玄武岩
地质学
火山作用
地球化学
地幔(地质学)
火山
锶
铷
撞击坑
月母马
地球科学
天体生物学
构造学
钾
古生物学
物理
化学
有机化学
核物理学
作者
Ze-Xian Cui,Qing Yang,Yanqiang Zhang,Chengyuan Wang,Haiyang Xian,Zhiming Chen,Zhiyong Xiao,Yuqi Qian,J. W. Head,C. R. Neal,Long Xiao,Fanglu Luo,Jingyou Chen,Peng‐Li He,Yonghua Cao,Qin Zhou,Fangfang Huang,Linli Chen,Bo Wei,Jintuan Wang
出处
期刊:Science
[American Association for the Advancement of Science]
日期:2024-11-15
卷期号:386 (6728): 1395-1399
被引量:12
标识
DOI:10.1126/science.adt1093
摘要
Remote sensing observations have shown that the far side of the Moon (lunar farside) has different geology and rock composition to those of the nearside, including the abundances of potassium, rare earth elements, and phosphorus (collectively known as KREEP). The Chang’e-6 (CE-6) spacecraft collected samples from the South Pole–Aitken (SPA) basin on the farside and brought them to Earth. We used lead-lead and rubidium-strontium isotope systems to date low-titanium basalt in a CE-6 sample, finding a consistent age of 2830 (±5) million years. We interpret this as the date of volcanism in SPA and incorporate it into lunar crater chronology. Strontium, neodymium, and lead isotopes indicate that the volcanic magma was from a lunar mantle source depleted in incompatible elements and containing almost no KREEP component.
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