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  2. 地质与地球物理研究所
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  4. 岩石圈演化国家重点实验室
Low Ni and Co olivine in Chang'E-5 basalts reveals the origin of the young volcanism on the Moon

文献类型：期刊论文

作者Su, Bin2; Zhang, Di2,3; Chen, Yi2,3; Yang, Wei1; Mao, Qian2; Li, Xian-Hua2; Wu, Fu-Yuan2
刊名SCIENCE BULLETIN
出版日期2023-09-15
卷号68期号:17页码:1918-1927
ISSN号2095-9273
关键词Chang'E-5 Mare basalts Olivine Minor elements Lunar magma ocean
DOI10.1016/j.scib.2023.07.020
英文摘要Mare basalts returned by the Chang'E-5 (CE5) mission extend the duration of lunar volcanism almost one billion years longer than previously dated. Recent studies demonstrated that the young volcanism was related neither to radiogenic heating nor to hydrous melting. These findings beg the question of how the young lunar volcanism happened. Here we perform high-precision minor element analyses of olivine in the CE5 basalts, focusing on Ni and Co. Our results reveal that the CE5 basalt olivines have overall lower Ni and Co than those in the Apollo low-Ti basalts. The distinctive olivine chemistry with recently reported bulk-rock chemistry carries evidence for more late-stage clinopyroxene-ilmenite cumulates of the lunar magma ocean (LMO) in the CE5 mantle source. The involvement of these Fe-rich cumulates could lower the mantle melting temperature and produce low MgO magma, inhibiting Ni and Co partitioning into the magma during lunar mantle melting and forming low Ni and Co olivines for the CE5 basalts. Moreover, the CE5 olivines show a continuous decrease of Ni and Co with crystallization proceeding. Fractional crystallization modeling indicates that Co decreasing with crystallization resulted from CaO and TiO2 enrichment (with MgO and SiO2 depletion) in the CE5 primary magma. This further supports the significant contribution of late-stage LMO cumulates to the CE5 volcanic formation. We suggest that adding easily melted LMO components resulting in mantle melting point depression is a key pathway for driving prolonged lunar volcanism. This study highlights the usefulness of olivine for investigating magmatic processes on the Moon.(c) 2023 Science China Press. Published by Elsevier B.V. and Science China Press. All rights reserved.
WOS关键词MARE BASALTS ; PARTITION-COEFFICIENTS ; TRACE-ELEMENTS ; PLANETARY BASALTS ; LAPAZ ICEFIELD ; ION MICROPROBE ; GREEN GLASSES ; MAGMA OCEAN ; LUNAR ; PETROGENESIS
资助项目National Natural Science Foundation of China[42272057] ; Key Research Program of the Chinese Academy of Sciences[ZDBS-SSW-JSC007-15] ; Key Research Program of the Institute of Geology and Geophysics, Chinese Academy of Sciences[IGGCAS-202101] ; Experimental Technology Innovation Fund of the IGGCAS[11990890]
WOS研究方向Science & Technology - Other Topics
语种英语
出版者ELSEVIER
WOS记录号WOS:001076691500001
资助机构National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Key Research Program of the Chinese Academy of Sciences ; Key Research Program of the Chinese Academy of Sciences ; Key Research Program of the Chinese Academy of Sciences ; Key Research Program of the Chinese Academy of Sciences ; Key Research Program of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Key Research Program of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Key Research Program of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Key Research Program of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Experimental Technology Innovation Fund of the IGGCAS ; Experimental Technology Innovation Fund of the IGGCAS ; Experimental Technology Innovation Fund of the IGGCAS ; Experimental Technology Innovation Fund of the IGGCAS ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Key Research Program of the Chinese Academy of Sciences ; Key Research Program of the Chinese Academy of Sciences ; Key Research Program of the Chinese Academy of Sciences ; Key Research Program of the Chinese Academy of Sciences ; Key Research Program of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Key Research Program of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Key Research Program of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Key Research Program of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Experimental Technology Innovation Fund of the IGGCAS ; Experimental Technology Innovation Fund of the IGGCAS ; Experimental Technology Innovation Fund of the IGGCAS ; Experimental Technology Innovation Fund of the IGGCAS ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Key Research Program of the Chinese Academy of Sciences ; Key Research Program of the Chinese Academy of Sciences ; Key Research Program of the Chinese Academy of Sciences ; Key Research Program of the Chinese Academy of Sciences ; Key Research Program of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Key Research Program of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Key Research Program of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Key Research Program of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Experimental Technology Innovation Fund of the IGGCAS ; Experimental Technology Innovation Fund of the IGGCAS ; Experimental Technology Innovation Fund of the IGGCAS ; Experimental Technology Innovation Fund of the IGGCAS ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Key Research Program of the Chinese Academy of Sciences ; Key Research Program of the Chinese Academy of Sciences ; Key Research Program of the Chinese Academy of Sciences ; Key Research Program of the Chinese Academy of Sciences ; Key Research Program of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Key Research Program of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Key Research Program of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Key Research Program of the Institute of Geology and Geophysics, Chinese Academy of Sciences ; Experimental Technology Innovation Fund of the IGGCAS ; Experimental Technology Innovation Fund of the IGGCAS ; Experimental Technology Innovation Fund of the IGGCAS ; Experimental Technology Innovation Fund of the IGGCAS
源URL[http://ir.iggcas.ac.cn/handle/132A11/110794]  
专题地质与地球物理研究所_岩石圈演化国家重点实验室
地质与地球物理研究所_中国科学院地球与行星物理重点实验室
通讯作者Su, Bin
作者单位1.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing 100029, Peoples R China
2.Chinese Acad Sci, Inst Geol & Geophys, State Key Lab Lithospher Evolut, Beijing 100029, Peoples R China
3.Univ Chinese Acad Sci, Coll Earth & Planetary Sci, Beijing 100049, Peoples R China
推荐引用方式
GB/T 7714		 Su, Bin,Zhang, Di,Chen, Yi,et al. Low Ni and Co olivine in Chang'E-5 basalts reveals the origin of the young volcanism on the Moon[J]. SCIENCE BULLETIN,2023,68(17):1918-1927.
APA Su, Bin.,Zhang, Di.,Chen, Yi.,Yang, Wei.,Mao, Qian.,...&Wu, Fu-Yuan.(2023).Low Ni and Co olivine in Chang'E-5 basalts reveals the origin of the young volcanism on the Moon.SCIENCE BULLETIN,68(17),1918-1927.
MLA Su, Bin,et al."Low Ni and Co olivine in Chang'E-5 basalts reveals the origin of the young volcanism on the Moon".SCIENCE BULLETIN 68.17(2023):1918-1927.

入库方式： OAI收割

来源：地质与地球物理研究所

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