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Hydrogen Plasma ReductionHydrogen plasma increases efficiency by strategically using energy to break bonds within the regolith to liberate oxygen instead of heating the entire bed of regolith. The energy used by the plasma system would be imparted into the H2 gas, forming highly energetic ions, electrons, and neutrals that would interact with the regolith surface. The energized atomic and ionic H2 provide the energy needed to make reduction of SiO2 (Silicon Dioxide) and other regolith mineral oxides favorable. What’s more, the high-energy plasma interaction occurs in a small, localized volume, and thus requires relatively little energy. The lunar regolith is well-suited for the process as the fine particles naturally available provide a high surface area for the plasma to interact with. The process would require a system to collect the regolith composed of metal oxides (MxOy) and load it into a reactor. An H2 plasma would pass over the surface (potentially at a low pressure, reducing complexity of the system as it would not require large increases in pressure from the lunar vacuum), then the gases from the plasma reaction would be collected and processed, and the spent regolith would be carried away. The gross reaction temperature would be near ambient (due to the localized nature of the plasma), eliminating the necessity of a regolith heating mechanism or handling of molten regolith. Also, the H2 used in the plasma could be subsequently recovered from the water produced by the plasma reaction. Thus, this approach would not require significant amounts of added commodities.
Document ID
20210024442
Acquisition Source
Kennedy Space Center
Document Type
Contractor or Grantee Report
Authors
Elspeth Petersen
(Kennedy Space Center Merritt Island, Florida, United States)
Kenneth Engeling
(Kennedy Space Center Merritt Island, Florida, United States)
Ryan Gott
(Universities Space Research Association Columbia, Maryland, United States)
Joel Olson
(Southeastern Universities Research Association Washington D.C., District of Columbia, United States)
Carolina Franco
(Aecom (United States) Los Angeles, California, United States)
Nilab Azim
(Kennedy Space Center Merritt Island, Florida, United States)
Date Acquired
November 16, 2021
Publication Date
December 16, 2021
Subject Category
Plasma Physics
Lunar And Planetary Science And Exploration
Funding Number(s)
WBS: 295670
CONTRACT_GRANT: KSC-UB-Generic
CONTRACT_GRANT: 80KSC017C0012
Distribution Limits
Public
Copyright
Public Use Permitted.
Technical Review
NASA Technical Management
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