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扎格罗斯造山带最东南部晚渐新世至中中新世的碰撞时间与物源转移

Collision Timing and Provenance Shifts from the Late Oligocene to Middle Miocene in the Southeasternmost Zagros Orogen.

作者信息

GholamiZadeh Parisa, Wan Bo, Garzanti Eduardo, Hu Xiumian, Esmaeili Rasoul, Ebrahimi Mohammad

机构信息

State Key Laboratory of Lithospheric and Environmental Coevolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, 100029, China.

Geological Survey of Iran, Tehran, Iran.

出版信息

Sci Rep. 2025 Feb 19;15(1):6023. doi: 10.1038/s41598-025-90186-x.

Abstract

Determining the timing of the initial continental collision is a fundamental step in accurately reconstructing the paleogeodynamic evolution of orogenic belts. This process necessitates a comprehensive integration of evidence gathered through various analytical techniques, both in the field and in the laboratory, to achieve a conclusive understanding. We here use comprehensive methods, including sandstone petrography, U-Pb dating, trace element and Hf isotopic compositions of the detrital zircon, in the Haji Abad (eastern Zagros Orogen) and the Shamil areas (west of the Minab-Zendan Fault) to constrain the timing of the initial collision between Arabia and Eurasia. Zircon U-Pb dating in the Haji Abad area reveals that detritus predominantly originates from the Arabia Pan-African basement (∼640 - 539 Ma, Ɛ (t): -10 to + 10) at the base of the Upper Oligocene-Lower Miocene Razak Formation. This is subsequently replaced up-section by detritus from Cenozoic and Mesozoic Eurasia magmatic-arc sources (~ 54 - 10 Ma, Ɛ (t): -2 to + 16; ~110 - 89 Ma, Ɛ (t): -2 to + 20, and ~ 175 - 163 Ma, Ɛ (t): -4 to + 10). In contrast, the Shamil area shows that detritus from the Pan-African Arabia basement remained dominant until the Early Miocene. The minimum age of continental collision is characterized by a significant change in provenance, transitioning from detritus sourced from the Arabia lower plate to that derived from the Eurasia upper plate. This transition is documented from the Late Oligocene in the Neyriz and Haji Abad areas along the Main Zagros Thrust, to the Middle Miocene (Langhian) in the Shamil area along the Minab-Zendan Fault.

摘要

确定初始大陆碰撞的时间是准确重建造山带古地球动力学演化的基本步骤。这一过程需要综合运用通过各种分析技术在野外和实验室收集的证据,以达成确凿的认识。我们在此运用综合方法,包括砂岩岩石学、U-Pb年代测定、碎屑锆石的微量元素和Hf同位素组成分析,对哈吉阿巴德(扎格罗斯造山带东部)和沙米尔地区(米纳卜-赞丹断层以西)进行研究,以限定阿拉伯板块与欧亚板块初始碰撞的时间。哈吉阿巴德地区的锆石U-Pb年代测定显示,碎屑主要源自上渐新统-下中新统拉扎克组底部的阿拉伯泛非基底(约640 - 539 Ma,Ɛ (t):-10至+10)。随后,在剖面中,这些碎屑被来自新生代和中生代欧亚岩浆弧源的碎屑所取代(约54 - 10 Ma,Ɛ (t):-2至+16;约110 - 89 Ma,Ɛ (t):-2至+20,以及约175 - 163 Ma,Ɛ (t):-4至+10)。相比之下,沙米尔地区显示,直到中新世早期,来自泛非阿拉伯基底的碎屑仍然占主导地位。大陆碰撞的最小年龄以物源的显著变化为特征,即从源自阿拉伯下盘的碎屑转变为源自欧亚上盘的碎屑。这种转变在扎格罗斯主逆冲断层沿线的内里斯和哈吉阿巴德地区从晚渐新世就有记录,在米纳卜-赞丹断层沿线的沙米尔地区则记录到了中新世中期(兰盖阶)。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/3f42/11839924/4e03de26d105/41598_2025_90186_Fig1_HTML.jpg

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