Weak influence of the secondary surface processes on the regolith of Chang’E-5 landing site
Weak influence of the secondary surface processes on the regolith of Chang’E-5 landing site
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DOI:
10.1038/s43247-023-00937-9
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发表时间:
2023-08
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通讯作者:
Junjie Li;Ziying Li;Zhixin Huang;Ting Li;Dongfa Guo;Hanbin Liu;Guang Fan;M. Qin;Liang Lei;Xin Zhou;Hailong Wang;Kaiyu Wang;Xiang Gao;Apeng Yu;Ruiping Liu;Jia Zhang;Liumin Deng;Sheng He;Yong Wu;Lin‐Fei Qiu
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作者:
Junjie Li;Ziying Li;Zhixin Huang;Ting Li;Dongfa Guo;Hanbin Liu;Guang Fan;M. Qin;Liang Lei;Xin Zhou;Hailong Wang;Kaiyu Wang;Xiang Gao;Apeng Yu;Ruiping Liu;Jia Zhang;Liumin Deng;Sheng He;Yong Wu;Lin‐Fei Qiu
Noble gases in lunar soils provide critical information regarding solar wind and cosmic-ray interactions with the lunar surface, as well as the history of impact events affecting the regolith turnover processes. Here, we studied the characteristics of noble gases He, Ne, Ar in Chang’E-5 soil. High4He/36Ar and20Ne/36Ar values show that the soil has typical mare terrain characteristics. Furthermore, both values are higher than those in other lunar soils, suggesting the secondary processes occurring in the soil may have been less strong than in other lunar samples. Trapped (3He/4He)trand (20Ne/22Ne)trvalues were less fractionated than those of Apollo soils, also indicating the weak secondary processes the Chang’E-5 soil underwent. Trapped (40Ar/36Ar)trvalues indicate the implanted solar wind was young. The integrated exposure times to solar wind of the soil on the lunar surface suggest the Chang’E-5 soil was not seriously admixed by sputtered material from nearby rocks.