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Molten Regolith Electrolysis Performed in Vacuum Testing at Kennedy Space Center: Analysis of the Retrieved Core SampleThe NASA Space Technology Mission Directorate (STMD) Game Changing Development (GCD) program funded a collaboration with NASA and industry to demonstrate the Molten Regolith Electrolysis (MRE) process in a vacuum
environment. MRE has been a long time studied technology for oxygen (O2) production from regolith on the lunar surface[1] [2]. MRE remains a promising technology for O2 production for human life support and propellant supply, as well as for construction materials that are retrieved from the molten metal slag. The MRE demonstration occurred in December 2024 at Kennedy Space Center (KSC) with Lunar Resources, Inc. (LUNAR), using ICN-LHT-1G (also known as CSM-LHT-1G) regolith [3]. LUNAR was funded via an SBIR Phase
III contract (Contract #80NSSC22C0001). A LUNAR manufactured reactor was tested in the KSC Atmospherically Sealed Simulator for In-situ System Testing (ASSIST) chamber. The O2 and its gaseous byproducts were analyzed during the regolith electrolysis using the NASA developed Volatile Monitoring and Oxygen Measurement System (VMOMS). VMOMS included a residual gas analyzer, oxygen sensors, and a gas chromatograph. A core sample was retrieved after the molten regolith cooled down post electrolysis. A computed tomography (CT) scan was performed on the retrieved core sample. X-ray photo-electron spectroscopy (XPS), scanning electron microscopy (SEM), energy dispersive spectrometer (EDS), and X-ray fluorescence (XRF) measurements were all collected to provide insights on composition and morphology of the sample. This work describes some of the results of the retrieved core analysis as well as discussions on future work that the KSC MRE team will be performing on a fully integrated MRE system, to further develop the technology.
Document ID
20250003220
Acquisition Source
Kennedy Space Center
Document Type
Extended Abstract
Authors
A J Meier ORCID
(Kennedy Space Center Merritt Island, Florida, United States)
J Olson
(Kennedy Space Center Merritt Island, Florida, United States)
D Essumang
(Kennedy Space Center Merritt Island, Florida, United States)
E Bell
(Kennedy Space Center Merritt Island, Florida, United States)
J Toro
(Kennedy Space Center Merritt Island, Florida, United States)
J Smith
(Kennedy Space Center Merritt Island, Florida, United States)
T Johnson
(Kennedy Space Center Merritt Island, Florida, United States)
M M Tessema
(Kennedy Space Center Merritt Island, Florida, United States)
R Ebrahim
(Lunar Resources, Inc.)
M Hinkel
(Lunar Resources, Inc.)
A Ignatiev
(Lunar Resources, Inc.)
Date Acquired
March 31, 2025
Subject Category
Engineering (General)
Meeting Information
Meeting: Lunar Surface Innovation Consortium (LSIC) Spring Meeting
Location: Laurel, MD
Country: US
Start Date: May 20, 2025
End Date: May 22, 2025
Sponsors: Johns Hopkins University Applied Physics Lab
Funding Number(s)
WBS: 596118.04.39.76
Distribution Limits
Public
Copyright
Use by or on behalf of the US Gov. Permitted.
Technical Review
NASA Peer Committee
Keywords
Molten regolith electrolysis
ISRU
regolith characterization
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