Abstract
High-Ti deposits on the Moon may emerge as a key resource for oxygen extraction. Descriptive models are the first qualitative step toward quantitative assessments of natural resources. Such models provide a structured framework for understanding the formation processes and spatial distribution of discrete types of resource deposits. In this study, we provide the first lunar descriptive models, characterizing high-Ti lunar deposits, drawing parallels with established models used in assessing mineral deposits on Earth.Our methodology involves utilizing remote sensing datasets and geological maps to identify and describe high-Ti deposits. This is supplemented by data extrapolated from Apollo missions. However, there remain critical knowledge gaps, particularly regarding petrography, subsurface information, surface characteristics, and physical properties of high-Ti deposits, which necessitate further exploration and analysis.
Published Version
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