希克苏鲁伯冲击变形锆石元素重分布与年龄重置

IF 4.5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Jiawei Zhao , Long Xiao , Zhiyong Xiao , Xiang Wu , Qi He , Jialong Hao , Ruiying Li , Yangting Lin
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引用次数: 0

摘要

锆石已被用来记录地球和其他行星体的地质演化。在某些情况下,锆石中的U-Pb放射性同位素体系可以通过冲击变质作用(如高压相的形成和逆转、再结晶)被完全重置,抹去了初始结晶记录,而记录了冲击年龄。这些元素重分布伴随结构变化的行为为揭示冲击锆石的极端冲击过程提供了关键证据。然而,由于与冲击事件相关的变质过程复杂而漫长,各种冲击效应对冲击锆石内部元素再分布的贡献尚不清楚。本文采用高分辨率纳米二次离子质谱(NanoSIMS)技术分析了希克苏鲁伯撞击构造中的锆石颗粒,发现其具有平面/不规则断裂、锆石孪晶、reidite和锆石颗粒等微观结构特征,记录了与冲击变质作用和撞击后变质作用相关的三种主要元素重分配过程。一是在锆石—泥质岩边界处优先富集钇(Y),这与高压多晶泥质岩的形成密切相关,但在含泥质岩的锆石中保留了原生分带。第二个过程涉及与冲击相关的加热,导致含reidite的锆石固态转变为粒状锆石,并形成新形成的锆石颗粒。这一过程促进了放射性成因铅(Pb)的损失,并且由于不同元素的扩散特性,使得颗粒锆石中铀(U)的主要分区得以保留,从而为确定撞击事件的日期提供了机会。③Chicxulub撞击构造内的锆石颗粒在撞击后热液作用下发生了不同程度的蚀变,其中钇(Y)、钛(Ti)、铀(U)、铅(Pb)和磷(P)等元素的局部掺入使其发生了不同程度的蚀变。这可能是震波锆石颗粒发生局部年龄重置的另一种机制。特别是在希克苏鲁伯冲击构造中,震荡锆石经历了从雷氏岩形成到锆石颗粒生长,再到热液蚀变的序贯变质过程,揭示了其元素重分布的系统特征。这些发现为陆地撞击坑极端冲击和撞击后变质条件下锆石元素重分布和年龄重置的行为和机制提供了有效约束。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Element Redistribution and Age Resetting in Shock-Deformed Zircon from the Chicxulub Impact Structure
Zircon has been used to chronicle the geological evolution of the Earth and other planetary bodies. In some circumstances the U-Pb radioisotopic system in zircon can be completely reset by shock metamorphism (e.g. high-pressure phase formation and reversion, and recrystallization), erasing the initial crystallization record and instead recording the impact age. These behaviors of element redistribution accompanied with structure variation in shocked zircon provide pivotal evidence to unravel the extreme impact processes. However, the contributions from a variety of shock effects to element redistribution within shocked zircons are not clear due to the complicated and protracted metamorphic processes associated with an impact event. Here we use high-resolution Nano secondary ion mass spectrometry (NanoSIMS) to show that zircon grains from the Chicxulub impact structure that contain microstructural features such as planar/irregular fractures, zircon twins, reidite and zircon granules, record three main types of element redistribution processes related to shock metamorphism and post-impact modification. The first is the preferential yttrium (Y) enrichments at the zircon-reidite boundaries that is closely related to the formation of the high-pressure polymorph reidite, but the primary zoning is preserved in reidite-bearing zircon. The second process involves shock-related heating, resulting in the solid-state transformation from reidite-bearing zircon to granular zircon, and the growth of neo-formed zircon granules. This process facilitates the loss of radiogenic lead (Pb) and allows the retain of primary zoning of uranium (U) in granular zircon due to the different element diffusion properties, thus providing the chance to date the impact event. Thirdly, the studied zircon grains within the Chicxulub impact structure experienced post-impact hydrothermal alteration to varying degrees by localized element incorporation of additional yttrium (Y), titanium (Ti), uranium (U), lead (Pb) and phosphorus (P). The U-Pb systematics altered by post-impact hydrothermal processes reveal a generally discordant line affected by the external input of U and common Pb, which could be an alternative mechanism of localized age resetting happened in shocked zircon grains. Particularly, this study demonstrates the systematic characteristics of element redistribution in shocked zircons that experienced the sequential metamorphic processes from reidite formation to growth of zircon granules, and subsequent hydrothermal alteration within the Chicxulub impact structure. These findings provide the effective constraints for behaviors and mechanisms of element redistribution and age resetting in zircon under extreme shock and post-impact metamorphic conditions in terrestrial impact craters.
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来源期刊
Geochimica et Cosmochimica Acta
Geochimica et Cosmochimica Acta 地学-地球化学与地球物理
CiteScore
9.60
自引率
14.00%
发文量
437
审稿时长
6 months
期刊介绍: Geochimica et Cosmochimica Acta publishes research papers in a wide range of subjects in terrestrial geochemistry, meteoritics, and planetary geochemistry. The scope of the journal includes: 1). Physical chemistry of gases, aqueous solutions, glasses, and crystalline solids 2). Igneous and metamorphic petrology 3). Chemical processes in the atmosphere, hydrosphere, biosphere, and lithosphere of the Earth 4). Organic geochemistry 5). Isotope geochemistry 6). Meteoritics and meteorite impacts 7). Lunar science; and 8). Planetary geochemistry.
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