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Mars Redox Chemistry: Atacama Desert Soils as a Terrestrial AnalogThe motivation for this work is to perform quantitative site characterizations of soil chemical processes to allow further development and field validation of the Mars Oxidant Instrument (MOI). The MOI is an in situ survey instrument designed to establish the presence of reactive chemical species in the martian soil, dust, or atmosphere, and to provide detailed reaction model system measurements to enable comprehensive Earthbased study. Functioning as a survey instrument, MOI tests the broad range of hypotheses explaining the reactivity of the martian surface material that have been put forth since the Viking experiments. This work is currently being carried out under the NASA ASTEP funded AstroBioLab (Jeffery Bada, PI). A second objective is to use Atacama field and Viking data to perform comparative studies, with the goal of furthering the understanding of the formation mechanisms and properties of martian oxidants.
Document ID
20030111359
Document Type
Conference Paper
Authors
Quinn, R. C. (Search for Extraterrestrial Intelligence Inst. Moffett Field, CA, United States)
Grunthaner, F. J. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Taylor, C. L. (Search for Extraterrestrial Intelligence Inst. Moffett Field, CA, United States)
Zent, A. P. (NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
August 21, 2013
Publication Date
January 1, 2003
Publication Information
Publication: Lunar and Planetary Science XXXIV
Subject Category
Geosciences (General)
Distribution Limits
Public
Copyright
Public Use Permitted.

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IDRelationTitle20030110578Analytic PrimaryLunar and Planetary Science XXXIV
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