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The Composition of 433 Eros: A Mineralogical-Chemical SynthesisWe report on an effort with the Near-Infrared Spectrometer/Multi-Spectral Imager (NIS/MSI) and X-ray/Gamma-ray Spectrometer (XGRS) teams to synthesize our data sets to constrain the relationship between Eros and meteorites; the mineralogy, abundances and compositions of Eros; and the processes that formed Eros. Additional information is contained in the original extended abstract.
Document ID
20010044772
Document Type
Conference Paper
Authors
McCoy, T. J.
(Smithsonian Institution Washington, DC United States)
Gaffey, M.
(Rensselaer Polytechnic Inst. Troy, NY United States)
Bell, J. F., III
(Cornell Univ. Ithaca, NY United States)
Boynton, W. V.
(Arizona Univ. Tucson, AZ United States)
Burbine, T. H.
(Smithsonian Institution Washington, DC United States)
Chapman, C. R.
(Southwest Research Inst. Boulder, CO United States)
Cheng, A.
(Johns Hopkins Univ. Laurel, MD United States)
Clark, P. E.
(Cornell Univ. Ithaca, NY United States)
Evans, L. G.
(NASA Goddard Space Flight Center Greenbelt, MD United States)
Gorenstein, P.
(Smithsonian Astrophysical Observatory Cambridge, MA United States)
Date Acquired
August 20, 2013
Publication Date
January 1, 2001
Publication Information
Publication: Lunar and Planetary Science XXXII
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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