Size, morphology, and composition of lunar samples returned by Chang’E-5 mission
Abstract This study focuses on the physical and chemical properties of surficial lunar regolith (LR) samples returned from the Moon by the Chang’E-5 (CE-5) mission. Insights regarding the effect of a new sampling geological site on the surficial lunar sample CE5C0400 were illustrated using nondestru...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Zhang, Hui [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2021 |
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| Anmerkung: |
© Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature 2021 |
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| Übergeordnetes Werk: |
Enthalten in: Science in China - Heidelberg : Springer, 2003, 65(2021), 2 vom: 10. Dez. |
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| Übergeordnetes Werk: |
volume:65 ; year:2021 ; number:2 ; day:10 ; month:12 |
| Links: |
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| DOI / URN: |
10.1007/s11433-021-1818-1 |
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| 520 | |a Abstract This study focuses on the physical and chemical properties of surficial lunar regolith (LR) samples returned from the Moon by the Chang’E-5 (CE-5) mission. Insights regarding the effect of a new sampling geological site on the surficial lunar sample CE5C0400 were illustrated using nondestructive techniques such as laser diffractometry coupled with image analysis, X-ray computed tomography, and field emission scanning electron microscopy equipped with energy dispersive spectroscopy, and X-ray diffraction combined with Rietveld refinement. From the characterization analyses, the CE-5 sampling site in the northeastern Oceanus Procellarum on the Moon yields a unique collection of relatively regular-shaped and fine basalt-dominated particles. The median grain size D50 is (55.24±0.96) µm, falling within the relatively low end of the range of the Apollo lunar returned samples. The coefficient of uniformity Cu of 15.1 and the coefficient of curvature Cc of 1.7 could classify CE5C0400 to be well-graded. The minerals in CE5C0400 comprise approximately 44.5% pyroxene, 30.4% plagioclase, 3.6% olivine, and 6.0% ilmenite. There is a relatively low content of approximately 15.5% glass phase in the CE-5 lunar sample. From the results, we deduce that the CE-5 LR structure could have mainly resulted from micrometeoroid impacts to achieve such a high level of maturity. | ||
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10.1007/s11433-021-1818-1 doi (DE-627)SPR050351370 (SPR)s11433-021-1818-1-e DE-627 ger DE-627 rakwb eng Zhang, Hui verfasserin aut Size, morphology, and composition of lunar samples returned by Chang’E-5 mission 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature 2021 Abstract This study focuses on the physical and chemical properties of surficial lunar regolith (LR) samples returned from the Moon by the Chang’E-5 (CE-5) mission. Insights regarding the effect of a new sampling geological site on the surficial lunar sample CE5C0400 were illustrated using nondestructive techniques such as laser diffractometry coupled with image analysis, X-ray computed tomography, and field emission scanning electron microscopy equipped with energy dispersive spectroscopy, and X-ray diffraction combined with Rietveld refinement. From the characterization analyses, the CE-5 sampling site in the northeastern Oceanus Procellarum on the Moon yields a unique collection of relatively regular-shaped and fine basalt-dominated particles. The median grain size D50 is (55.24±0.96) µm, falling within the relatively low end of the range of the Apollo lunar returned samples. The coefficient of uniformity Cu of 15.1 and the coefficient of curvature Cc of 1.7 could classify CE5C0400 to be well-graded. The minerals in CE5C0400 comprise approximately 44.5% pyroxene, 30.4% plagioclase, 3.6% olivine, and 6.0% ilmenite. There is a relatively low content of approximately 15.5% glass phase in the CE-5 lunar sample. From the results, we deduce that the CE-5 LR structure could have mainly resulted from micrometeoroid impacts to achieve such a high level of maturity. Zhang, Xian aut Zhang, Guang aut Dong, Keqi aut Deng, Xiangjin aut Gao, Xiaosong aut Yang, Yaodong aut Xiao, Yuan aut Bai, Xiao aut Liang, Kaixin aut Liu, Yiwei aut Ma, Wenbin aut Zhao, Shaofan aut Zhang, Ce aut Zhang, Xiaojing aut Song, Jian aut Yao, Wei aut Chen, Hong aut Wang, Weihua aut Zou, Zhigang aut Yang, Mengfei aut Enthalten in Science in China Heidelberg : Springer, 2003 65(2021), 2 vom: 10. Dez. (DE-627)385614799 (DE-600)2142901-7 1862-2844 nnns volume:65 year:2021 number:2 day:10 month:12 https://dx.doi.org/10.1007/s11433-021-1818-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 AR 65 2021 2 10 12 |
