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Chemical Alteration on Mars Indicated by the Iron-Manganese RatioThe Alpha Particle X-ray Spectrometers (APXS) onboard the Mars Exploration Rovers (MER) have measured the chemical compositions of over 400 samples on the surface of Mars. Fe and Mn are among the elements which are well established by this instrumentation. Fe2+ and Mn2+ have nearly the same ionic radii and distribute similarly in primary igneous rocks, maintaining a consistent Fe:Mn ratio. Upon exposure to an oxidative weathering environment, Fe 3+ and Mn4+ are commonly formed, and elemental fractionation can occur. Thus, altered samples will typically exhibit a Fe:Mn ratio different from precursor materials.
Document ID
20100005043
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Yen, A. S.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Clark, B. C.
(Space Science Inst. Boulder, CO, United States)
Ming, D. W.
(NASA Johnson Space Center Houston, TX, United States)
Mittlefehldt, D. W.
(NASA Johnson Space Center Houston, TX, United States)
Gellert, R.
(Guelph Univ. Ontario, Canada)
Morris, R. V.
(NASA Johnson Space Center Houston, TX, United States)
Date Acquired
August 25, 2013
Publication Date
January 1, 2010
Subject Category
Space Sciences (General)
Report/Patent Number
JSC-CN-19548
Report Number: JSC-CN-19548
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: The Woodlands, TX
Country: United States
Start Date: March 1, 2010
End Date: March 5, 2010
Sponsors: Lunar and Planetary Inst., NASA Headquarters
Distribution Limits
Public
Copyright
Public Use Permitted.
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