Emplacement of shocked basement clasts during crater excavation in the Ries impact structure

IF 1.8 3区 地球科学 Q3 GEOSCIENCES, MULTIDISCIPLINARY International Journal of Earth Sciences Pub Date : 2024-04-19 DOI:10.1007/s00531-024-02403-z
Fabian Dellefant, Lina Seybold, Claudia A. Trepmann, Stuart A. Gilder, Iuliia V. Sleptsova, Stefan Hölzl, Melanie Kaliwoda
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Abstract

In the Aumühle quarry of the Ries impact structure, moderately shocked clasts from the Variscan basement occur sandwiched between overlying suevite and components derived from the Mesozoic sedimentary cover of the underlying Bunte Breccia without distinct shock effects. We analyzed the clasts by optical microscopy, scanning electron microscopy (SEM/EDS/EBSD), and Raman spectroscopy to unravel their emplacement relation to the overlying suevite and the sediment-rock clasts of the Bunte Breccia. Clasts sizes range up to few decimeters and are embedded in a fine-grained lithic matrix; no impact-melt fragments are observed. Amphibolite clasts contain maskelynite with few lamellar remnants of feldspar, indicating shock pressures of 28–34 GPa. Amphiboles have cleavage fractures and (\(\overline{1}\)01) mechanical twins suggesting differential stresses > 400 MPa. Felsic gneiss components have optically isotropic SiO2 indicative of shock pressures ≈35 GPa. Metagranite cataclasite clasts contain shocked calcite aggregates and quartz with a high density of fine rhombohedral planar deformation features indicating shock pressures ≈20 GPa. The moderately shocked basement clasts originate from deeper levels of the transient cavity and lower radial distance to the center of the structure compared to the sediment-rock clasts. Both were ballistically ejected during crater excavation. In accordance with palaeo- and rock magnetic data, they were mixed during turbulent deposition at the top of the Bunte Breccia before the emplacement of suevite. The high amount of basement clasts below suevite and on top of the underlying Bunte Breccia is consistent with the commonly reported inverse stratigraphy in the Ries impact structure.

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里斯撞击结构中陨石坑挖掘过程中冲击基底碎屑的置换
在里斯撞击构造的奥姆勒采石场,来自瓦利斯坎基底的中度冲击碎屑岩夹杂在上覆矽卡岩和来自下伏邦特角砾岩中生代沉积覆盖层的成分之间,没有明显的冲击效应。我们利用光学显微镜、扫描电子显微镜(SEM/EDS/EBSD)和拉曼光谱对这些碎屑进行了分析,以揭示它们与上覆闪长岩和本特角砾岩的沉积岩碎屑之间的置换关系。碎屑大小可达几分米,嵌入细粒岩石基质中;没有观察到撞击熔融碎片。闪长岩岩屑含有蒙长石和少量长石的片状残留物,表明冲击压力为 28-34 GPa。闪长岩具有劈裂断口和((overline{1}\)01)机械孪晶,表明存在400兆帕的差应力。长英片麻岩成分具有光学各向同性的二氧化硅,表明冲击压力≈35 GPa。玄武质白云母碎屑岩含有冲击方解石集合体和石英,具有高密度的细斜方体平面变形特征,表明冲击压力≈20 GPa。与沉积岩碎屑相比,中度休克基底碎屑来自瞬变腔体的较深层,与结构中心的径向距离较小。两者都是在陨石坑挖掘过程中被弹射出来的。根据古生物学和岩石磁性数据,它们是在布恩特角砾岩顶部的湍流沉积过程中混合在一起的,然后才被矽卡岩所取代。大量基底碎屑岩位于绥维岩之下和底层邦特角砾岩之上,这与通常报道的里斯撞击结构中的反地层学相一致。
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来源期刊
International Journal of Earth Sciences
International Journal of Earth Sciences 地学-地球科学综合
CiteScore
4.60
自引率
4.30%
发文量
120
审稿时长
4-8 weeks
期刊介绍: The International Journal of Earth Sciences publishes process-oriented original and review papers on the history of the earth, including - Dynamics of the lithosphere - Tectonics and volcanology - Sedimentology - Evolution of life - Marine and continental ecosystems - Global dynamics of physicochemical cycles - Mineral deposits and hydrocarbons - Surface processes.
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