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Article: Mineralogy of Surface Materials at the Chang'E-5 Landing Site and Possible Exotic Sources From In Situ Spectral Observations

TitleMineralogy of Surface Materials at the Chang'E-5 Landing Site and Possible Exotic Sources From In Situ Spectral Observations
Authors
KeywordsChang'E-5
exotic material origin
lunar mineralogical spectrometer
Moon
northern Oceanus procellarum
spectral data analysis
Issue Date2023
Citation
Journal of Geophysical Research: Planets, 2023, v. 128, n. 10, article no. e2023JE007908 How to Cite?
AbstractChina's Chang'E-5 (CE-5) mission landed at 43.06°N and 51.92°W on 1 December 2020, within the Northern Oceanus Procellarum region of the Moon. The CE-5 landing site is situated within a young lunar basalt unit estimated to be around 2.0 Ga. A comprehensive understanding of the lunar regolith composition within the CE-5 region is pivotal as it furnishes additional scientific evidence concerning its origin. This, in turn, would further improve our understanding of lunar geology and evolution. In our studies, we employed a variety of spectral data and derived products including the CE-5 Lunar Mineralogical Spectrometer data, the ferrous mineral abundance derived from Kaguya Multiband Imager, and the Chandrayaan-1 Moon Mineralogical Mapper data. These data enabled us to determine and analyze the compositions of the diverse materials present in the CE-5 region and to pinpoint the origins of exotic materials found therein. Our results indicated that the exotic material within the CE-5 region is principally composed of clinopyroxene and plagioclase (Pl). Further analysis unveils that the CE-5 regolith embodies a blend of two distinct varieties of clinopyroxene, designated as Type A and Type B, along with feldspar. This discovery markedly diverges from the conclusions drawn by preceding studies, which relied solely on remote sensing data. Moreover, the exotic materials are predominantly constituted by the ejecta of Harpalus and Aristarchus craters. This finding furnishes a substantial geological background for the analysis of exotic materials in the samples returned by the CE-5 mission in forthcoming studies.
Persistent Identifierhttp://hdl.handle.net/10722/353119
ISSN
2023 Impact Factor: 3.9
2023 SCImago Journal Rankings: 1.650
ISI Accession Number ID

 

DC FieldValueLanguage
dc.contributor.authorYang, Maosheng-
dc.contributor.authorQian, Yuqi-
dc.contributor.authorHorgan, Briony-
dc.contributor.authorHuang, Jun-
dc.contributor.authorXiao, Long-
dc.date.accessioned2025-01-13T03:02:10Z-
dc.date.available2025-01-13T03:02:10Z-
dc.date.issued2023-
dc.identifier.citationJournal of Geophysical Research: Planets, 2023, v. 128, n. 10, article no. e2023JE007908-
dc.identifier.issn2169-9097-
dc.identifier.urihttp://hdl.handle.net/10722/353119-
dc.description.abstractChina's Chang'E-5 (CE-5) mission landed at 43.06°N and 51.92°W on 1 December 2020, within the Northern Oceanus Procellarum region of the Moon. The CE-5 landing site is situated within a young lunar basalt unit estimated to be around 2.0 Ga. A comprehensive understanding of the lunar regolith composition within the CE-5 region is pivotal as it furnishes additional scientific evidence concerning its origin. This, in turn, would further improve our understanding of lunar geology and evolution. In our studies, we employed a variety of spectral data and derived products including the CE-5 Lunar Mineralogical Spectrometer data, the ferrous mineral abundance derived from Kaguya Multiband Imager, and the Chandrayaan-1 Moon Mineralogical Mapper data. These data enabled us to determine and analyze the compositions of the diverse materials present in the CE-5 region and to pinpoint the origins of exotic materials found therein. Our results indicated that the exotic material within the CE-5 region is principally composed of clinopyroxene and plagioclase (Pl). Further analysis unveils that the CE-5 regolith embodies a blend of two distinct varieties of clinopyroxene, designated as Type A and Type B, along with feldspar. This discovery markedly diverges from the conclusions drawn by preceding studies, which relied solely on remote sensing data. Moreover, the exotic materials are predominantly constituted by the ejecta of Harpalus and Aristarchus craters. This finding furnishes a substantial geological background for the analysis of exotic materials in the samples returned by the CE-5 mission in forthcoming studies.-
dc.languageeng-
dc.relation.ispartofJournal of Geophysical Research: Planets-
dc.subjectChang'E-5-
dc.subjectexotic material origin-
dc.subjectlunar mineralogical spectrometer-
dc.subjectMoon-
dc.subjectnorthern Oceanus procellarum-
dc.subjectspectral data analysis-
dc.titleMineralogy of Surface Materials at the Chang'E-5 Landing Site and Possible Exotic Sources From In Situ Spectral Observations-
dc.typeArticle-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1029/2023JE007908-
dc.identifier.scopuseid_2-s2.0-85174859548-
dc.identifier.volume128-
dc.identifier.issue10-
dc.identifier.spagearticle no. e2023JE007908-
dc.identifier.epagearticle no. e2023JE007908-
dc.identifier.eissn2169-9100-
dc.identifier.isiWOS:001089495900001-

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