Petrogenesis of Chang'E-6 basalts and implication for multi-episode volcanism in the lunar farside basin

IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Dehan Shen , Shijie Li , Shaolin Li , Yingkui Xu , Yang Li , Mingbao Li , Deliang Wang , Ronghua Pang , Yuwei Zhang , Zhipeng Han
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Abstract

Mare basalts are products of lunar mantle via partial melting, and hence viewed as crucial probes of the mantle's composition and thermal state. While previous mission-returned lunar samples have provided valuable insights into the composition and structure of the lunar interior, our understanding remains limited because all samples have been collected from the lunar nearside. Consequently, numerous scientific questions about the Moon's dichotomy remain unresolved. In June 2024, China's Chang'E-6 (CE-6) mission successfully returned the first-ever samples from lunar farside, which marks a new era in lunar science. In this work, we examine the petrography, mineralogy, and geochemistry of CE-6 basaltic fragments. Our results reveal that the basaltic fragments at the CE-6 landing site exhibit variable chemical compositions, ranging from very low-Ti to low-Ti types. The diversity in the petrogenesis of these basaltic rocks demonstrates significant differences in the mantle source and subsequent magmatic processes. Combined with remote sensing data, these findings indicate a complex thermal evolution for the southern mare of the Apollo basin in the South Pole-Aitken (SPA) basin, which experienced at least three episodes of volcanism. Additionally, the broad variation in TiO2 content suggests the possibility of even more episodes of volcanism occurred and more types of basalts existed in this farside basin of the Moon. Furthermore, the multi-episodes magmatism occurred in the lunar farside basin, suggests that spatial variations in magma production rates across the Moon's interior may be negligible. The petrogenetic modeling of CE-6 basaltic fragments demonstrates that incompatible element concentrations and mineral modes are likely to be similar across lunar nearside to farside mantle. In contrast, the lunar crust appears to play a critical role in controlling basaltic magma eruptions on the farside surface.
嫦娥六号玄武岩成因及月后盆地多期火山作用意义
海玄武岩是月幔部分熔融的产物,因此被认为是探测月幔成分和热状态的重要工具。虽然以前的任务返回的月球样本提供了对月球内部组成和结构的宝贵见解,但我们的理解仍然有限,因为所有样本都是从月球的近端收集的。因此,关于月球两面性的许多科学问题仍未得到解决。2024年6月,中国的嫦娥六号(CE-6)任务成功地从月球背面带回了第一个样本,这标志着月球科学进入了一个新时代。在这项工作中,我们研究了CE-6玄武岩碎片的岩石学,矿物学和地球化学。我们的研究结果表明,CE-6着陆点的玄武岩碎片具有不同的化学成分,从极低钛到低钛类型不等。这些玄武岩岩石成因的多样性表明,其地幔源和后续岩浆作用存在显著差异。结合遥感数据,这些发现表明,南极-艾特肯(SPA)盆地的阿波罗盆地南部海经历了复杂的热演化,至少经历了三次火山活动。此外,TiO2含量的广泛变化表明,在月球背面盆地可能发生过更多的火山活动,存在更多类型的玄武岩。此外,多期岩浆活动发生在月球背面盆地,这表明月球内部岩浆产生率的空间变化可以忽略不计。CE-6玄武岩碎片的岩石成因模拟表明,月球近端和远端地幔中不相容的元素浓度和矿物模式可能相似。相比之下,月球地壳似乎在控制月球背面玄武岩岩浆喷发方面起着关键作用。
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来源期刊
Earth and Planetary Science Letters
Earth and Planetary Science Letters 地学-地球化学与地球物理
CiteScore
10.30
自引率
5.70%
发文量
475
审稿时长
2.8 months
期刊介绍: Earth and Planetary Science Letters (EPSL) is a leading journal for researchers across the entire Earth and planetary sciences community. It publishes concise, exciting, high-impact articles ("Letters") of broad interest. Its focus is on physical and chemical processes, the evolution and general properties of the Earth and planets - from their deep interiors to their atmospheres. EPSL also includes a Frontiers section, featuring invited high-profile synthesis articles by leading experts on timely topics to bring cutting-edge research to the wider community.
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