Diverse rock types detected in the lunar South Pole-Aitken Basin by the Chang'E-4 lunar mission

被引:30
|
作者
Huang, Jun [1 ,2 ]
Xiao, Zhiyong [2 ,3 ,4 ]
Xiao, Long [1 ,2 ,4 ]
Horgan, Briony [5 ]
Hu, Xiaoyi [1 ]
Lucey, Paul [6 ]
Xiao, Xiao [1 ]
Zhao, Siyuan [1 ]
Qian, Yuqi [1 ]
Zhang, Hao [1 ]
Li, Chunlai [7 ]
Xu, Rui [7 ]
He, Zhiping [7 ]
Yang, Jianfeng [8 ]
Xue, Bin [8 ]
He, Qi [1 ]
Zhong, Jie [9 ]
Lin, Hongyu [10 ]
Huang, Changning [10 ]
Xie, Jianfeng [11 ]
机构
[1] China Univ Geosci, Sch Earth Sci, Planetary Sci Inst, State Key Lab Geol Proc & Mineral Resources, Wuhan 430074, Hubei, Peoples R China
[2] Chinese Acad Sci, Ctr Excellence Comparat Planetol, Hefei 230026, Anhui, Peoples R China
[3] Sun Yat Sen Univ, Sch Atmospher Sci, Planetary Environm & Astrobiol Lab, Zhuhai 519000, Guangdong, Peoples R China
[4] Macau Univ Sci & Technol, Space Sci Inst, State Key Lab Lunar & Planetary Sci, Macau 999078, Peoples R China
[5] Purdue Univ, Dept Earth Atmospher & Planetary Sci, W Lafayette, IN 47907 USA
[6] Univ Hawaii Manoa, Hawaii Inst Geophys & Planetol, Honolulu, HI 96822 USA
[7] Chinese Acad Sci, Shanghai Inst Tech Phys, Key Lab Space Act Optoelect Technol, Shanghai 200083, Peoples R China
[8] Chinese Acad Sci, Xian Inst Opt & Precis Mech, Xian 710119, Peoples R China
[9] Chinese Acad Sci, Inst Opt & Elect, Chengdu 610209, Peoples R China
[10] China Acad Space Technol, Inst Space Mech & Elect, Beijing 100086, Peoples R China
[11] Beijing Aerosp Flight Control Ctr, Beijing 100094, Peoples R China
关键词
NEAR-INFRARED SPECTRA; MINERAL MIXTURES; LANDING SITE; SURFACE; DIFFERENTIATION; IDENTIFICATION; SPECTROSCOPY; PYROXENES; BANDS;
D O I
10.1130/G47280.1
中图分类号
P5 [地质学];
学科分类号
0709 ; 081803 ;
摘要
The South Pole-Aitken (SPA) basin, located between the South Pole and Aitken crater on the far side of the Moon, is the largest confirmed lunar impact structure. The pre-Nectarian SPA basin is a 2400 x 2050 km elliptical structure centered at 53 degrees S, 191 degrees E, which should have exposed lower crust and upper mantle due to the enormous excavation depth. Olivine, the dominant mineral in Earth's mantle, has only been identified in small and localized exposures in the margins of the SPA basin, and the dominant mafic component is, instead, pyroxene. These mineralogical characteristics could be explained by the recent hypothesis that the lunar upper mantle is dominated by low-calcium pyroxene, not olivine. Here, we present observations from imaging and spectral data from China's Chang'E-4 (CE-4) lunar mission in the first 4 synodic days, especially the first in situ visible/near-infrared spectrometer observations of an exposed boulder. We identified a variety of rock types, but not the recently reported olivine-rich materials in the landing region. The results are consistent with orbital observations. The obtained mineralogical information provides a better understanding of the nature and origin of SPA materials.
引用
收藏
页码:723 / 727
页数:5
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