利用锆石U-Pb-Hf同位素资料揭示伊斯坦堡带(远东阿瓦洛尼亚)早期地质历史

IF 3.2 2区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY
Sinan Yılmazer , Gültekin Topuz , Marcel Guillong , Aral I. Okay , İnal Demirkaya , Fulya Uzun
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引用次数: 0

摘要

伊斯坦布尔带位于阿瓦洛尼亚的远东,是在一个由大洋弧和大陆域组成的晚新元古代复合基底上形成的。基底上覆寒武纪至中奥陶世碎屑沉积岩,不整合。从角闪岩相大陆变质岩和洋弧不整合上覆碎屑岩中提取的锆石U-Pb-Hf同位素新分析阐明了洋弧最早的地质历史,并细化了洋弧与大陆碰撞的时间线。大陆变质岩可划分为两个明显的角闪岩相域:(i)上部角闪岩相域,其变质峰值为568±10 Ma (2σ); (ii)下部角闪岩相域,其变质峰值为591±6 Ma (2σ)。角闪岩相变质碎屑岩中的锆石颗粒主要表现为早新元古代至古元古代(0.9 ~ 2.1 Ga),初始εHf值以正为主,并伴有晚新元古代变质过度生长。它们的原岩可能沉积于东世的陆内裂谷环境中。寒武系上段至奥陶系下段砂岩碎屑锆石年龄分布以601 ~ 608 Ma为主,701 ~ 710 Ma和1500 ~ 1501 Ma为次峰。晚新元古代锆石主要表现为负初始εHf值(~ 78%),表明幔源岩浆中有明显的地壳物质参与。因此,洋弧上寒武纪上端至奥陶纪下端砂岩的碎屑物来源主要是邻近的晚新元古代大陆岩浆弧,中、古元古代基底的输入可以忽略。将碎屑锆石数据与先前发表的其他远东阿瓦洛尼亚地体的数据进行比较分析,发现了显著的相似性。(2)上埃迪卡拉统和上寒武系-奥陶系碎屑岩的主要锆石年龄峰在589-608 Ma,小锆石年龄峰在701-738 Ma, (3) 575-615 Ma和695-715 Ma的火成岩的存在,与伊斯坦布尔带上寒武系和中奥陶系碎屑岩的碎屑锆石年龄峰相对应,尽管这些岩石尚未被记录。因此,远东部的阿瓦洛尼亚地体是统一的新元古代地壳域的一部分,可能从未被大洋分开。结合已公布的波罗的海上新元古代至寒武系碎屑锆石U-Pb年龄,支持远东阿瓦洛尼亚地体与波罗的海的物源联系,表明伊斯坦布尔带在新元古代晚期至早寒武世期间被增生到波罗的海。随后的碰撞后隆起和侵蚀很可能在寒武纪晚期移除了弧的上地壳部分。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Revealing the early geological history of the Istanbul Zone (Far-East Avalonia) through zircon U-Pb-Hf isotopic data
The Istanbul Zone, located in the far-eastern part of Avalonia, is built over a composite late Neoproterozoic basement consisting of an oceanic arc and a continental domain. This basement is unconformably overlain by uppermost Cambrian to Middle Ordovician clastic sedimentary rocks. New U-Pb-Hf isotopic analyses of zircons extracted from amphibolite-facies continental metamorphic rocks and the unconformably overlying clastic rocks on the oceanic arc elucidate the earliest geological history and refine the timeline for the collision between the oceanic arc and the continent. The continental metamorphic rocks are subdivided into two distinct amphibolite-facies domains: (i) an upper amphibolite-facies domain with peak metamorphism at 568 ± 10 Ma (2σ), and (ii) a lower amphibolite-facies domain with peak metamorphism at 591 ± 6 Ma (2σ). The zircon grains in the amphibolite-facies metaclastic rocks display mainly early Neoproterozoic to Paleoproterozoic ages (0.9–2.1 Ga) with predominantly positive initial εHf values, apart from late Neoproterozoic metamorphic overgrowths. Their protoliths were likely deposited in an intracontinental rift setting during the Tonian. In contrast, the uppermost Cambrian to lowermost Ordovician sandstones reveal detrital zircon age distributions with major peaks at 601–608 Ma and minor peaks at 701–710 Ma and 1500–1501 Ma. The late Neoproterozoic zircons predominantly demonstrate negative initial εHf values (∼78 %), indicating significant involvement of crustal material in the mantle-derived magmas. Thus, the provenance of the detritus for the uppermost Cambrian to lowermost Ordovician sandstones on the oceanic arc is mainly a neighboring late Neoproterozoic continental magmatic arc with negligible input from the Meso- and Paleoproterozoic basement. A comparative analysis of the detrital zircon data with previously published data from other far-eastern Avalonian terranes reveals notable similarities. These include (i) the occurrence of metaclastic rocks with Tonian maximum deposition ages, (ii) major zircon age peaks at 589–608 Ma and minor peaks at 701–738 Ma in upper Ediacaran and uppermost Cambrian–Ordovician clastic rocks, and (iii) the occurrence of 575–615 Ma and 695–715 Ma igneous rocks that correspond to the detrital zircon age peaks in the uppermost Cambrian and Middle Ordovician clastic rocks of the Istanbul Zone, although such rocks have not yet been documented. Thus, the far-eastern Avalonian terranes were part of a unified Neoproterozoic crustal domain and were likely never separated by a large ocean. Integration of these data with published detrital zircon U–Pb ages from upper Neoproterozoic to Cambrian clastic successions in Baltica supports a provenance linkage between far-eastern Avalonian terranes and Baltica, indicating that the Istanbul Zone was accreted to Baltica during the late Neoproterozoic to early Cambrian. Subsequent post-collisional uplift and erosion likely removed the upper crustal portion of the arc by the latest Cambrian.
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来源期刊
Precambrian Research
Precambrian Research 地学-地球科学综合
CiteScore
7.20
自引率
28.90%
发文量
325
审稿时长
12 months
期刊介绍: Precambrian Research publishes studies on all aspects of the early stages of the composition, structure and evolution of the Earth and its planetary neighbours. With a focus on process-oriented and comparative studies, it covers, but is not restricted to, subjects such as: (1) Chemical, biological, biochemical and cosmochemical evolution; the origin of life; the evolution of the oceans and atmosphere; the early fossil record; palaeobiology; (2) Geochronology and isotope and elemental geochemistry; (3) Precambrian mineral deposits; (4) Geophysical aspects of the early Earth and Precambrian terrains; (5) Nature, formation and evolution of the Precambrian lithosphere and mantle including magmatic, depositional, metamorphic and tectonic processes. In addition, the editors particularly welcome integrated process-oriented studies that involve a combination of the above fields and comparative studies that demonstrate the effect of Precambrian evolution on Phanerozoic earth system processes. Regional and localised studies of Precambrian phenomena are considered appropriate only when the detail and quality allow illustration of a wider process, or when significant gaps in basic knowledge of a particular area can be filled.
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