甘肃西北伊特兰卡地块寒武系—奥陶系岩浆活动地球化学及年代学证据

IF 2.6 3区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Sabah Yılmaz Şahin , Özge Naycı , Namık Aysal , Zeynep Cansu , Fatma Şişman Tükel
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引用次数: 0

摘要

不同时代的深成岩被剥离出来,形成伊斯特兰卡地块的基底岩。位于基底的寒武-奥陶系维泽岩体(Vize-Kırklareli)在某些特征上与其他岩体有所区别。该岩体侵入高变质沉积岩中,由三叠系低变质岩和始新世古珊瑚礁灰岩(Soğucak组)不整合覆盖。根据新的全岩地球化学和两个不同时代的锆石UPb资料,可以认为威泽岩体受到了长期岩浆活动的影响。维泽岩体的火成岩矿物和结构部分保存下来,具有糜棱岩结构,有明显的明暗区叶理。此外,变质花岗岩在某些地方还含有镁质岩浆包体。威泽岩体是一个以过铝质为主,微含铝质的i型岩体。它也是高钾、钙碱性的,反映了火山弧和碰撞后的构造环境。矿物化学分析表明,威泽岩体中的基性矿物主要由铁黑云母和钙角闪石组成。钛-黑云母测温结果表明,岩体最终结晶温度为834 ~ 850℃(平均845±4℃),角闪石结晶温度为876 ~ 910℃(平均893±22℃)。结晶深度估计在6.5至7.9公里之间。可以认为,钙质角闪石(logƒO2)的氧逸度稳定在−10.7 ~−11.3 bar之间(平均值=−11.05±0.4 bar)。∆NNO值在0.72 ~ 1.11之间(平均= 0.96±0.12),H2O熔体含量在4.63% ~ 5.43%之间(平均= 5.04±0.4%)。氧逸度值是钙碱性岩浆结晶的典型值之一。根据锆石UPb定年,维泽岩体在寒武—奥陶系结晶,集中在526.16±3.26 Ma和452.93±2.76 Ma两个不同的种群中。所得资料与产生维泽岩体的岩浆活动年龄(420 ~ 470 Ma,平均447.17±3.24 Ma)一致,表明其可能形成于冈瓦纳北部。受同世长英质和镁质岩浆混合作用和深熔作用的影响。地质年代学和地球化学数据表明,与会聚环境(长寿命岩浆弧)有关的岩浆活动持续存在,迫使维泽-普鲁顿经历了多阶段的熔融结晶过程。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Geochemical and geochronological evidences from Cambrian to Ordovician protracted magmatism in the Istranca Massif, NW Türkiye
Plutonic rocks in different ages are cropted out and form the basement rocks in the Istranca Massif. One of the plutons located at the basement is the Cambrian-Ordovician Vize pluton (Vize-Kırklareli) and is distinguished from other plutons by some of its characteristic features. This pluton intruded into the high-grade metamorphic sedimentary rocks, and is unconformably overlay by Triassic low-grade metamorphic rocks and Eocene aged coral reef limestones (Soğucak Formation). Based on new whole rock geochemical and zircon UPb data concentrated in two different ages, it can be said that the Vize pluton was affected by protracted magmatic activity. The igneous minerals and texture of Vize pluton are partly preserved, It has a mylonitic texture, a distinct foliation consisting of light and dark zones. In addition, metagranites contain mafic magmatic enclaves (MMEs) in some places.
The Vize pluton is an I-type pluton with predominantly peraluminous and slightly metaluminous character. It is also High-K, calc-alkaline, and reflecting volcanic arc and post-collisional tectonic settings. Mineral chemical analyses show that the mafic minerals in the Vize pluton consist of Fe-biotite and calcic amphibole (hornblende). Ti-in biotite thermometry shows that the temperature of the pluton in the final crystallization temperatures are between 834 and 850 °C (mean = 845 ± 4 °C), while the crystallization temperatures of amphiboles are between 876 and 910 °C (mean = 893 ± 22 °C). Crystallization depths are estimated to be a range of 6.5 to 7.9 km. It can be assumed that the oxygen fugacity of calcic amphiboles (logƒO2) is stabilized between −10.7 and − 11.3 bar (mean = −11.05 ± 0.4 bar). ∆NNO values are between 0.72 and 1.11 (mean = 0.96 ± 0.12) and H2O melt content is between 4.63 % and 5.43 % (mean = 5.04 ± 0.4 %). Oxygen fugacity values are among the typical values of calc-alkaline magma crystallization.
The Vize pluton was crystallized in Cambrian to Ordovician times according to zircon UPb dating is concentrated in two different populations as 526.16 ± 3.26 Ma and 452.93 ± 2.76 Ma. All data obtained are consistent with the ages of the magmatism that produced the Vize Pluton in the Balkanides and Istranca Massif of 420–470 Ma (mean 447.17 ± 3.24 Ma) and indicate that it probably formed in the northern Gondwana. It was affected by the magma-mixing processes of coeval felsic and mafic magmas, and anatexis processes. Geochronological and geochemical data indicate the existence of a protracted magmatic activity related to convergent setting (long-lived magmatic arc) that forced the Vize-Pluton to undergo multi-stage melting-crystallization processes.
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来源期刊
Chemie Der Erde-Geochemistry
Chemie Der Erde-Geochemistry 地学-地球化学与地球物理
CiteScore
7.10
自引率
0.00%
发文量
40
审稿时长
3.0 months
期刊介绍: GEOCHEMISTRY was founded as Chemie der Erde 1914 in Jena, and, hence, is one of the oldest journals for geochemistry-related topics. GEOCHEMISTRY (formerly Chemie der Erde / Geochemistry) publishes original research papers, short communications, reviews of selected topics, and high-class invited review articles addressed at broad geosciences audience. Publications dealing with interdisciplinary questions are particularly welcome. Young scientists are especially encouraged to submit their work. Contributions will be published exclusively in English. The journal, through very personalized consultation and its worldwide distribution, offers entry into the world of international scientific communication, and promotes interdisciplinary discussion on chemical problems in a broad spectrum of geosciences. The following topics are covered by the expertise of the members of the editorial board (see below): -cosmochemistry, meteoritics- igneous, metamorphic, and sedimentary petrology- volcanology- low & high temperature geochemistry- experimental - theoretical - field related studies- mineralogy - crystallography- environmental geosciences- archaeometry
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