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太阳风注入促进月球土壤中微相铁颗粒生长。

Microphase iron particle growth promoted by solar wind implantation in lunar soils.

作者信息

Lu Xuejin, Chen Jian, Cao Haijun, Fu Xiaohui, Zeng Xiaojia, Qiao Le, Liu Chengbao, Zhang Guang, Zhang Peng, Ling Zongcheng

机构信息

Shandong Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Institute of Space Sciences, Shandong University, No. 180, Wenhua Xilu, Huancui District, Weihai 264209, China.

Technology and Engineering Center for Space Utilization, Chinese Academy of Sciences, No. 9, Dengzhuang Nanlu, Hai Dian District, Beijing 100094, China.

出版信息

PNAS Nexus. 2024 Oct 8;3(10):pgae450. doi: 10.1093/pnasnexus/pgae450. eCollection 2024 Oct.

Abstract

Lunar soils record the history and spectral changes resulting from the space-weathering process. The solar wind and micrometeoroids are the main space-weathering agents leading to darkening (decreasing albedo) and reddening (increasing reflectance with longer wavelength) of visible and near-infrared spectra. Nevertheless, their relative contributions are not well constrained and understood. In this study, we examine the near-infrared spectral variation as a function of lunar latitude and chemical composition using remote spectroscopic analysis of mare basalts and swirl regions. The results indicate that the reflectance of lunar mature soils darkens and the spectral slope flattens (reddening effect saturation) in areas of enhanced solar wind flux. We propose a previously unrecognized stage of space weathering (the post-mature stage), in which solar wind implantation may contribute to the growth and coarsening of metallic iron particles into larger microphase iron. This space-weathering mechanism is dominated by the solar wind and has important implications for understanding the alteration processes of airless bodies across our solar system.

摘要

月球土壤记录了空间风化过程产生的历史和光谱变化。太阳风和微流星体是导致可见光和近红外光谱变暗(反照率降低)和变红(随着波长变长反射率增加)的主要空间风化因素。然而,它们的相对贡献尚未得到很好的限制和理解。在这项研究中,我们使用月海玄武岩和漩涡区域的遥感光谱分析,研究了近红外光谱变化作为月球纬度和化学成分的函数。结果表明,在太阳风通量增强的区域,月球成熟土壤的反射率变暗,光谱斜率变平(变红效应饱和)。我们提出了一个以前未被认识到的空间风化阶段(成熟后阶段),其中太阳风注入可能有助于金属铁颗粒生长和粗化成为更大的微相铁。这种空间风化机制以太阳风为主导,对于理解我们太阳系中无大气天体的蚀变过程具有重要意义。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/fce9/11521327/7092540782be/pgae450f1.jpg

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