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Fusible mantle cumulates trigger young mare volcanism on the cooling Moon

文献类型：期刊论文

作者Su, Bin3; Yuan, Jiangyan3; Chen, Yi3; Yang, Wei4; Mitchell, Ross N.3; Hui, Hejiu1,2,5; Wang, Hao3; Tian, Hengci4; Li, Xian-Hua3; Wu, Fu-Yuan3
刊名SCIENCE ADVANCES
出版日期2022-10-19
卷号8期号:42页码:7
ISSN号2375-2548
DOI10.1126/sciadv.abn2103
英文摘要The Chang'E-5 (CE5) mission has demonstrated that lunar volcanism was still active until two billion years ago, much younger than the previous isotopically dated lunar basalts. How the small Moon retained enough heat to drive such late volcanism is unknown, particularly as the CE5 mantle source was anhydrous and depleted in heat-producing elements. We conduct fractional crystallization and mantle melting simulations that show that mantle melting point depression by the presence of fusible, easily melted components could trigger young volcanism. Enriched in calcium oxide and titanium dioxide compared to older Apollo magmas, the young CE5 magma was, thus, sourced from the overturn of the late-stage fusible cumulates of the lunar magma ocean. Mantle melting point depression is the first mechanism to account for young volcanism on the Moon that is consistent with the newly returned CE5 basalts.
WOS关键词EXPERIMENTAL CONSTRAINTS ; LUNAR ; BASALTS ; PETROGENESIS ; ORIGIN ; GLASSES ; CRYSTALLIZATION ; MAGMATISM ; EVOLUTION ; ILMENITE
资助项目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]
WOS研究方向Science & Technology - Other Topics
语种英语
WOS记录号WOS:000880308800001
出版者AMER ASSOC ADVANCEMENT SCIENCE
资助机构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 ; 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 ; 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 ; 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
源URL[http://ir.iggcas.ac.cn/handle/132A11/107719]  
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; Chen, Yi
作者单位1.Nanjing Univ, Sch Earth Sci & Engn, State Key Lab Mineral Deposits Res, Nanjing 210023, Peoples R China
2.CAS Ctr Excellence Comparat Planetol, Hefei 230026, Peoples R China
3.Chinese Acad Sci, Inst Geol & Geophys, State Key Lab Lithospher Evolut, Beijing 100029, Peoples R China
4.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing 100029, Peoples R China
5.Nanjing Univ, Sch Earth Sci & Engn, Lunar & Planetary Sci Inst, Nanjing 210023, Peoples R China
推荐引用方式
GB/T 7714		 Su, Bin,Yuan, Jiangyan,Chen, Yi,et al. Fusible mantle cumulates trigger young mare volcanism on the cooling Moon[J]. SCIENCE ADVANCES,2022,8(42):7.
APA Su, Bin.,Yuan, Jiangyan.,Chen, Yi.,Yang, Wei.,Mitchell, Ross N..,...&Wu, Fu-Yuan.(2022).Fusible mantle cumulates trigger young mare volcanism on the cooling Moon.SCIENCE ADVANCES,8(42),7.
MLA Su, Bin,et al."Fusible mantle cumulates trigger young mare volcanism on the cooling Moon".SCIENCE ADVANCES 8.42(2022):7.

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来源：地质与地球物理研究所

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