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Volcanic history of the Imbrium basin: A close-up view from the lunar rover Yutu
文献类型：期刊论文
| 作者 | Zhang, Jinhai; Yang, Wei; Hu, Sen; Lin, Yangting; Fang, Guangyou; Li, Chunlai; Peng, Wenxi; Zhu, Sanyuan; He, Zhiping; Zhou, Bin |
| 刊名 | PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA
 |
| 出版日期 | 2015 |
| 卷号 | 112期号:17页码:5342-5347 |
| ISSN号 | 0027-8424 |
| 中文摘要 | We report the surface exploration by the lunar rover Yutu that landed on the young lava flow in the northeastern part of the Mare Imbrium, which is the largest basin on the nearside of the Moon and is filled with several basalt units estimated to date from 3.5 to 2.0 Ga. The onboard lunar penetrating radar conducted a 114-m-long profile, which measured a thickness of similar to 5 m of the lunar regolith layer and detected three underlying basalt units at depths of 195, 215, and 345 m. The radar measurements suggest underestimation of the global lunar regolith thickness by other methods and reveal a vast volume of the last volcano eruption. The in situ spectral reflectance and elemental analysis of the lunar soil at the landing site suggest that the young basalt could be derived from an ilmenite-rich mantle reservoir and then assimilated by 10-20% of the last residual melt of the lunar magma ocean. |
| 英文摘要 | We report the surface exploration by the lunar rover Yutu that landed on the young lava flow in the northeastern part of the Mare Imbrium, which is the largest basin on the nearside of the Moon and is filled with several basalt units estimated to date from 3.5 to 2.0 Ga. The onboard lunar penetrating radar conducted a 114-m-long profile, which measured a thickness of similar to 5 m of the lunar regolith layer and detected three underlying basalt units at depths of 195, 215, and 345 m. The radar measurements suggest underestimation of the global lunar regolith thickness by other methods and reveal a vast volume of the last volcano eruption. The in situ spectral reflectance and elemental analysis of the lunar soil at the landing site suggest that the young basalt could be derived from an ilmenite-rich mantle reservoir and then assimilated by 10-20% of the last residual melt of the lunar magma ocean. |
| 学科主题 | MARE BASALTS; CLEMENTINE UVVIS; RADAR SOUNDER; REGOLITH; LAYER; MOON; PROSPECTOR; NEARSIDE; DEPTH |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000353554000041 |
| 源URL | [http://ir.ioe.ac.cn/handle/181551/5139]  |
| 专题 | 光电技术研究所_光电传感技术研究室（六室） |
| 推荐引用方式 GB/T 7714 | Zhang, Jinhai,Yang, Wei,Hu, Sen,et al. Volcanic history of the Imbrium basin: A close-up view from the lunar rover Yutu[J]. PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA,2015,112(17):5342-5347. |
| APA | Zhang, Jinhai.,Yang, Wei.,Hu, Sen.,Lin, Yangting.,Fang, Guangyou.,...&Ouyang, Ziyuan.(2015).Volcanic history of the Imbrium basin: A close-up view from the lunar rover Yutu.PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA,112(17),5342-5347. |
| MLA | Zhang, Jinhai,et al."Volcanic history of the Imbrium basin: A close-up view from the lunar rover Yutu".PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA 112.17(2015):5342-5347. |
入库方式： OAI收割
来源：光电技术研究所
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