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Lunar and Planetary Science XXXV: Weird Martian Minerals: Complex Mars Surface ProcessesThe session "Complex Mars Surface" included the following reports:A Reappraisal of Adsorbed Superoxide Ion as the Cause Behind the Reactivity of the Martian Soils; Sub-Surface Deposits of Hydrous Silicates or Hydrated Magnesium Sulfates as Hydrogen Reservoirs near the Martian Equator: Plausible or Not?; Thermal and Evolved Gas Analysis of Smectites: The Search for Water on Mars; Aqueous Alteration Pathways for K, Th, and U on Mars; Temperature Dependence of the Moessbauer Fraction in Mars-Analog Minerals; Acid-Sulfate Vapor Reactions with Basaltic Tephra: An Analog for Martian Surface Processes; Iron Oxide Weathering in Sulfuric Acid: Implications for Mars; P/Fe as an Aquamarker for Mars; Stable Isotope Composition of Carbonates Formed in Low-Temperature Terrestrial Environments as Martian Analogs; Can the Phosphate Sorption and Occlusion Properties Help to Elucidate the Genesis of Specular Hematite on the Mars Surface?; Sulfate Salts, Regolith Interactions, and Water Storage in Equatorial Martian Regolith; Potential Pathways to Maghemite in Mars Soils: The Key Role of Phosphate; and Mineralogy, Abundance, and Hydration State of Sulfates and Chlorides at the Mars Pathfinder Landing Site.
Document ID
20040062536
Acquisition Source
Johnson Space Center
Document Type
Conference Proceedings
Date Acquired
August 21, 2013
Publication Date
January 1, 2004
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
LPI-Contrib-1197
Meeting Information
Meeting: Lunar and Planetary Science XXXV
Location: Houston, TX
Country: United States
Start Date: March 15, 2004
End Date: March 19, 2004
Sponsors: Lunar and Planetary Inst., NASA Johnson Space Center
Funding Number(s)
CONTRACT_GRANT: NCC5-679
Distribution Limits
Public
Copyright
Public Use Permitted.

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