自然杂志 ›› 2026, Vol. 48 ›› Issue (4): 247-256.doi: 10.3969/j.issn.0253-9608.2026.04.001

• 特约专稿 •    下一篇

嫦娥六号样品解密月球背面演化历史

杨蔚   

  1. 中国科学院地质与地球物理研究所 行星科学与前沿技术重点实验室,北京 100029
  • 收稿日期:2026-06-28 出版日期:2026-08-25 发布日期:2026-08-14

Chang’e-6 samples unveil the evolutionary history of the Moon’s farside

YANG Wei   

  1. Key Laboratory of Planetary Science and Frontier Technology, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, China
  • Received:2026-06-28 Online:2026-08-25 Published:2026-08-14

摘要: 嫦娥六号首次实现月球背面采样返回,成为人类月球探测的里程碑。它着陆在月球三大地体之一的南极-艾特肯盆地,所采集的月壤样品使我们有机会一窥月球背面的演化历史。在嫦娥六号月壤中发现一种新的岩石类型——撞击熔岩。年代学研究指示,南极-艾特肯撞击可能形成于42.5亿年前,为内太阳系早期撞击历史提供了关键锚点。嫦娥六号月壤中也包含多种类型的玄武岩,如喷发于42亿年前的高铝玄武岩、喷发于29亿年前的极低钛玄武岩和喷发于28亿年前的低钛玄武岩,指示月球背面火山活动至少持续了14亿年。玄武岩化学组成研究显示,南极-艾特肯盆地下覆月幔具有“超亏损”“超贫水”“超还原”“重K同位素”的特征,与正面月幔显著不同,指示该月幔经历了大型撞击导致的熔体抽取和去气作用。古磁场强度研究显示,月球磁场强度在约28亿年前曾出现反弹。综合这些研究结果,初步揭开月球背面42.5亿至28亿年前的演化历史,并进一步支持南极-艾特肯撞击对月球二分性形成的重要贡献。

关键词: 嫦娥六号, 月壤, 南极-艾特肯盆地, 大型撞击, 火山活动, 玄武岩, 撞击熔岩

Abstract: The Chang’e-6 mission has successfully returned samples from the farside of the Moon for the first time, marking a significant milestone in the realm of human lunar exploration. The Chang’e-6 mission successfully landed in the South Pole-Aitken (SPA) basin, one of the Moon’s three major geological terranes. Analysis of the lunar soil samples collected by Chang’e-6 provides valuable insights into the evolutionary history of the Moon’s farside. A new type of rock, designated as impact melt rock, was discovered in the Chang’e-6 soil. Chronological studies on the impact melt rock indicate that the SPA impact may have occurred 4.25 billion years ago, providing a key anchor point for the early impact history of the inner Solar System. The Chang’e-6 soil also contains various types of basalt, including high-alumina basalt erupted 4.2 billion years ago, very-low-titanium basalt erupted 2.9 billion years ago, and low-titanium basalt erupted 2.8 billion years ago. These findings indicate that volcanic activity on the farside lasted for at least 1.4 billion years. The geochemical compositions of the low-titanium basalts indicate that the lunar mantle underlying the SPA basin exhibits characteristics of “ultra-depleted”, “more drier”, “more reduced” and “heavier potassium isotope”, which differ significantly from those observed on the nearside mantle. This finding suggests that the mantle beneath the SPA basin has undergone processes of melt extraction and degassing, likely induced by the SPA impact. Paleomagnetic studies have indicated that the palaeointensities of the Moon rebounded approximately 2.8 billion years ago. When considered as a whole, these findings provide the first insights into the evolutionary history of the Moon’s farside and further support the significant contribution of the SPA impact to the formation of the Moon’s asymmetry.