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Experimental reduction of lunar mare soil and volcanic glassWe have reduced high-titanium lunar mare soil and iron-rich lunar volcanic glass with hydrogen at temperatures of 900-1100 C. Ilmenite is the most reactive phase in the soil, exhibiting rapid and complete reduction at all temperatures. Ferrous iron in the glass is extensively reduced concurrent with partial crystallization. In both samples pyroxene and olivine undergo partial reduction along with chemical and mineralogical modifications. High-temperature reduction provides insight into the optical and chemical effects of lunar soil maturation, and places constraints on models of that process. Mare soil and volcanic glass are attractive feedstocks for lunar oxygen production, with achievable yields of 2-5 wt%.
Document ID
19950035561
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Allen, Carlton C.
(Lockheed Engineering and Sciences Company, Houston, TX United States)
Morris, Richard V.
(NASA Johnson Space Center Houston, TX, United States)
Mckay, David S.
(NASA Johnson Space Center Houston, TX, United States)
Date Acquired
August 16, 2013
Publication Date
November 25, 1994
Publication Information
Publication: Journal of Geophysical Research
Volume: 99
Issue: E11
ISSN: 0148-0227
Subject Category
Lunar And Planetary Exploration
Accession Number
95A67160
Distribution Limits
Public
Copyright
Other

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