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10.1007/s11433-021-1818-1 doi (DE-627)SPR050351370 (SPR)s11433-021-1818-1-e DE-627 ger DE-627 rakwb eng Zhang, Hui verfasserin aut Size, morphology, and composition of lunar samples returned by Chang’E-5 mission 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature 2021 Abstract This study focuses on the physical and chemical properties of surficial lunar regolith (LR) samples returned from the Moon by the Chang’E-5 (CE-5) mission. Insights regarding the effect of a new sampling geological site on the surficial lunar sample CE5C0400 were illustrated using nondestructive techniques such as laser diffractometry coupled with image analysis, X-ray computed tomography, and field emission scanning electron microscopy equipped with energy dispersive spectroscopy, and X-ray diffraction combined with Rietveld refinement. From the characterization analyses, the CE-5 sampling site in the northeastern Oceanus Procellarum on the Moon yields a unique collection of relatively regular-shaped and fine basalt-dominated particles. The median grain size D50 is (55.24±0.96) µm, falling within the relatively low end of the range of the Apollo lunar returned samples. The coefficient of uniformity Cu of 15.1 and the coefficient of curvature Cc of 1.7 could classify CE5C0400 to be well-graded. The minerals in CE5C0400 comprise approximately 44.5% pyroxene, 30.4% plagioclase, 3.6% olivine, and 6.0% ilmenite. There is a relatively low content of approximately 15.5% glass phase in the CE-5 lunar sample. From the results, we deduce that the CE-5 LR structure could have mainly resulted from micrometeoroid impacts to achieve such a high level of maturity. Zhang, Xian aut Zhang, Guang aut Dong, Keqi aut Deng, Xiangjin aut Gao, Xiaosong aut Yang, Yaodong aut Xiao, Yuan aut Bai, Xiao aut Liang, Kaixin aut Liu, Yiwei aut Ma, Wenbin aut Zhao, Shaofan aut Zhang, Ce aut Zhang, Xiaojing aut Song, Jian aut Yao, Wei aut Chen, Hong aut Wang, Weihua aut Zou, Zhigang aut Yang, Mengfei aut Enthalten in Science in China Heidelberg : Springer, 2003 65(2021), 2 vom: 10. Dez. (DE-627)385614799 (DE-600)2142901-7 1862-2844 nnns volume:65 year:2021 number:2 day:10 month:12 https://dx.doi.org/10.1007/s11433-021-1818-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 AR 65 2021 2 10 12 |
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10.1007/s11433-021-1818-1 doi (DE-627)SPR050351370 (SPR)s11433-021-1818-1-e DE-627 ger DE-627 rakwb eng Zhang, Hui verfasserin aut Size, morphology, and composition of lunar samples returned by Chang’E-5 mission 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature 2021 Abstract This study focuses on the physical and chemical properties of surficial lunar regolith (LR) samples returned from the Moon by the Chang’E-5 (CE-5) mission. Insights regarding the effect of a new sampling geological site on the surficial lunar sample CE5C0400 were illustrated using nondestructive techniques such as laser diffractometry coupled with image analysis, X-ray computed tomography, and field emission scanning electron microscopy equipped with energy dispersive spectroscopy, and X-ray diffraction combined with Rietveld refinement. From the characterization analyses, the CE-5 sampling site in the northeastern Oceanus Procellarum on the Moon yields a unique collection of relatively regular-shaped and fine basalt-dominated particles. The median grain size D50 is (55.24±0.96) µm, falling within the relatively low end of the range of the Apollo lunar returned samples. The coefficient of uniformity Cu of 15.1 and the coefficient of curvature Cc of 1.7 could classify CE5C0400 to be well-graded. The minerals in CE5C0400 comprise approximately 44.5% pyroxene, 30.4% plagioclase, 3.6% olivine, and 6.0% ilmenite. There is a relatively low content of approximately 15.5% glass phase in the CE-5 lunar sample. From the results, we deduce that the CE-5 LR structure could have mainly resulted from micrometeoroid impacts to achieve such a high level of maturity. Zhang, Xian aut Zhang, Guang aut Dong, Keqi aut Deng, Xiangjin aut Gao, Xiaosong aut Yang, Yaodong aut Xiao, Yuan aut Bai, Xiao aut Liang, Kaixin aut Liu, Yiwei aut Ma, Wenbin aut Zhao, Shaofan aut Zhang, Ce aut Zhang, Xiaojing aut Song, Jian aut Yao, Wei aut Chen, Hong aut Wang, Weihua aut Zou, Zhigang aut Yang, Mengfei aut Enthalten in Science in China Heidelberg : Springer, 2003 65(2021), 2 vom: 10. Dez. (DE-627)385614799 (DE-600)2142901-7 1862-2844 nnns volume:65 year:2021 number:2 day:10 month:12 https://dx.doi.org/10.1007/s11433-021-1818-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 AR 65 2021 2 10 12 |
