Discovery of crystalline Fe <sub>2</sub> O <sub>3</sub> in returned lunar soils

Lunar materials were believed to have formed and been preserved in a reducing environment, with only Fe<sup>2+</sup> and Fe<sup>0</sup> present. Native oxidized minerals, such as hematite, have not been validated in previously returned lunar samples. In this work, we report the discovery of micrometer-scale crystalline Fe<sub>2</sub>O<sub>3</sub> in the forms of hematite (α-Fe<sub>2</sub>O<sub>3</sub>) and maghemite (γ-Fe<sub>2</sub>O<sub>3</sub>) overgrowing troilite in the recently returned Chang'e-6 (CE6) lunar soils. It is possible that impact-induced oxygen release created localized micrometer-scale regions of elevated oxygen fugacity, facilitating the formation of Fe<sub>2</sub>O<sub>3</sub> at temperatures between ~700° and 1000°C. This finding provides credible evidence for the presence of Fe<sub>2</sub>O<sub>3</sub> on the lunar surface, challenging the traditional understanding of lunar surface redox states. In addition, the Fe<sub>2</sub>O<sub>3</sub> in the form of maghemite may be the mineralogical reason for the generation of the magnetic anomalies observed around the South Pole-Aitken basin.

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Publication Details

Journal
Science Advances
Published
2025-11-14
DOI
https://doi.org/10.1126/sciadv.ady5169
Citations
3
Primary Topic
Planetary Science and Exploration
Type
article
Field-Weighted Citation Impact
3.46

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article

Discovery of crystalline Fe 2 O 3 in returned lunar soils

X. Lu, Y.G. Liu, Xiaohui Fu, Le Qiao et al.
3 citations
Science Advances
Planetary Science and Exploration
3.46
article

Discovery of crystalline Fe 2 O 3 in returned lunar soils

X. Lu, Y.G. Liu, Xiaohui Fu, Le Qiao, Zongcheng Ling, Xiaojia Zeng, Rui Li, Haijun Cao, Chen Li, Jian Chen, Yang Li, Jianzhong Liu, Changqing Liu, Ziyi Jia, Yanqing Xin, Ying‐Bo Lu, Can Bin Yin
article en
3 citations

Abstract

Lunar materials were believed to have formed and been preserved in a reducing environment, with only Fe<sup>2+</sup> and Fe<sup>0</sup> present. Native oxidized minerals, such as hematite, have not been validated in previously returned lunar samples. In this work, we report the discovery of micrometer-scale crystalline Fe<sub>2</sub>O<sub>3</sub> in the forms of hematite (α-Fe<sub>2</sub>O<sub>3</sub>) and maghemite (γ-Fe<sub>2</sub>O<sub>3</sub>) overgrowing troilite in the recently returned Chang'e-6 (CE6) lunar soils. It is possible that impact-induced oxygen release created localized micrometer-scale regions of elevated oxygen fugacity, facilitating the formation of Fe<sub>2</sub>O<sub>3</sub> at temperatures between ~700° and 1000°C. This finding provides credible evidence for the presence of Fe<sub>2</sub>O<sub>3</sub> on the lunar surface, challenging the traditional understanding of lunar surface redox states. In addition, the Fe<sub>2</sub>O<sub>3</sub> in the form of maghemite may be the mineralogical reason for the generation of the magnetic anomalies observed around the South Pole-Aitken basin.

Science AdvancesVol. 11(46)
Yunnan University (CN), Chinese Academy of Sciences (CN), Institute of Space Sciences (ES), Institute of Geochemistry (CN)
National Key Research and Development Program of China
Openalex Percentile: Top 7%
Planetary Science and Exploration
3.46
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