Mare soil and orange and black pyroclastic glass were reduced in hydrogen gas at temperatures of 900 to 1100 C. The experiments support studies of regolith maturation, lunar volcanism, and the production of oxygen on the moon. The most reactive component in the high-Ti soil was FeO in ilmenite, which was completely reduced to iron metal at all temperatures. Vitreous orange glass crystallized and was partially reduced to iron metal, pyroxene, and minor olivine. Initially devitrified black glass was similarly reduced and converted to iron metal, pyroxene, and minor olivine. The degree of reaction in both glasses increased with temperature
In the past 20 years, considerable attention been paid to returning to our natural satellite with ro...
A suite of lightning strike glasses and unmelted starting materials has been studied by electron mic...
The mineralogy and petrology of the Apollo 11 rocks are consistent with impact melting of ilmenite ...
The first set of hydrogen reduction experiments to use actual lunar material was recently completed....
The most abundant element in lunar rocks and soils is oxygen which makes up approximately 45 percent...
The Carbotek/Shimizu process to produce oxygen from lunar soils has been successfully demonstrated o...
Future human habitation of the Moon will likely require the use of locally derived materials because...
The kinetics and mechanism of the reduction of simulants of the iron-bearing lunar minerals olivine ...
Future human habitation of the Moon will likely require the use of locally derived materials because...
Hawke et al. (1990) suggest that ilmenite found in Apollo 17-type pyroclastic glass may provide feed...
The chemical composition of a volcanic ash deposited near Flagstaff, Arizona, USA closely resembles ...
Various high temperature chemical processes have been developed to extract oxygen and metals from lu...
The goal is to fabricate useful ceramic materials from the by-products of lunar oxygen production pr...
In the past 20 years, considerable attention been paid to returning to our natural satellite with r...
The research described in this progress report involved the study of petrological, geochemical and v...
In the past 20 years, considerable attention been paid to returning to our natural satellite with ro...
A suite of lightning strike glasses and unmelted starting materials has been studied by electron mic...
The mineralogy and petrology of the Apollo 11 rocks are consistent with impact melting of ilmenite ...
The first set of hydrogen reduction experiments to use actual lunar material was recently completed....
The most abundant element in lunar rocks and soils is oxygen which makes up approximately 45 percent...
The Carbotek/Shimizu process to produce oxygen from lunar soils has been successfully demonstrated o...
Future human habitation of the Moon will likely require the use of locally derived materials because...
The kinetics and mechanism of the reduction of simulants of the iron-bearing lunar minerals olivine ...
Future human habitation of the Moon will likely require the use of locally derived materials because...
Hawke et al. (1990) suggest that ilmenite found in Apollo 17-type pyroclastic glass may provide feed...
The chemical composition of a volcanic ash deposited near Flagstaff, Arizona, USA closely resembles ...
Various high temperature chemical processes have been developed to extract oxygen and metals from lu...
The goal is to fabricate useful ceramic materials from the by-products of lunar oxygen production pr...
In the past 20 years, considerable attention been paid to returning to our natural satellite with r...
The research described in this progress report involved the study of petrological, geochemical and v...
In the past 20 years, considerable attention been paid to returning to our natural satellite with ro...
A suite of lightning strike glasses and unmelted starting materials has been studied by electron mic...
The mineralogy and petrology of the Apollo 11 rocks are consistent with impact melting of ilmenite ...