NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Composition and Color of Martian Soil from Oxidation of Meteoritic MaterialAqueous weathering is not necessary for formation of the martian soils. The chemical composition and oxidation state of the surface fines can be attributed to meteoritic influx. Additional information is contained in the original extended abstract.
Document ID
20010045309
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
Authors
Yen, A. S.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA 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.

Available Downloads

There are no available downloads for this record.
No Preview Available