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The Martian Soil as a Geochemical Sink for Hydrothermally Altered Crustal Rocks and Mobile Elements: Implications of Early MER ResultsHydrothermal and aqueous alteration can explain some of the exciting results from the MER team s analyses of the martian soil, including the major elements, mobile elements, and the nickel enrichment. Published results from the five lander missions lead to the following conclusions: 1) The soil appears to be globally mixed and basaltic with only small local variations in chemistry. Relative to martian basaltic meteorites and Gusev rocks the soils are depleted in the fluid-mobile element calcium, but only slightly enriched to somewhat depleted in iron oxide. 2) The presence of olivine in the soils based on M ssbauer data argues that the soil is only partly weathered and is more akin to a lunar regolith than a terrestrial soil. 3) The presence of bromine along with sulfur and chlorine in the soils is consistent with addition of a mobile element component to the soil.
Document ID
Acquisition Source
Document Type
Conference Paper
Newsom, H. E.
(New Mexico Univ. Albuquerque, NM, United States)
Nelson, M. J.
(New Mexico Univ. Albuquerque, NM, United States)
Shearer, C. K.
(New Mexico Univ. Albuquerque, NM, United States)
Draper, D. S.
(New Mexico Univ. Albuquerque, NM, United States)
Date Acquired
September 7, 2013
Publication Date
January 1, 2005
Publication Information
Publication: Lunar and Planetary Science XXXVI, Part 14
Subject Category
Lunar And Planetary Science And Exploration
Funding Number(s)
Distribution Limits
Public Use Permitted.
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