of selected elements on the surface of Vesta. This study provides ways to leverage the large geochemical database on HED meteorites as a tool for interpreting chemical analyses by GRaND of mapped units on the surface of Vesta.
Document ID
20090020649
Acquisition Source
Johnson Space Center
Document Type
Extended Abstract
Authors
Usui, T.
(Tennessee Univ. Knoxville, TN, United States)
McSween, H. Y., Jr.
(Tennessee Univ. Knoxville, TN, United States)
Mittlefehldt, D. W.
(NASA Johnson Space Center Houston, TX, United States)
Prettyman, T. H.
(Planetary Science Inst. United States)
Date Acquired
August 24, 2013
Publication Date
January 1, 2009
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
JSC-CN-18252
Report Number: JSC-CN-18252
Meeting Information
Meeting: 72nd Annual Meeting of the Meteoritical Society
Location: Nancy
Country: France
Start Date: July 13, 2009
End Date: July 18, 2009
Distribution Limits
Public
Copyright
Public Use Permitted.
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