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在嫦娥六号月壤中发现撞击诱发的超高熔点硫镁钙石。

Impact-induced ultra-high melting point oldhamite discovered in Chang'E-6 lunar soil.

作者信息

Li Chen, Li Yang, Pang Ronghua, Xie Jiyang, Han Zixuan, Wen Yuanyun, Zeng Xiaojia, Wang Li, Qin Ziyan, Yang Jie, Hu Wanbiao, Liu Jianzhong, Li Xiongyao, Ma Wenhui

机构信息

Center for Lunar and Planetary Sciences, Institute of Geochemistry, Chinese Academy of Sciences, Guiyang, China.

School of Engineering, Yunnan University, Kunming, China.

出版信息

Nat Commun. 2025 Mar 4;16(1):2155. doi: 10.1038/s41467-025-57337-0.

DOI:10.1038/s41467-025-57337-0
PMID:40038308
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC11880381/
Abstract

Chang'E-6 lunar soil was the first sample collected on the lunar farside. It provides insights into impact history and thermodynamic evolution of the Moon. Here we show the discovered widespread oldhamite (CaS) in lunar regolith samples. Analysis of the microscopic composition and crystal structure showed that the oldhamite has a cubic structure and presence at the interface of glass and iron on the surface of the impact glass beads, suggesting a interface thermochemical reaction. Thermodynamic calculations show that the formation of chemical reactions requires a reducing atmosphere and high temperature to ensure reducing environment and high iron activity for promoting the interaction. Such environment suggests a potential large-scale, high-energy impact event with a S-rich asteroid or involving lunar S-rich mantle-core excavation. Oldhamite has never been observed in other lunar samples from near side. Our findings reveal a unique evolution history of the South Pole-Aitken basin, which is distinct from nearside.

摘要

嫦娥六号月球土壤是首次在月球背面采集的样本。它为月球的撞击历史和热力学演化提供了见解。在此我们展示了在月球风化层样本中发现的广泛存在的硫钙石(CaS)。对微观成分和晶体结构的分析表明,硫钙石具有立方结构,且存在于撞击玻璃珠表面的玻璃与铁的界面处,这表明存在界面热化学反应。热力学计算表明,化学反应的形成需要还原性气氛和高温,以确保还原环境和高铁活性来促进相互作用。这种环境表明可能发生了与富含硫的小行星的大规模、高能撞击事件,或者涉及挖掘月球富含硫的地幔 - 核心。在来自月球近侧的其他样本中从未观察到硫钙石。我们的发现揭示了南极 - 艾特肯盆地独特的演化历史,这与近侧不同。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e2bd/11880381/fe09c81f06fe/41467_2025_57337_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e2bd/11880381/83d68cbb8c6e/41467_2025_57337_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e2bd/11880381/427a5bc0e231/41467_2025_57337_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e2bd/11880381/1282aca4aaa0/41467_2025_57337_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e2bd/11880381/2ef62a99295c/41467_2025_57337_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e2bd/11880381/fe09c81f06fe/41467_2025_57337_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e2bd/11880381/83d68cbb8c6e/41467_2025_57337_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e2bd/11880381/427a5bc0e231/41467_2025_57337_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e2bd/11880381/1282aca4aaa0/41467_2025_57337_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e2bd/11880381/2ef62a99295c/41467_2025_57337_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/e2bd/11880381/fe09c81f06fe/41467_2025_57337_Fig5_HTML.jpg

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本文引用的文献

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2
Geological context of the Chang'e-6 landing area and implications for sample analysis.嫦娥六号着陆区的地质背景及其对样品分析的意义。
Innovation (Camb). 2024 Jun 24;5(5):100663. doi: 10.1016/j.xinn.2024.100663. eCollection 2024 Sep 9.
3
Redox condition changes caused by impacts: Insights from Chang'e-5 lunar glass beads.
撞击引起的氧化还原条件变化:来自嫦娥五号月球玻璃珠的见解
Sci Bull (Beijing). 2024 May 30;69(10):1495-1505. doi: 10.1016/j.scib.2024.03.004. Epub 2024 Mar 4.
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Oldhamite: a new link in upper mantle for C-O-S-Ca cycles and an indicator for planetary habitability.奥尔德姆石:上地幔中碳-氧-硫-钙循环的新环节及行星宜居性指标。
Natl Sci Rev. 2023 Jun 5;10(10):nwad159. doi: 10.1093/nsr/nwad159. eCollection 2023 Oct.
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Vapor-deposited digenite in Chang'e-5 lunar soil.嫦娥五号月壤中的气相沉积蓝辉铜矿
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Sub-microscopic magnetite and metallic iron particles formed by eutectic reaction in Chang'E-5 lunar soil.嫦娥五号月壤中通过共晶反应形成的亚微观磁铁矿和金属铁颗粒。
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