嫦娥五号月球玄武岩中具有两种形态的巴德雷石的岩相学、晶体学和地质年代学

IF 3.9 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Liying Huang, Yuchen Xu, Lang Qin, Yang Liu, Lixin Gu, Heng-Ci Tian, Jialong Hao, Feng Zhang, Wei Du, Jing Yang, Hejiu Hui, Wei Yang, Yangting Lin, Yongliao Zou
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引用次数: 0

摘要

巴德来特(ZrO2)广泛存在于月球玄武岩中,经常被用于岩浆和撞击事件的铀-铅地质年代。巴德雷石的形成主要涉及两种机制:(a)晚期岩浆的结晶;(b)锆石在高温(高T)条件下的分解。具有不同形成机制的巴德磊石通常表现出不同的形态。在嫦娥五号月球玄武岩中,我们报告了具有两种不同形态的巴德来特,分别称为 "单一型 "和 "集合型"。我们对这两种类型的巴德雷石进行了岩相学和晶体学分析,以了解它们的形成条件和演化过程。尽管集合型巴德来特与锆石分解产物在形态和矿物组合上相似,但岩石学特征和锆石在月球玄武岩中的稀有性倾向于表明这两种类型的巴德来特都来自岩浆结晶。在这两种类型中观察到的晶体学关系表明,前体四方-ZrO2/立方-ZrO2 或正长方-ZrO2 相发生了相变。这些微结构的形成有两种可能的情况:(a) 从岩浆中直接结晶出高对称性 ZrO2;(b) 从岩浆中结晶出巴德来特,然后通过高压(high-P)事件导致其相变。然而,由于这两种假设中的科学问题尚未解决,目前无法确定准确的演化过程。因此,有必要进行广泛的热力学实验,以加深我们对作为 P-T 过程指标的巴德利石微结构的了解,从而深入了解岩浆活动和行星体的撞击历史。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Petrography, Crystallography, and Geochronology of Baddeleyite With Two Morphologies in a Chang'e-5 Lunar Basalt

Petrography, Crystallography, and Geochronology of Baddeleyite With Two Morphologies in a Chang'e-5 Lunar Basalt

Baddeleyite (ZrO2) is widespread in lunar basalts and frequently used for U-Pb geochronology of magmatic and impact events. The formation of baddeleyite involves two primary mechanisms: (a) crystallization from late-stage magma, and (b) decomposition of zircon under high-temperature (high-T) conditions. Baddeleyite with distinct formation mechanisms commonly displays different morphologies. In a Chang'e-5 lunar basalt, we report baddeleyite with two different morphologies, termed “singular type” and “aggregate type.” Petrographic and crystallographic analyses were conducted on both types of baddeleyite to understand their formation conditions and evolution processes. Despite the similarity in the morphology and mineral assemblages between the aggregate type baddeleyite and zircon decomposition products, the petrographic characteristics and the rarity of zircon in lunar basalts tend to suggest that both types of baddeleyite are derived from magma crystallization. Crystallographic relationships observed in both types indicate a phase transformation from the precursor tetragonal-ZrO2/cubic-ZrO2 or orthorhombic-ZrO2 phase. Two potential scenarios are proposed for the formation of these microstructures: (a) direct crystallization of high symmetry ZrO2 from magma, and (b) crystallization of baddeleyite from magma followed by a high-pressure (high-P) event causing its phase transition. However, due to unresolved scientific issues in both scenarios, an accurate evolutionary process cannot currently be determined. Therefore, extensive thermodynamic experiments are necessary to enhance our understanding of baddeleyite microstructures as indicators of P-T processes, providing insights into magmatism and the impact history of planetary bodies.

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来源期刊
Journal of Geophysical Research: Planets
Journal of Geophysical Research: Planets Earth and Planetary Sciences-Earth and Planetary Sciences (miscellaneous)
CiteScore
8.00
自引率
27.10%
发文量
254
期刊介绍: The Journal of Geophysical Research Planets is dedicated to the publication of new and original research in the broad field of planetary science. Manuscripts concerning planetary geology, geophysics, geochemistry, atmospheres, and dynamics are appropriate for the journal when they increase knowledge about the processes that affect Solar System objects. Manuscripts concerning other planetary systems, exoplanets or Earth are welcome when presented in a comparative planetology perspective. Studies in the field of astrobiology will be considered when they have immediate consequences for the interpretation of planetary data. JGR: Planets does not publish manuscripts that deal with future missions and instrumentation, nor those that are primarily of an engineering interest. Instrument, calibration or data processing papers may be appropriate for the journal, but only when accompanied by scientific analysis and interpretation that increases understanding of the studied object. A manuscript that describes a new method or technique would be acceptable for JGR: Planets if it contained new and relevant scientific results obtained using the method. Review articles are generally not appropriate for JGR: Planets, but they may be considered if they form an integral part of a special issue.
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