Diverse Geological Evolution of Impact Basins on the Moon
文献类型:期刊论文
作者 | Deng, Jiayin2,3; Cheng, Weiming1,2,3,4; Jiao, Yimeng2,3 |
刊名 | REMOTE SENSING
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出版日期 | 2022-12-01 |
卷号 | 14期号:24页码:21 |
关键词 | moon impact basins geological features chemical composition mineralogical composition |
DOI | 10.3390/rs14246335 |
通讯作者 | Cheng, Weiming(chengwm@lreis.ac.cn) |
英文摘要 | Impact basins are the dominant landforms on the lunar surface, and their geological evolution varies. This research studied the diversity in the geological evolution of three impact basins: the Dirichlet-Jackson Basin, the Nectaris Basin, and the Orientale Basin. First, the regional topography and geomorphology of the three basins were studied using the SLDEM2015 digital elevation model (DEM). Clementine ultraviolet-visible (UVVIS) data and Moon Mineralogy Mapper (M3) data were used to study the chemical composition and mineralogical composition of the three basins. Additionally, the lunar crust thickness data have been used to study the subsurface structure of the three basins. The topographical analogies of the three basins indicate that the shapes of the basins are cavity-like. However, the shape of the Dirichlet-Jackson basin is not an obvious cavity compared with the other basins. The positions with minimum and maximum crustal thickness of the three basins are located at the center and the rim. The uplift of the crust-mantle interface of the Nectaris Basin and Orientale Basin is relatively larger than in the Dirichlet-Jackson Basin. Below the center of the maria of the Nectaris Basin and Orientale Basin, collapses occurred at the crust-mantle interface. The concentrations of FeO and TiO2 in the non-mare formation of the basin and maria show expected bimodal distributions. Moreover, we found exposures of olivine-rich materials in the Nectaris Basin and Orientale Basin which are located in the Rosse and Maunder craters, respectively. These exposures of olivine may be explained by the fact that the formation of the large impact basin, which might penetrate and blast away the upper lunar crust, excavating deep-seated material. |
WOS关键词 | MULTIRING BASINS ; LUNAR ; ORIENTALE ; ABUNDANCE ; HISTORY ; MODEL ; IRON |
WOS研究方向 | Environmental Sciences & Ecology ; Geology ; Remote Sensing ; Imaging Science & Photographic Technology |
语种 | 英语 |
WOS记录号 | WOS:000903348000001 |
出版者 | MDPI |
源URL | [http://ir.igsnrr.ac.cn/handle/311030/188362] ![]() |
专题 | 中国科学院地理科学与资源研究所 |
通讯作者 | Cheng, Weiming |
作者单位 | 1.Jiangsu Ctr Collaborat Innovat Geog Informat Resou, Nanjing 210023, Peoples R China 2.Chinese Acad Sci, Inst Geog Sci & Nat Resources Res, State Key Lab Resources & Environm Informat Syst, Beijing 100101, Peoples R China 3.Univ Chinese Acad Sci, Beijing 100049, Peoples R China 4.Chinese Acad Sci, Ctr Excellence Comparat Planetol, Hefei 230052, Peoples R China |
推荐引用方式 GB/T 7714 | Deng, Jiayin,Cheng, Weiming,Jiao, Yimeng. Diverse Geological Evolution of Impact Basins on the Moon[J]. REMOTE SENSING,2022,14(24):21. |
APA | Deng, Jiayin,Cheng, Weiming,&Jiao, Yimeng.(2022).Diverse Geological Evolution of Impact Basins on the Moon.REMOTE SENSING,14(24),21. |
MLA | Deng, Jiayin,et al."Diverse Geological Evolution of Impact Basins on the Moon".REMOTE SENSING 14.24(2022):21. |
入库方式: OAI收割
来源:地理科学与资源研究所
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