Physicochemical properties of lunar regolith simulant for in situ oxygen production
Alyssa Ang De Guzman, Anish Mathai Varghese, Saif Alshalloudi, Lance Kosca, Kyriaki Polychronopoulou, Marko Gacesa

TL;DR
This study characterizes lunar regolith simulants to understand oxygen extraction potential, highlighting the importance of whole-regolith processing over solely ilmenite content for lunar in situ resource utilization.
Contribution
It provides a detailed validation and analysis of high-fidelity lunar regolith simulants, emphasizing their mineralogical fidelity and the factors influencing oxygen extraction.
Findings
Ilmenite is the most readily reducible oxygen-bearing phase.
Whole-regolith response influences oxygen extraction more than ilmenite content.
Surface and microstructural properties affect gas interactions.
Abstract
Permanent lunar settlements will rely on in situ oxygen production from regolith for life support and propulsion. While oxygen is abundant in lunar materials, it is chemically bound within metal oxides whose extractability depends strongly on regolith composition and processing strategy. In this study, we validate and characterize high-fidelity lunar regolith simulants representative of the lunar highlands and south pole using scanning electron microscopy with energy-dispersive X-ray spectroscopy, X-ray diffraction, Brunauer-Emmett-Teller surface area and pore structure analysis, and hydrogen temperature-programmed reduction. The simulants exhibit strong mineralogical and compositional fidelity to returned Apollo and Chang'e samples, with ilmenite confirmed as the most readily reducible oxygen-bearing phase. However, despite low ilmenite abundance, bulk highland simulants display…
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Taxonomy
TopicsPlanetary Science and Exploration · Astro and Planetary Science · Granular flow and fluidized beds
