A young multilayered terrane of the northern Mare Imbrium revealed by Chang’E-3 mission

Author:

Xiao Long12,Zhu Peimin1,Fang Guangyou3,Xiao Zhiyong14,Zou Yongliao5,Zhao Jiannan1,Zhao Na1,Yuan Yuefeng1,Qiao Le1,Zhang Xiaoping2,Zhang Hao1,Wang Jiang1,Huang Jun1,Huang Qian1,He Qi1,Zhou Bin3,Ji Yicai3,Zhang Qunying3,Shen Shaoxiang3,Li Yuxi3,Gao Yunze3

Affiliation:

1. China University of Geosciences, Wuhan 430074, China.

2. Macau University of Science and Technology, Macau, China.

3. Institute of Electronics, China Academy of Science, Beijing 100190, China.

4. The Centre for Earth Evolution and Dynamics, University of Oslo, Sem Sælandsvei 24, 0371 Oslo, Norway.

5. National Astronomical Observatories, China Academy of Science, Beijing 100012 China.

Abstract

Onsite radar shows what lies beneath In more active periods of the Moon's history, volcanic eruptions created lava plains that formed layers of dark basalt. Without subsurface probing, we can only examine the most recent flows. After the soft landing of the Chang'E-3 spacecraft, Xiao et al. made penetrating radar measurements of the lunar crust with the Yutu rover. Several subsurface layers suggest multiple geologic processes at play throughout the crustal history, including multiple lava flows and the weathering-induced creation of dust and rocky debris. Science , this issue p. 1226

Funder

Natural Science Foundation of China

Chinese Academy of Sciences

Science and Technology Development Fund (FDCT) of Macau

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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