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月球近侧和远侧空间风化的差异:来自嫦娥六号样本的证据。

Differences in space weathering between the near and far side of the Moon: evidence from Chang'e-6 samples.

作者信息

Lin Jiarui, Xian Haiyang, Yang Yiping, Li Shan, Xi Jiaxin, Lin Xiaoju, Xiao Yao, Chen Shengdong, Zhao Chenyi, Zhang Miaomiao, Tsuchiyama Akira, Zhu Jianxi, He Hongping, Xu Yi-Gang

机构信息

State Key Laboratory of Deep Earth Processes and Resources, Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, Guangzhou 510640, China.

Center for Advanced Planetary Science (CAPS), Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, Guangzhou 510640, China.

出版信息

Natl Sci Rev. 2025 Mar 5;12(6):nwaf087. doi: 10.1093/nsr/nwaf087. eCollection 2025 Jun.

Abstract

The differences in terrain and chemical composition between the far side of the Moon (lunar farside) and the near side have been identified through remote sensing spectroscopy. The lunar farside samples returned by the Chang'e-6 mission show differences in terms of space weathering features compared to nearside samples. The studied farside samples lack vapor deposition layers found on the nearside and exhibit thinner amorphized layers, lower solar flare track densities, reduced number densities of nano phase metallic iron (npFe) and larger npFe grain sizes. These findings suggest that the solar wind plays a dominant role in space weathering on the Chang'e-6 sampling site, surpassing micrometeorite impacts. This could provide critical sample-based evidence of the lunar space environment's dichotomy, enhancing our understanding of how solar wind and micrometeoroid impacts shape the lunar surface, even over short exposure periods.

摘要

通过遥感光谱法已确定了月球背面(月背)与正面在地形和化学成分上的差异。嫦娥六号任务带回的月背样本与正面样本相比,在空间风化特征方面存在差异。所研究的月背样本缺乏在正面发现的气相沉积层,且呈现出更薄的非晶化层、更低的太阳耀斑轨迹密度、更低的纳米相金属铁(npFe)数密度以及更大的npFe晶粒尺寸。这些发现表明,太阳风在嫦娥六号采样点的空间风化过程中起主导作用,超过了微陨石撞击的影响。这可为月球空间环境二分法提供关键的基于样本的证据,增进我们对太阳风和微流星体撞击如何塑造月球表面的理解,即使在短暴露期内也是如此。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/d190/12051863/a2533054055a/nwaf087fig1.jpg

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