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10.1007/s11433-021-1818-1 doi (DE-627)SPR050351370 (SPR)s11433-021-1818-1-e DE-627 ger DE-627 rakwb eng Zhang, Hui verfasserin aut Size, morphology, and composition of lunar samples returned by Chang’E-5 mission 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature 2021 Abstract This study focuses on the physical and chemical properties of surficial lunar regolith (LR) samples returned from the Moon by the Chang’E-5 (CE-5) mission. Insights regarding the effect of a new sampling geological site on the surficial lunar sample CE5C0400 were illustrated using nondestructive techniques such as laser diffractometry coupled with image analysis, X-ray computed tomography, and field emission scanning electron microscopy equipped with energy dispersive spectroscopy, and X-ray diffraction combined with Rietveld refinement. From the characterization analyses, the CE-5 sampling site in the northeastern Oceanus Procellarum on the Moon yields a unique collection of relatively regular-shaped and fine basalt-dominated particles. The median grain size D50 is (55.24±0.96) µm, falling within the relatively low end of the range of the Apollo lunar returned samples. The coefficient of uniformity Cu of 15.1 and the coefficient of curvature Cc of 1.7 could classify CE5C0400 to be well-graded. The minerals in CE5C0400 comprise approximately 44.5% pyroxene, 30.4% plagioclase, 3.6% olivine, and 6.0% ilmenite. There is a relatively low content of approximately 15.5% glass phase in the CE-5 lunar sample. From the results, we deduce that the CE-5 LR structure could have mainly resulted from micrometeoroid impacts to achieve such a high level of maturity. Zhang, Xian aut Zhang, Guang aut Dong, Keqi aut Deng, Xiangjin aut Gao, Xiaosong aut Yang, Yaodong aut Xiao, Yuan aut Bai, Xiao aut Liang, Kaixin aut Liu, Yiwei aut Ma, Wenbin aut Zhao, Shaofan aut Zhang, Ce aut Zhang, Xiaojing aut Song, Jian aut Yao, Wei aut Chen, Hong aut Wang, Weihua aut Zou, Zhigang aut Yang, Mengfei aut Enthalten in Science in China Heidelberg : Springer, 2003 65(2021), 2 vom: 10. Dez. (DE-627)385614799 (DE-600)2142901-7 1862-2844 nnns volume:65 year:2021 number:2 day:10 month:12 https://dx.doi.org/10.1007/s11433-021-1818-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 AR 65 2021 2 10 12 |
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10.1007/s11433-021-1818-1 doi (DE-627)SPR050351370 (SPR)s11433-021-1818-1-e DE-627 ger DE-627 rakwb eng Zhang, Hui verfasserin aut Size, morphology, and composition of lunar samples returned by Chang’E-5 mission 2021 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature 2021 Abstract This study focuses on the physical and chemical properties of surficial lunar regolith (LR) samples returned from the Moon by the Chang’E-5 (CE-5) mission. Insights regarding the effect of a new sampling geological site on the surficial lunar sample CE5C0400 were illustrated using nondestructive techniques such as laser diffractometry coupled with image analysis, X-ray computed tomography, and field emission scanning electron microscopy equipped with energy dispersive spectroscopy, and X-ray diffraction combined with Rietveld refinement. From the characterization analyses, the CE-5 sampling site in the northeastern Oceanus Procellarum on the Moon yields a unique collection of relatively regular-shaped and fine basalt-dominated particles. The median grain size D50 is (55.24±0.96) µm, falling within the relatively low end of the range of the Apollo lunar returned samples. The coefficient of uniformity Cu of 15.1 and the coefficient of curvature Cc of 1.7 could classify CE5C0400 to be well-graded. The minerals in CE5C0400 comprise approximately 44.5% pyroxene, 30.4% plagioclase, 3.6% olivine, and 6.0% ilmenite. There is a relatively low content of approximately 15.5% glass phase in the CE-5 lunar sample. From the results, we deduce that the CE-5 LR structure could have mainly resulted from micrometeoroid impacts to achieve such a high level of maturity. Zhang, Xian aut Zhang, Guang aut Dong, Keqi aut