Submicroscopic magnetite may be ubiquitous in the lunar regolith of the high-Ti region

Magnetite is rare on the Moon. The ubiquitous presence of magnetite in lunar soil has been hypothesized in previous Apollo Mössbauer spectroscopy and electron spin resonance studies, but there is currently no mineralogical evidence to prove it. Here, we report a large number of submicroscopic magnetite particles embedded within iron-sulfide on the surface of Chang'e-5 glass, with a close positive correlation between magnetite content and the TiO<sub>2</sub> content of the surrounding glass. The morphology and mineralogy of the iron-sulfide grains suggest that these magnetite particles formed via an impact process between iron-sulfide droplets and silicate glass melt, and ilmenite is necessary for magnetite formation. Magnetite in lunar glass is a potential candidate for the "magnetite-like" phase detected in the Apollo era and suggests that impact-induced submicroscopic magnetite may be ubiquitous in high-Ti regions of the Moon. Moreover, these impact-induced magnetite particles may be crucial for understanding the lunar magnetic anomalies and mineral components of the deep Moon.

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Publication Details

Journal
Science Advances
Published
2024-09-20
DOI
https://doi.org/10.1126/sciadv.adn2301
Citations
16
Primary Topic
Planetary Science and Exploration
Type
article
Field-Weighted Citation Impact
5.30

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article

Submicroscopic magnetite may be ubiquitous in the lunar regolith of the high-Ti region

Xiongyao Li, Long Xiao, Yuanyun Wen, Zhuang Guo et al.
16 citations
Science Advances
Planetary Science and Exploration
5.30
article

Submicroscopic magnetite may be ubiquitous in the lunar regolith of the high-Ti region

Xiongyao Li, Long Xiao, Yuanyun Wen, Zhuang Guo, Sizhe Zhao, Chen Li, Yang Li, Zhiyong Xiao, Jianzhong Liu, Lifang Li, Junhu Wang, Zhi Cao, Qi He
article en
16 citations

Abstract

Magnetite is rare on the Moon. The ubiquitous presence of magnetite in lunar soil has been hypothesized in previous Apollo Mössbauer spectroscopy and electron spin resonance studies, but there is currently no mineralogical evidence to prove it. Here, we report a large number of submicroscopic magnetite particles embedded within iron-sulfide on the surface of Chang'e-5 glass, with a close positive correlation between magnetite content and the TiO<sub>2</sub> content of the surrounding glass. The morphology and mineralogy of the iron-sulfide grains suggest that these magnetite particles formed via an impact process between iron-sulfide droplets and silicate glass melt, and ilmenite is necessary for magnetite formation. Magnetite in lunar glass is a potential candidate for the "magnetite-like" phase detected in the Apollo era and suggests that impact-induced submicroscopic magnetite may be ubiquitous in high-Ti regions of the Moon. Moreover, these impact-induced magnetite particles may be crucial for understanding the lunar magnetic anomalies and mineral components of the deep Moon.

Science AdvancesVol. 10(38)
Macau University of Science and Technology (MO), Sun Yat-sen University (CN), Dalian Institute of Chemical Physics (CN), Harbin Institute of Technology (CN), Hefei Institutes of Physical Science (CN), China University of Geosciences (CN), Northwest University (CN), Institute of Geochemistry (CN), University of Hong Kong (HK)
Chinese Academy of Sciences, China Postdoctoral Science Foundation, Youth Innovation Promotion Association of the Chinese Academy of Sciences, Youth Innovation Promotion Association, Institute of Geochemistry, Chinese Academy of Sciences
Life in Land
Openalex Percentile: Top 4%
Planetary Science and Exploration
5.30
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