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Chang’E-5 samples reveal high water content in lunar minerals

Author

Listed:
  • Chuanjiao Zhou

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

  • Hong Tang

    (Chinese Academy of Sciences
    CAS Center for Excellence in Comparative Planetology
    Chinese Academy of Sciences)

  • Xiongyao Li

    (Chinese Academy of Sciences
    CAS Center for Excellence in Comparative Planetology
    Chinese Academy of Sciences)

  • Xiaojia Zeng

    (Chinese Academy of Sciences
    Chinese Academy of Sciences)

  • Bing Mo

    (Chinese Academy of Sciences
    CAS Center for Excellence in Comparative Planetology
    Chinese Academy of Sciences)

  • Wen Yu

    (Chinese Academy of Sciences
    CAS Center for Excellence in Comparative Planetology
    Chinese Academy of Sciences)

  • Yanxue Wu

    (Guangdong University of Technology)

  • Xiandi Zeng

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

  • Jianzhong Liu

    (Chinese Academy of Sciences
    CAS Center for Excellence in Comparative Planetology
    Chinese Academy of Sciences)

  • Yuanyun Wen

    (Chinese Academy of Sciences)

Abstract

The formation and distribution of lunar surficial water remains ambiguous. Here, we show the prominence of water (OH/H2O) attributed to solar wind implantation on the uppermost surface of olivine, plagioclase, and pyroxene grains from Chang’E-5 samples. The results of spectral and microstructural analyses indicate that solar wind-derived water is affected by exposure time, crystal structure, and mineral composition. Our estimate of a minimum of 170 ppm water content in lunar soils in the Chang’E-5 region is consistent with that reported by the Moon Minerology Mapper and Chang’E-5 lander. By comparing with remote sensing data and through lunar soil maturity analysis, the amount of water in Chang’E-5 provides a reference for the distribution of surficial water in middle latitude of the Moon. We conclude that minerals in lunar soils are important reservoirs of water, and formation and retention of water originating from solar wind occurs on airless bodies.

Suggested Citation

  • Chuanjiao Zhou & Hong Tang & Xiongyao Li & Xiaojia Zeng & Bing Mo & Wen Yu & Yanxue Wu & Xiandi Zeng & Jianzhong Liu & Yuanyun Wen, 2022. "Chang’E-5 samples reveal high water content in lunar minerals," Nature Communications, Nature, vol. 13(1), pages 1-10, December.
  • Handle: RePEc:nat:natcom:v:13:y:2022:i:1:d:10.1038_s41467-022-33095-1
    DOI: 10.1038/s41467-022-33095-1
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    References listed on IDEAS

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    1. Sen Hu & Huicun He & Jianglong Ji & Yangting Lin & Hejiu Hui & Mahesh Anand & Romain Tartèse & Yihong Yan & Jialong Hao & Ruiying Li & Lixin Gu & Qian Guo & Huaiyu He & Ziyuan Ouyang, 2021. "A dry lunar mantle reservoir for young mare basalts of Chang’e-5," Nature, Nature, vol. 600(7887), pages 49-53, December.
    2. Qiu-Li Li & Qin Zhou & Yu Liu & Zhiyong Xiao & Yangting Lin & Jin-Hua Li & Hong-Xia Ma & Guo-Qiang Tang & Shun Guo & Xu Tang & Jiang-Yan Yuan & Jiao Li & Fu-Yuan Wu & Ziyuan Ouyang & Chunlai Li & Xian, 2021. "Two-billion-year-old volcanism on the Moon from Chang’e-5 basalts," Nature, Nature, vol. 600(7887), pages 54-58, December.
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