Su Bin, Chen Yi, Wang Zeling, Zhang Di, Chen Haojie, Gou Sheng, Yue Zongyu, Liu Yanhong, Yuan Jiangyan, Tang Guoqiang, Guo Shun, Li Qiuli, Lin Yang-Ting, Li Xian-Hua, Wu Fu-Yuan
State Key Laboratory of Lithospheric and Environmental Coevolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, China.
Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, China.
Natl Sci Rev. 2025 Mar 20;12(6):nwaf103. doi: 10.1093/nsr/nwaf103. eCollection 2025 Jun.
As the largest and oldest well-preserved impact structure on the Moon, the South Pole-Aitken (SPA) basin on the lunar farside is critical for understanding early solar system dynamics and lunar history, but accurately determining its age remains challenging. Crater-counting chronology and Apollo sample studies propose various SPA-forming ages, which require validation by sampling of the SPA basin. Here, we present the petrology, geochemistry and chronology of norite clasts from the SPA basin that were returned by Chang'e-6. These norites have highly anorthite-rich, rare-earth element-poor plagioclase and magnesium-rich pyroxene, in contrast to Mg-suite norites that were returned from the lunar nearside. Abundant Fe-Ni metals with meteoritic Ni/Co ratios, depletion of volatile elements and variable grain sizes and cooling rates strongly indicate that the norites were crystallized from an impact melt sheet. Precise Pb-Pb ages of zirconium-bearing minerals in the norites yield two distinct impact events at 3.87 and 4.25 Ga. The former represents an impact-resetting event within the basin. The latter finding is most consistent with the age of the SPA impact, providing an initial 4.25-Ga anchor for the older end of the lunar crater chronology and refining the timeline for early lunar evolution.
作为月球上最大、最古老且保存完好的撞击构造,月球背面的南极-艾特肯(SPA)盆地对于理解早期太阳系动力学和月球历史至关重要,但准确确定其年龄仍然具有挑战性。撞击坑计数年代学和阿波罗样本研究提出了各种SPA形成年龄,这需要通过对SPA盆地进行采样来验证。在这里,我们展示了由嫦娥六号带回的SPA盆地苏长岩碎屑的岩石学、地球化学和年代学。这些苏长岩具有高度富钙长石、稀土元素贫乏的斜长石和富镁辉石,这与从月球近侧带回的镁质苏长岩不同。具有陨石镍钴比的大量铁镍金属、挥发性元素的亏损以及可变的晶粒尺寸和冷却速率强烈表明,这些苏长岩是从撞击熔岩层结晶形成的。苏长岩中含锆矿物的精确铅铅年龄产生了3.87和4.25 Ga的两个不同撞击事件。前者代表盆地内的撞击重置事件。后一发现与SPA撞击的年龄最为一致,为月球撞击坑年代学的较老端提供了一个初始的4.25 Ga锚定,并完善了早期月球演化的时间线。