Deng, Xiangjin aut Gao, Xiaosong aut Yang, Yaodong aut Xiao, Yuan aut Bai, Xiao aut Liang, Kaixin aut Liu, Yiwei aut Ma, Wenbin aut Zhao, Shaofan aut Zhang, Ce aut Zhang, Xiaojing aut Song, Jian aut Yao, Wei aut Chen, Hong aut Wang, Weihua aut Zou, Zhigang aut Yang, Mengfei aut Enthalten in Science in China Heidelberg : Springer, 2003 65(2021), 2 vom: 10. Dez. (DE-627)385614799 (DE-600)2142901-7 1862-2844 nnns volume:65 year:2021 number:2 day:10 month:12 https://dx.doi.org/10.1007/s11433-021-1818-1 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_152 GBV_ILN_161 GBV_ILN_171 GBV_ILN_187 GBV_ILN_224 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 AR 65 2021 2 10 12 |
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Zhang, Hui @@aut@@ Zhang, Xian @@aut@@ Zhang, Guang @@aut@@ Dong, Keqi @@aut@@ Deng, Xiangjin @@aut@@ Gao, Xiaosong @@aut@@ Yang, Yaodong @@aut@@ Xiao, Yuan @@aut@@ Bai, Xiao @@aut@@ Liang, Kaixin @@aut@@ Liu, Yiwei @@aut@@ Ma, Wenbin @@aut@@ Zhao, Shaofan @@aut@@ Zhang, Ce @@aut@@ Zhang, Xiaojing @@aut@@ Song, Jian @@aut@@ Yao, Wei @@aut@@ Chen, Hong @@aut@@ Wang, Weihua @@aut@@ Zou, Zhigang @@aut@@ Yang, Mengfei @@aut@@ |
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Zhang, Hui Zhang, Xian Zhang, Guang Dong, Keqi Deng, Xiangjin Gao, Xiaosong Yang, Yaodong Xiao, Yuan Bai, Xiao Liang, Kaixin Liu, Yiwei Ma, Wenbin Zhao, Shaofan Zhang, Ce Zhang, Xiaojing Song, Jian Yao, Wei Chen, Hong Wang, Weihua Zou, Zhigang Yang, Mengfei |
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size, morphology, and composition of lunar samples returned by chang’e-5 mission |
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Size, morphology, and composition of lunar samples returned by Chang’E-5 mission |
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Abstract This study focuses on the physical and chemical properties of surficial lunar regolith (LR) samples returned from the Moon by the Chang’E-5 (CE-5) mission. Insights regarding the effect of a new sampling geological site on the surficial lunar sample CE5C0400 were illustrated using nondestructive techniques such as laser diffractometry coupled with image analysis, X-ray computed tomography, and field emission scanning electron microscopy equipped with energy dispersive spectroscopy, and X-ray diffraction combined with Rietveld refinement. From the characterization analyses, the CE-5 sampling site in the northeastern Oceanus Procellarum on the Moon yields a unique collection of relatively regular-shaped and fine basalt-dominated particles. The median grain size D50 is (55.24±0.96) µm, falling within the relatively low end of the range of the Apollo lunar returned samples. The coefficient of uniformity Cu of 15.1 and the coefficient of curvature Cc of 1.7 could classify CE5C0400 to be well-graded. The minerals in CE5C0400 comprise approximately 44.5% pyroxene, 30.4% plagioclase, 3.6% olivine, and 6.0% ilmenite. There is a relatively low content of approximately 15.5% glass phase in the CE-5 lunar sample. From the results, we deduce that the CE-5 LR structure could have mainly resulted from micrometeoroid impacts to achieve such a high level of maturity. © Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature 2021 |
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Abstract This study focuses on the physical and chemical properties of surficial lunar regolith (LR) samples returned from the Moon by the Chang’E-5 (CE-5) mission. Insights regarding the effect of a new sampling geological site on the surficial lunar sample CE5C0400 were illustrated using nondestructive techniques such as laser diffractometry coupled with image analysis, X-ray computed tomography, and field emission scanning electron microscopy equipped with energy dispersive spectroscopy, and X-ray diffraction combined with Rietveld refinement. From the characterization analyses, the CE-5 sampling site in the northeastern Oceanus Procellarum on the Moon yields a unique collection of relatively regular-shaped and fine basalt-dominated particles. The median grain size D50 is (55.24±0.96) µm, falling within the relatively low end of the range of the Apollo lunar returned samples. The coefficient of uniformity Cu of 15.1 and the coefficient of curvature Cc of 1.7 could classify CE5C0400 to be well-graded. The minerals in CE5C0400 comprise approximately 44.5% pyroxene, 30.4% plagioclase, 3.6% olivine, and 6.0% ilmenite. There is a relatively low content of approximately 15.5% glass phase in the CE-5 lunar sample. From the results, we deduce that the CE-5 LR structure could have mainly resulted from micrometeoroid impacts to achieve such a high level of maturity. © Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature 2021 |
