Magnetic vortex state of natural lunar γ-Fe

On the lunar surface α-Fe and Fe-Ni alloys are widespread and the dominant carriers of the lunar remanent magnetization. Metallic γ-Fe, however, is stable only at high temperatures and has not been documented in lunar samples. Here we report the identification of ambient stable γ-Fe preserved as nanometer-scale particles in Chang’e-6 impact glass fragments from the South Pole-Aitken Basin. Electron holography analyses reveal that these γ-Fe particles have a magnetic vortex domain state. Based on these results, we propose that the formation and preservation of γ-Fe at lunar surface temperature requires incorporation of trace γ-phase-stabilizing elements together with extremely rapid quenching during lunar impact processes. Our findings provide a basis for understanding the lunar core dynamo evolution and impact-induced magnetic recording mechanisms.

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Publication Details

Journal
Proceedings of the National Academy of Sciences
Published
2026-09-16
DOI
https://doi.org/10.1073/pnas.2608395123
Primary Topic
Planetary Science and Exploration
Type
article
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article

Magnetic vortex state of natural lunar γ-Fe

Dongsheng Song, Haifeng Du, Ann M. Hirt, Zheng Gong et al.
Proceedings of the National Academy of Sciences
Planetary Science and Exploration
article

Magnetic vortex state of natural lunar γ-Fe

Dongsheng Song, Haifeng Du, Ann M. Hirt, Zheng Gong, Wyn Williams, Kelei Zhu, Ziliang Jin, Jinhua Li, Pengfei Liu, Jing Liu, Keke Zhang, Xiandi Zeng, Kang Wang, Chuanxin Yan, Long Li
article en

Abstract

On the lunar surface α-Fe and Fe-Ni alloys are widespread and the dominant carriers of the lunar remanent magnetization. Metallic γ-Fe, however, is stable only at high temperatures and has not been documented in lunar samples. Here we report the identification of ambient stable γ-Fe preserved as nanometer-scale particles in Chang’e-6 impact glass fragments from the South Pole-Aitken Basin. Electron holography analyses reveal that these γ-Fe particles have a magnetic vortex domain state. Based on these results, we propose that the formation and preservation of γ-Fe at lunar surface temperature requires incorporation of trace γ-phase-stabilizing elements together with extremely rapid quenching during lunar impact processes. Our findings provide a basis for understanding the lunar core dynamo evolution and impact-induced magnetic recording mechanisms.

Proceedings of the National Academy of SciencesVol. 123(38)
Macau University of Science and Technology (MO), Planetary Science Institute (US), Anhui University (CN), Hefei Institutes of Physical Science (CN), Institute of Geology and Geophysics (AZ), Institute of Geophysics (RU), Institute of Geology and Geophysics (CN), University of Chinese Academy of Sciences (CN), Nanjing University (CN), University of Edinburgh (GB)
Openalex Percentile: Top 10%
Planetary Science and Exploration
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