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Magnetic signatures and origins of ferromagnetic minerals in Chang’e-6 lunar farside soils

Author

Listed:
  • Jinhua Li

    (Chinese Academy of Sciences
    University of Chinese Academy of Sciences)

  • Lin Xing

    (Chinese Academy of Sciences
    University of Chinese Academy of Sciences)

  • Zheng Gong

    (Nanjing University)

  • Jiawei Liu

    (University of Chinese Academy of Sciences
    Chinese Academy of Sciences)

  • Yan Liu

    (Chinese Academy of Sciences
    University of Chinese Academy of Sciences)

  • Weiwei Wu

    (Chinese Academy of Sciences
    University of Chinese Academy of Sciences)

  • Kelei Zhu

    (Chinese Academy of Sciences
    University of Chinese Academy of Sciences)

  • Yuqin Wang

    (Chinese Academy of Sciences
    University of Chinese Academy of Sciences)

  • Xu Tang

    (Chinese Academy of Sciences
    University of Chinese Academy of Sciences)

  • Lixin Gu

    (Chinese Academy of Sciences
    University of Chinese Academy of Sciences)

  • Yi Chen

    (University of Chinese Academy of Sciences
    Chinese Academy of Sciences)

  • Qiuli Li

    (University of Chinese Academy of Sciences
    Chinese Academy of Sciences)

  • Zhaoyang Cao

    (Chinese Academy of Sciences
    University of Chinese Academy of Sciences)

  • Shuangchi Liu

    (University of Chinese Academy of Sciences
    Chinese Academy of Sciences)

  • Shuhui Cai

    (University of Chinese Academy of Sciences
    Chinese Academy of Sciences)

  • Yongxin Pan

    (University of Chinese Academy of Sciences
    Chinese Academy of Sciences)

Abstract

Ferromagnetic minerals in lunar materials record key information regarding the Moon’s ancient dynamo, impact events, and space weathering. However, interpreting the magnetic signals is complicated by their diverse origins and properties. Here, we present comprehensive magnetic and mineralogical results of farside lunar soils returned by Chang’e-6 mission from the South Pole-Aitken Basin. Compared to nearside samples, these soils exhibit higher magnetic susceptibility and saturation magnetization, and the highest saturation remanence, despite weak local crustal magnetic anomalies. Advanced electron microscopy reveals two primary mineralogical populations: nickel-poor iron particles with euhedral shapes in basalt clasts (magmatic origin) and nickel-rich metallic iron and Fe-Ni alloys in breccias, agglutinates, and glassy materials (impact origin). These findings offer insights into the formation of magnetic minerals on the lunar farside, thereby enhancing our understanding of lunar dynamo evolution and crustal magnetic anomalies.

Suggested Citation

  • Jinhua Li & Lin Xing & Zheng Gong & Jiawei Liu & Yan Liu & Weiwei Wu & Kelei Zhu & Yuqin Wang & Xu Tang & Lixin Gu & Yi Chen & Qiuli Li & Zhaoyang Cao & Shuangchi Liu & Shuhui Cai & Yongxin Pan, 2025. "Magnetic signatures and origins of ferromagnetic minerals in Chang’e-6 lunar farside soils," Nature Communications, Nature, vol. 16(1), pages 1-9, December.
  • Handle: RePEc:nat:natcom:v:16:y:2025:i:1:d:10.1038_s41467-025-61705-1
    DOI: 10.1038/s41467-025-61705-1
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    References listed on IDEAS

    as
    1. Huijuan Zhang & Wei Yang & Di Zhang & Hengci Tian & Renhao Ruan & Sen Hu & Yi Chen & Hejiu Hui & Yanhao Lin & Ross N. Mitchell & Di Zhang & Shitou Wu & Lihui Jia & Lixin Gu & Yangting Lin & XianHua Li, 2024. "Long-term reduced lunar mantle revealed by Chang’e-5 basalt," Nature Communications, Nature, vol. 15(1), pages 1-9, December.
    2. David A. Kring & Danielle P. Kallenborn & Gareth S. Collins, 2025. "Grand canyons on the Moon," Nature Communications, Nature, vol. 16(1), pages 1-7, December.
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