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Abstract This study focuses on the physical and chemical properties of surficial lunar regolith (LR) samples returned from the Moon by the Chang’E-5 (CE-5) mission. Insights regarding the effect of a new sampling geological site on the surficial lunar sample CE5C0400 were illustrated using nondestructive techniques such as laser diffractometry coupled with image analysis, X-ray computed tomography, and field emission scanning electron microscopy equipped with energy dispersive spectroscopy, and X-ray diffraction combined with Rietveld refinement. From the characterization analyses, the CE-5 sampling site in the northeastern Oceanus Procellarum on the Moon yields a unique collection of relatively regular-shaped and fine basalt-dominated particles. The median grain size D50 is (55.24±0.96) µm, falling within the relatively low end of the range of the Apollo lunar returned samples. The coefficient of uniformity Cu of 15.1 and the coefficient of curvature Cc of 1.7 could classify CE5C0400 to be well-graded. The minerals in CE5C0400 comprise approximately 44.5% pyroxene, 30.4% plagioclase, 3.6% olivine, and 6.0% ilmenite. There is a relatively low content of approximately 15.5% glass phase in the CE-5 lunar sample. From the results, we deduce that the CE-5 LR structure could have mainly resulted from micrometeoroid impacts to achieve such a high level of maturity. © Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature 2021 |
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Insights regarding the effect of a new sampling geological site on the surficial lunar sample CE5C0400 were illustrated using nondestructive techniques such as laser diffractometry coupled with image analysis, X-ray computed tomography, and field emission scanning electron microscopy equipped with energy dispersive spectroscopy, and X-ray diffraction combined with Rietveld refinement. From the characterization analyses, the CE-5 sampling site in the northeastern Oceanus Procellarum on the Moon yields a unique collection of relatively regular-shaped and fine basalt-dominated particles. The median grain size D50 is (55.24±0.96) µm, falling within the relatively low end of the range of the Apollo lunar returned samples. The coefficient of uniformity Cu of 15.1 and the coefficient of curvature Cc of 1.7 could classify CE5C0400 to be well-graded. The minerals in CE5C0400 comprise approximately 44.5% pyroxene, 30.4% plagioclase, 3.6% olivine, and 6.0% ilmenite. There is a relatively low content of approximately 15.5% glass phase in the CE-5 lunar sample. From the results, we deduce that the CE-5 LR structure could have mainly resulted from micrometeoroid impacts to achieve such a high level of maturity.</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Zhang, Xian</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Zhang, Guang</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Dong, Keqi</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Deng, Xiangjin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Gao, Xiaosong</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Yang, Yaodong</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Xiao, Yuan</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Bai, Xiao</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Liang, Kaixin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Liu, Yiwei</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Ma, Wenbin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Zhao, Shaofan</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Zhang, Ce</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Zhang, Xiaojing</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Song, Jian</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Yao, Wei</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Chen, Hong</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Wang, Weihua</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Zou, Zhigang</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Yang, Mengfei</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Science in China</subfield><subfield code="d">Heidelberg : Springer, 2003</subfield><subfield code="g">65(2021), 2 vom: 10. 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