中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Compositional Variability of 2.0-Ga Lunar Basalts at the Chang'e-5 Landing Site

文献类型:期刊论文

作者Boschi, Samuele1; Wang, Xiao-Lei1; Hui, Hejiu2,3; Yin, Zongjun4; Guan, Yue1; Hu, Huan1; Zhang, Wenlan1; Chen, Jiayang1; Li, Weiqiang1,2,3
刊名JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS
出版日期2023-05-01
卷号128期号:5页码:12
ISSN号2169-9097
关键词Chang'e-5 lunar basalt SIMS pigeonite compositional variability
DOI10.1029/2022JE007627
通讯作者Li, Weiqiang(liweiqiang@nju.edu.cn)
英文摘要China's Chang'e-5 (CE-5) mission successfully returned a total of 1.731 kg of lunar material from the north-eastern Oceanus Procellarum region. Young (similar to 2.0 Ga) ages were reported from the CE-5 basalts. However, there are controversies on whether they are low-Ti or high-Ti mare basalt type. Here, we report the results of a comprehensive petrographic, elemental, and Pb isotopic investigation on a 17.6 mg CE-5 basalt clast (CE5C0000YJYX048). By combining high-resolution X-ray tomography of the clast and microbeam (scanning electron microscope SEM, electron probe microanalyzer EPMA) analyses of mineral grains peeled off the clast surface, we derived the bulk clast chemical composition with a very small sample consumption (i.e., <3 mg). The poikilitic clast has a bulk TiO2 content of 3.78 +/- 1.01 wt%, which is representative of a low-Ti basalt end-member in the lunar mare basalts samples. Furthermore, the pyroxene in the studied clast is dominantly pigeonite, in contrast to other reported CE-5 samples where augite is the dominant pyroxene mineralogy. Despite these compositional peculiarities, in situ secondary ion mass spectrometer dating yielded a Pb-Pb age of 2,040 +/- 22 Ma for the fragment, which is consistent with ages reported from other CE-5. Based on the chemical and age data analyzed in this study, it can be concluded that the lunar basalts obtained from the CE-5 mission originated from a low-Ti mare basalt-type source. The mineral composition of the mare basalt clast studied, which is dominated by pigeonite, fayalite, and anorthite, likely resulted from late-stage magmatic crystallization when the magma was enriched in Fe.
WOS关键词MARE BASALTS ; RARE-EARTH ; PETROGENESIS ; MINERALOGY ; DIVERSITY ; CHEMISTRY ; REGOLITH ; MELT
WOS研究方向Geochemistry & Geophysics
语种英语
出版者AMER GEOPHYSICAL UNION
WOS记录号WOS:001000271300001
源URL[http://ir.nigpas.ac.cn/handle/332004/42132]  
专题中国科学院南京地质古生物研究所
通讯作者Li, Weiqiang
作者单位1.Nanjing Univ, Sch Earth Sci & Engn, State Key Lab Mineral Deposits Res, Nanjing, Peoples R China
2.Nanjing Univ, Lunar & Planetary Sci Inst, Sch Earth Sci & Engn, Nanjing, Peoples R China
3.CAS Ctr Excellence Comparat Planetol, Hefei, Peoples R China
4.Chinese Acad Sci, Nanjing Inst Geol & Palaeontol, State Key Lab Palaeobiol & Stratig, Nanjing, Peoples R China
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GB/T 7714
Boschi, Samuele,Wang, Xiao-Lei,Hui, Hejiu,et al. Compositional Variability of 2.0-Ga Lunar Basalts at the Chang'e-5 Landing Site[J]. JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS,2023,128(5):12.
APA Boschi, Samuele.,Wang, Xiao-Lei.,Hui, Hejiu.,Yin, Zongjun.,Guan, Yue.,...&Li, Weiqiang.(2023).Compositional Variability of 2.0-Ga Lunar Basalts at the Chang'e-5 Landing Site.JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS,128(5),12.
MLA Boschi, Samuele,et al."Compositional Variability of 2.0-Ga Lunar Basalts at the Chang'e-5 Landing Site".JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS 128.5(2023):12.

入库方式: OAI收割

来源:南京地质古生物研究所

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