The Moon's farside shallow subsurface structure unveiled by Chang'E-4 Lunar Penetrating Radar

被引:160
作者
Li, Chunlai [1 ,2 ]
Su, Yan [1 ,2 ]
Pettinelli, Elena [3 ]
Xing, Shuguo [1 ]
Ding, Chunyu [4 ]
Liu, Jianjun [1 ,2 ]
Ren, Xin [1 ]
Lauro, Sebastian E. [3 ]
Soldovieri, Francesco [5 ]
Zeng, Xingguo [1 ]
Gao, Xingye [1 ]
Chen, Wangli [1 ]
Dai, Shun [1 ]
Liu, Dawei [1 ]
Zhang, Guangliang [1 ]
Zuo, Wei [1 ,2 ]
Wen, Weibin [1 ]
Zhang, Zhoubin [1 ]
Zhang, Xiaoxia [1 ]
Zhang, Hongbo [1 ]
机构
[1] Chinese Acad Sci, Natl Astron Observ, Key Lab Lunar & Deep Space Explorat, Beijing 100101, Peoples R China
[2] Univ Chinese Acad Sci, Beijing 100049, Peoples R China
[3] Roma Tre Univ, Math & Phys Dept, I-00146 Rome, Italy
[4] Sun Yat Sen Univ, Sch Atmospher Sci, Zhuhai 519000, Peoples R China
[5] CNR, IREA, I-80124 Naples, Italy
基金
中国国家自然科学基金;
关键词
ALGORITHMS; MIGRATION; CRATER; MARIA; BASIN;
D O I
10.1126/sciadv.aay6898
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
On 3 January 2019, China's Chang'E-4 (CE-4) successfully landed on the eastern floor of Von karman crater within the South Pole-Aitken Basin, becoming the first spacecraft in history to land on the Moon's farside. Here, we report the observations made by the Lunar Penetrating Radar (LPR) onboard the Yutu-2 rover during the first two lunar days. We found a signal penetration at the CE-4 landing site that is much greater than that at the CE-3 site. The CE-4 LPR images provide clear information about the structure of the subsurface, which is primarily made of low-loss, highly porous, granular materials with embedded boulders of different sizes; the images also indicate that the top of the mare basal layer should be deeper than 40 m. These results represent the first high-resolution image of a lunar ejecta sequence ever produced and the first direct measurement of its thickness and internal architecture.
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页数:8
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