Hydrogen Plasma Reduction of Silicates for Lunar Oxygen Liberation
ORAL
Abstract
As crewed missions to the moon become closer, the focus on in-situ resource utilization efforts has increased. Since lunar soil has abundant oxygen on the surface of the moon, work has been done to process this resource in an efficient manner. Hydrogen reduction of lunar regolith has emerged as a method of liberating oxygen that can be used for fuel and water production. Traditional reduction techniques require high temperatures and increased complexity when dealing with high amounts of silicates. Plasma can reduce silicates efficiently and thus has become of high interest for use in the lunar highlands where silicates exist in high quantities. NASA’s Kennedy Space Center is exploring the use of low temperature plasmas for the reduction of silicates. This work shows that exposing silicates to a hydrogen plasma produces water. Residual gas analysis and optical emission spectroscopy were used to measure the relative quantities of water vapor production and OH (A-X) emission for hydrogen plasma interactions with lunar highland simulant and silica. X-ray photo-electron spectroscopy and scanning electron microscopy/energy-dispersive X-ray spectroscopy were also used to observe surface modifications to the silicates that reflect the key chemical reactions that occurred. From this data, plasma has emerged as a promising solution to produce oxygen on the lunar surface.
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Presenters
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Ryan Gott
University Space Research Association, NASA Kennedy
Authors
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Ryan Gott
University Space Research Association, NASA Kennedy
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Kenneth Engeling
NASA's Kennedy Space Center
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Nilab Azim
NASA's Kennedy Space Center
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Elspeth Petersen
NASA's Kennedy Space Center
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Joel Olson
Southeastern Universities Research Association
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Carolina Franco
AECOM Management Services Inc.