Age and composition of young basalts on the Moon, measured from samples returned by Chang'e-5

被引:245
作者
Che, Xiaochao [1 ]
Nemchin, Alexander [1 ,2 ]
Liu, Dunyi [1 ,3 ]
Long, Tao [1 ]
Wang, Chen [1 ]
Norman, Marc D. [4 ]
Joy, Katherine H. [5 ]
Tartese, Romain [5 ]
Head, James [6 ]
Jolliff, Bradley [7 ,8 ]
Snape, Joshua F. [5 ]
Neal, Clive R. [9 ]
Whitehouse, Martin J. [10 ]
Crow, Carolyn [11 ]
Benedix, Gretchen [2 ,12 ]
Jourdan, Fred [2 ]
Yang, Zhiqing [1 ]
Yang, Chun [1 ]
Liu, Jianhui [1 ]
Xie, Shiwen [1 ]
Bao, Zemin [1 ]
Fan, Runlong [1 ]
Li, Dapeng [3 ]
Li, Zengsheng [3 ]
Webb, Stuart G. [9 ]
机构
[1] Chinese Acad Geol Sci, Beijing SHRIMP Ctr, Inst Geol, Beijing 100037, Peoples R China
[2] Curtin Univ, Sch Earth & Planetary Sci, Perth, WA 6845, Australia
[3] Shandong Inst Geol Sci, Jinan 250013, Shandong, Peoples R China
[4] Australian Natl Univ, Res Sch Earth Sci, Canberra, ACT 2601, Australia
[5] Univ Manchester, Dept Earth & Environm Sci, Manchester M13 9PL, Lancs, England
[6] Brown Univ, Dept Earth Environm & Planetary Sci, Providence, RI 02912 USA
[7] Washington Univ, Dept Earth & Planetary Sci, St Louis, MO 63130 USA
[8] Washington Univ, McDonnell Ctr Space Sci, St Louis, MO 63130 USA
[9] Univ Notre Dame, Dept Civil & Environm Engn & Earth Sci, Notre Dame, IN 46556 USA
[10] Swedish Museum Nat Hist, Dept Geosci, SE-10405 Stockholm, Sweden
[11] Univ Colorado, Dept Geol Sci, Boulder, CO 80309 USA
[12] Planetary Sci Inst, Tucson, AZ 85719 USA
基金
国家重点研发计划; 英国科学技术设施理事会;
关键词
MARE BASALTS; LUNAR; HISTORY; BHVO-2G; BCR-2G; REGION; BIR-1G; CRUST;
D O I
10.1126/science.abl7957
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
Orbital data indicate that the youngest volcanic units on the Moon are basalt lavas in Oceanus Procellarum, a region with high levels of the heat-producing elements potassium, thorium, and uranium. The Chang'e-5 mission collected samples of these young lunar basalts and returned them to Earth for laboratory analysis. We measure an age of 1963 +/- 57 million years for these lavas and determine their chemical and mineralogical compositions. This age constrains the lunar impact chronology of the inner Solar System and the thermal evolution of the Moon. There is no evidence for high concentrations of heat-producing elements in the deep mantle of the Moon that generated these lavas, so alternate explanations are required for the longevity of lunar magmatism.
引用
收藏
页码:887 / +
页数:37
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