Impact-Driven Cr-Fe-O Vaporization and Deposition on the Moon

1,2Xiaojia Zeng, 3Chenkun Sun, 2Mingchao Xiong, 1,2Xiongyao Li
Journal of Geophysical Research: Planets, 131, e2026JE009807 Link to Article [DOI: 10.1029/2026JE009807]
1State Key Laboratory of Critical Mineral Research and Exploration, Institute of Geochemistry, Chinese Academy of Sciences, Guiyang, China
2Center for Lunar and Planetary Sciences, Institute of Geochemistry, Chinese Academy of Sciences, Guiyang, China
3State Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, Macau, China
Published by arrangement with John Wiley & Sons

Hypervelocity impacts from micrometeorites or asteroids are a dominant long‐term geologicalprocess that modifies the mineralogical and elemental components of surface regolith on the Moon and otherairless planetary bodies. However, the pathways by which impacts drive elemental redistribution on the Moonremain poorly understood. Here, we report the discovery of thousands of chromite (FeCr2O4) nanoparticlesdeposited on a space‐weathered olivine fragment from Chang’e

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