Million-year solar wind irradiation recorded in chang’E-5 and chang’E-6 samples

The long-term effects of Earth's magnetosphere on solar wind (SW) irradiation asymmetry between the lunar nearside and farside, and their implications for space weathering processes, remain poorly characterized. Here, we measure exposure ages and SW-induced amorphous rim thicknesses of individual grains from the Chang'E-5 (CE-5) and Chang'E-6 (CE-6) lunar soils to derive rim growth rates. Comparative analysis of SW irradiation records from CE-5, CE-6, and Apollo (11, 16, 17) samples reveals that CE-6 grains from the southern mid-latitude farside exhibit higher rim growth rates than those from the low-latitude nearside Apollo sites. This trend aligns with simulated lunar surface SW fluxes and is consistent with the hypothesis that reduced SW exposure on the nearside, due to Earth's magnetospheric shielding, may contribute to a persistent hemispheric asymmetry in SW irradiation. However, CE-5 samples from the northern mid-latitude nearside yield unexpectedly high rim growth rates, suggesting the potential involvement of additional local factors. The exact reasons for this anomaly remain unclear and warrant further investigation.

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Publication Details

Journal
Nature Communications
Published
2025-10-16
DOI
https://doi.org/10.1038/s41467-025-64239-8
Citations
5
Primary Topic
Planetary Science and Exploration
Type
article
Field-Weighted Citation Impact
5.77

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article

Million-year solar wind irradiation recorded in chang’E-5 and chang’E-6 samples

Xiongyao Li, Chenkun Sun, Qiugang Zong, Zhiguo Meng et al.
5 citations
Nature Communications
Planetary Science and Exploration
5.77
article

Million-year solar wind irradiation recorded in chang’E-5 and chang’E-6 samples

Xiongyao Li, Chenkun Sun, Qiugang Zong, Zhiguo Meng, Xiaojia Zeng, Yi Xu, Sizhe Zhao, Renrui Liu, Chen Li, Yang Li, Xiaoping Zhang, Lianghai Xie, P. W. Luo, Ronghua Pang, Chi Wang
article en
5 citations

Abstract

The long-term effects of Earth's magnetosphere on solar wind (SW) irradiation asymmetry between the lunar nearside and farside, and their implications for space weathering processes, remain poorly characterized. Here, we measure exposure ages and SW-induced amorphous rim thicknesses of individual grains from the Chang'E-5 (CE-5) and Chang'E-6 (CE-6) lunar soils to derive rim growth rates. Comparative analysis of SW irradiation records from CE-5, CE-6, and Apollo (11, 16, 17) samples reveals that CE-6 grains from the southern mid-latitude farside exhibit higher rim growth rates than those from the low-latitude nearside Apollo sites. This trend aligns with simulated lunar surface SW fluxes and is consistent with the hypothesis that reduced SW exposure on the nearside, due to Earth's magnetospheric shielding, may contribute to a persistent hemispheric asymmetry in SW irradiation. However, CE-5 samples from the northern mid-latitude nearside yield unexpectedly high rim growth rates, suggesting the potential involvement of additional local factors. The exact reasons for this anomaly remain unclear and warrant further investigation.

Nature CommunicationsVol. 16(1)
Macau University of Science and Technology (MO), Yunnan University (CN), Jilin University (CN), Chinese Academy of Sciences (CN), China National Space Administration (CN), National Space Science Center (CN), Jilin Province Science and Technology Department (CN), Institute of Geochemistry (CN)
China National Space Administration, National Natural Science Foundation of China, Chinese Academy of Sciences, Fundo para o Desenvolvimento das Ciências e da Tecnologia, Suzhou Institute of Nanotechnology, Chinese Academy of Sciences, Institute of Geochemistry, Chinese Academy of Sciences
Openalex Percentile: Top 4%
Planetary Science and Exploration
5.77
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