Shock deformation and U-Pb isotope systematics in zircon from impactites of the Rochechouart impact structure: Impact age and zircon provenance

IF 4.5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Daniela Guerrero, Wolf Uwe Reimold, Natalia Hauser, Gavin Kenny, Martin Whitehouse, Philippe Lambert
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引用次数: 0

Abstract

The >23 km diameter, ∼207 Ma old Rochechouart impact structure is located in the NW part of the Paleozoic basement of the French Massif Central. Despite significant erosion, this impact structure preserves a heterogeneous suite of impactites, and the transition between the crater floor and the basement. Recent textural and geochronologic studies of U-Pb on zircon from impactites and basement lithologies of this structure have shown a wide variety of shock deformation textures and age distributions. In this study, we present a comprehensive analysis combining detailed textural characterization (CL, BSE, EBSD) and U-Pb geochronological analyses at different spatial resolutions (SIMS and LA-ICP-MS) of zircon from two melt-bearing breccias (suevites) from Chassenon and Videix, and one impact melt rock (IMR) from Babaudus. The analyzed crystals display a variety of shock deformation textures. Identification of FRIGN zircon and grains with high proportions of reidite in the Videix suevite indicates that these types of shock deformation are more widespread than previously reported. In the Chassenon suevite, U-Pb age resetting increases with shock intensity, whereas in the Videix suevite, higher U and/or Th contents also appear to control resetting. In the Babaudus IMR, the similar ages for shocked granular zircons and some unshocked grains suggest that additional factors, beyond shock deformation and zircon composition, influence age resetting. The SIMS analyses yielded more reliable results after common Pb correction. The best estimate of the impact age obtained from this study is 203 ± 4 Ma (2σ, MSWD = 3.4, probability = 0.065) for SIMS analyses of two granular grains from the Babaudus IMR and one granular crystal from the Videix suevite. Zircons with younger (191 ± 4 Ma, post-impact) ages show similar characteristics to those close to the widely accepted age for the impact at 207 Ma, highlighting the challenge of distinguishing between grains and separating ages related to the impact from possible post-impact events (e.g., hydrothermal alteration). Finally, the geochronological results for the Videix and the Chassenon suevites show a clear correlation with provenance results for granitic and gneissic target lithologies, respectively. In contrast, the Babaudus IMR has an age distribution comparable with other impact melt rocks from Montoume and Recoudert but cannot be related to an identified target lithology.
Rochechouart冲击构造冲击物中锆石的冲击变形和U-Pb同位素系统:冲击年龄和锆石物源
直径23 km, ~ 207 Ma的Rochechouart撞击构造位于法国中部地块古生代基底的西北部分。尽管有明显的侵蚀,这个撞击结构保留了一套不均匀的撞击物,以及陨石坑底部和地下室之间的过渡。近年来对该构造的冲击岩和基底岩性锆石中U-Pb的结构和年代学研究表明,该构造具有多种冲击变形结构和年龄分布。在本研究中,我们对来自Chassenon和Videix的两个含熔体角砾岩(suevites)和来自Babaudus的一个冲击熔融岩(IMR)的锆石进行了详细的结构表征(CL, BSE, EBSD)和不同空间分辨率(SIMS和LA-ICP-MS)的U-Pb年代分析。所分析的晶体显示出多种激波变形织构。在Videix suvite中鉴定出FRIGN锆石和高比例reidite颗粒,表明这些类型的冲击变形比以前报道的更为广泛。在Chassenon suevite中,U- pb年龄重置随着冲击强度的增加而增加,而在Videix suevite中,较高的U和/或Th含量也似乎控制了重置。在Babaudus IMR中,受冲击的颗粒锆石和一些未受冲击的颗粒锆石年龄相近,这表明除了冲击变形和锆石成分外,还有其他因素影响了年龄重置。SIMS分析在常规Pb校正后得到了更可靠的结果。对Babaudus IMR的两个颗粒和Videix suevite的一个颗粒晶体进行SIMS分析,得到的撞击年龄的最佳估计为203±4 Ma (2σ, MSWD = 3.4,概率= 0.065)。较年轻(191±4 Ma,撞击后)年龄的锆石显示出与接近被广泛接受的撞击年龄(207 Ma)的锆石相似的特征,这突出了区分颗粒和将与撞击有关的年龄与可能的撞击后事件(如热液蚀变)分开的挑战。最后,Videix和Chassenon花岗岩的年代学结果分别与花岗岩和片麻岩目标岩性的物源结果具有明显的相关性。相比之下,Babaudus IMR的年龄分布与来自Montoume和redert的其他撞击熔融岩相当,但与已确定的目标岩性无关。
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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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