奥地利阿尔卑斯山脉锡格拉本复合体的岩石学、锆英铅地质年代和地球化学:前阿尔卑斯山与阿尔卑斯山历史

IF 2.9 2区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Marián Putiš , Jiří Sláma , Qiu-Li Li , Ondrej Nemec , Martin Ondrejka , Xian-Hua Li , Friedrich Koller , Lukáš Ackerman , Ladislav Strnad , Peter Ružička
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引用次数: 0

摘要

奥地利东部的锡格拉本复合地层(Sieggraben Complex,SC)提供了奥地利阿尔卑斯山基底高/超高压带地壳和地幔地段前二叠纪、二叠纪和阿尔卑斯山(白垩纪)演化阶段的全面信息。锡格拉本-施瓦岑巴赫地区的地壳由三个自上而下的构造地层单元组成:(1) Paragneiss 单元;(2) 包含 MORB 和 OIB 类型岩浆岩的大理岩-斜长岩单元;(3) Micaschist-Calcschist 单元。N-MORB型岩浆岩的UPb年龄为369.7 ± 2.0 Ma,εNd(370) = +8.5 至 +7.4,TDM(2st) 为0.42-0.50 Ga;E-MORB型岩浆岩(UPb年龄约为400 Ma)的εNd(400) = +9.4至+5.6,TDM(2st)为0.37-0.67 Ga,两者都表明在推断的泥盆纪大洋盆地形成过程中,地幔源相当年轻。这些单元的岩石揭示了寒武纪、新生代和奥陶纪的锆石来源。辉绿岩和闪长岩的年龄分别为 285.8 ± 9.2 Ma 和 265.7 ± 2.1 Ma,而辉绿岩的年龄为 265.5 ± 1.4 Ma,这表明二叠纪的变质叠加十分重要。二叠纪花岗岩堤的年代在 265 至 260 Ma 之间,特别是 273 和 253 Ma,横切了岩性单元。与下伏地幔碎块的哈兹堡岩相交的一个挛辉石堤的岩浆年龄为 253.3 ± 2.9 Ma。总体而言,这些年龄表明二叠纪发生了强烈的延伸、过热以及地壳和地幔岩石的熔化。从 ∼100 Ma,但主要在 92 至 90 Ma 之间的斜长岩年龄可以确定白垩纪晚期的变质事件,该事件由 Paragneiss 单元中 88.4 ± 0.8 Ma 的伟晶岩侵入所终止。二叠纪和白垩纪变质事件往往导致相对较早的锆石年龄重置,同时锆石εHf(t)值下降,全岩 87Sr/86Sr 值上升。很少检测到石炭纪变质年龄为 ∼340 Ma。SC最终代表了晚白垩世早期大陆内部俯冲带的一部分,该俯冲带形成于泥盆纪和二叠纪延伸所造成的强烈减薄的结晶基底中。在新生代 AL-CA-PA(阿尔卑斯-喀尔巴阡山-潘诺尼亚)微板块的框架内,在西喀尔巴阡山内Gemeric和Veporic构造单元之间的Lubeník线附近,也描述了一个类似的白垩纪缝合带,该缝合带具有HP闪长岩,白云母ArAr年龄测定为130-100 Ma(100-90 Ma出露)。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Lithology, UPb zircon geochronology, and geochemistry of the Austroalpine Sieggraben Complex: Pre-Alpine vs. Alpine history

The Sieggraben Complex (SC) in Eastern Austria provides comprehensive information on the pre-Permian, Permian, and Alpine (Cretaceous) evolutional stages of the crustal and mantle sections included into the Austroalpine basement HP/UHP belt. The SC in the Sieggraben–Schwarzenbach area consists of three, top-to-bottom tectono-stratigraphic units: (1) the Paragneiss unit, (2) the Marble–Eclogite unit, which contains MORB and OIB types of mafic rocks, and (3) the Micaschist–Calcschist unit. The N-MORB type mafic rocks yield a UPb age of 369.7 ± 2.0 Ma, have εNd(370) = +8.5 to +7.4 and TDM(2st) of 0.42–0.50 Ga, while the E-MORB types (UPb ages around 400 Ma) show εNd(400) = +9.4 to +5.6 and TDM(2st) of 0.37–0.67 Ga, both indicating rather juvenile mantle sources during the formation of the inferred oceanic Devonian basin. The rocks of these units revealed Cambrian, Proterozoic, and Archean zircon sources. The ages of 285.8 ± 9.2 and 265.7 ± 2.1 Ma from eclogite and amphibolite, respectively, and 265.5 ± 1.4 Ma from paragneiss indicate an important Permian metamorphic overprint. Permian granitic dykes dated from ∼265 to 260 Ma, exceptionally at 273 and 253 Ma, crosscut the lithological units. A clinopyroxenite dyke, which crosscuts harzburgite of the underlying mantle fragment, yielded a magmatic age of 253.3 ± 2.9 Ma. Overall, these ages suggest a strong Permian extension, overheating, and melting of the crustal and mantle rocks. The eclogite ages from ∼100 Ma, but mainly between 92 and 90 Ma, constrain the Late Cretaceous metamorphic event terminated by an 88.4 ± 0.8 Ma pegmatite intrusion in the Paragneiss unit. The Permian and Cretaceous metamorphic events often caused resetting of the relatively older zircon ages, together with a decrease of zircon εHf(t) values, and an increase of whole-rock 87Sr/86Sr values. A Carboniferous metamorphic age of ∼340 Ma was rarely detected. The SC finally represents a part of an early Late Cretaceous intra-continental subduction zone, which formed within a strongly-thinned crystalline basement due to the Devonian and Permian extensions. A similar Cretaceous suture zone with HP amphibolite, dated at ∼130–100 Ma by white mica ArAr ages (100–90 Ma exhumation), has been described around the Lubeník line between the Gemeric and Veporic tectonic units of the Inner Western Carpathians in the framework of the Cenozoic AL–CA–PA (Alpine–Carpathian–Pannonian) microplate.

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来源期刊
Lithos
Lithos 地学-地球化学与地球物理
CiteScore
6.80
自引率
11.40%
发文量
286
审稿时长
3.5 months
期刊介绍: Lithos publishes original research papers on the petrology, geochemistry and petrogenesis of igneous and metamorphic rocks. Papers on mineralogy/mineral physics related to petrology and petrogenetic problems are also welcomed.
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