Decoding the evolution of Paleo-Tethys: Geochemical and geochronological reinterpretation of the Paleozoic ultra-mafic to felsic rocks in Northeast Iran
Hadi Karimi , Hripsime Gevorgyan , Lothar Ratschbacher , Zhao Yang , Axel Gerdes , Abbas Etemadi
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引用次数: 0
Abstract
The tectono-magmatic evolution of NE Iran records the Paleozoic–early Mesozoic formation and consumption of the Paleo-Tethys Ocean. Debates focus on how the regionally-distributed basement exposures and their diverse evolution settings—such as rifting, oceanic-plateau formation, arc magmatism, and collision—are connected. The compositionally diverse meta-igneous rocks comprise the early Paleozoic Neyshabur complex, the Mississippian–Cisuralian Vakilabad complex (‘Mashhad metamorphics’), the Cisuralian Fariman complex, and the Frasnian–Permian Darreh Anjir complex; the age assignment is preliminary. Combining new field, geochemical, and geochronologic data with published ones, we specify the connection and evolution of these complexes. The Neyshabur complex has dominantly alkaline and subordinate tholeiitic rocks dated at 490–435 Ma (UPb zircon). In terms of high field strength element rations, such as Nb/Y vs. Zr/Y, they record long-lasting, mantle-plume triggered continental rifting along the northern Gondwana margin. A ∼ 364 Ma (UPb apatite) age dates hydrothermal alteration and deformation, possibly recording the integration of this complex into an oceanic accretionary wedge. Circa 195 Ma (Ar/Ar amphibole and plagioclase) metamorphism dates collisional-wedge formation, i.e., the collision of the Central Iranian (Gondwana) and Turan Blocks (Eurasia). In the Vakilabad complex, 281–268 Ma (Ar/Ar amphibole) ages of meta-komatiite/gabbro match those (∼276 Ma; cumulate) of ultra-mafic to mafic rocks of the southern Fariman complex; a ∼ 320 Ma (UPb titanite) age of tholeiitic basalt in the Vakilabad complex supports the presence of older rocks, suggested by Carboniferous radiolarian cherts. 188–183 Ma (Ar/Ar mica) metamorphism again dates collisional-wedge formation. The Darreh Anjir-complex rocks with a supra-subduction zone signature record subduction beneath an oceanic plateau within the Paleo-Tethys Ocean. The Vakilabad and the southern Fariman complexes comprise an oceanic plateau built by a mantle plume. This plateau accreted to the hanging-wall plate prior to the terminal collision, detached from the lower plate, blocked the subduction, and caused slab break-off and slab-window formation; the slab window allowed plume material to ascend. The northern Fariman complex documents this process: the rising plume material— depleted by the extraction of OIB-like magma—mixed with fluids from the subducting slab, creating boninite-like magmas. Calc-alkaline andesitic magmas, likely originating from the mantle wedge, coexisted with the OIB-like and boninite-like magmas. Our study provides an evolution model that integrates the various complexes of NE Iran into a common Late Cambrian to Late Triassic evolution of the Paleo-Tethys.
伊朗东北部的构造-岩浆演化记录了古生代-中生代早期古特提斯洋的形成和消耗。争论集中在区域分布的基底暴露及其不同的演化背景(如裂陷、海洋高原形成、弧岩浆作用和碰撞)是如何联系在一起的。变质火成岩组成多样,包括早古生代Neyshabur杂岩、西侏罗统—西侏罗统Vakilabad杂岩(“Mashhad变质岩”)、西侏罗统Fariman杂岩和frasian—permian Darreh Anjir杂岩;年龄分配是初步的。结合新的野外、地球化学和地质年代学资料和已发表的资料,明确了这些杂合体的联系和演化。Neyshabur杂岩以碱性和次生拉斑岩为主,年龄为490 ~ 435 Ma (UPb锆石)。就高场强元素比率而言,例如Nb/Y vs. Zr/Y,它们记录了沿冈瓦纳北部边缘的长时间、地幔柱引发的大陆裂谷。A ~ 364 Ma (UPb磷灰石)年龄确定了热液蚀变和变形,可能记录了该复合体与海洋增生楔的整合。约195 Ma (Ar/Ar角闪洞和斜长石)变质作用日期为碰撞楔块形成,即中伊朗(冈瓦纳)和图兰地块(欧亚大陆)的碰撞。在Vakilabad杂岩中,变质科马长岩/辉长岩的281 ~ 268 Ma (Ar/Ar角闪洞)年龄与(~ 276 Ma)相符;南法里曼杂岩的超基性至基性岩的堆积;瓦基拉巴德杂岩中拉斑玄武岩的一个~ 320 Ma (UPb钛矿)年龄支持石炭纪放射虫质燧石的存在。188-183 Ma (Ar/Ar云母)变质作用再次追溯到碰撞楔形成时期。具有超俯冲带特征的Darreh anjir杂岩记录了古特提斯洋海洋高原下的俯冲作用。瓦基拉巴德和南法里曼复合体组成了一个由地幔柱形成的海洋高原。该高原在最终碰撞前向上壁板块吸积,与下壁板块分离,阻断俯冲,导致板块断裂和板块窗形成;厚板窗允许羽流物质上升。北法里曼复合体记录了这一过程:上升的羽流物质——被类似oib的岩浆所耗尽——与俯冲板块的流体混合,形成了类似博尼玛岩的岩浆。钙碱性安山岩岩浆可能起源于地幔楔,并与类欧布岩和类硼岩浆岩共存。我们的研究提供了一个演化模式,将伊朗东北部的各种复合体整合为一个共同的晚寒武世至晚三叠世的古特提斯演化。
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.