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Interpretative models of the Permian-Triassic evolution of western Laurentia and Gondwana margins. A: Idealized representation of the Pangea rotation from 260 to 230 Ma with respect to the Euler pole of rotation located in northernmost South America (Marcano et al., 1999; Golonka, 2007; Torsvik et al., 2012). The color brushes are identical to those of Fig. 1. B: Schematic cross-sections of the margins at different locations reported in A. (For interpretation of the references to colour in this figure legend, the reader is referred to the web version of this article.) 

Interpretative models of the Permian-Triassic evolution of western Laurentia and Gondwana margins. A: Idealized representation of the Pangea rotation from 260 to 230 Ma with respect to the Euler pole of rotation located in northernmost South America (Marcano et al., 1999; Golonka, 2007; Torsvik et al., 2012). The color brushes are identical to those of Fig. 1. B: Schematic cross-sections of the margins at different locations reported in A. (For interpretation of the references to colour in this figure legend, the reader is referred to the web version of this article.) 

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We present a new conceptual model to explain the first order Permian-Triassic evolution of the whole > 30 000 km long Pangea margin facing the Panthalassa ocean. Compilation of available geological, geochemical, geochronogical and paleomagnetic data all along this system allowed us to distinguish three part of the margin: western Laurentia, western...

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... margin. Since the Permian-Triassic Euler Pole of Pangea was roughly located in the Equatorial plane in northernmost South America ( Marcano et al., 1999;Golonka, 2007;Torsvik et al., 2012), we expect synchronous and opposite changes in tectonic/magmatic settings north and south of the Euler pole, in the Laurentia and Gondwana margin, respectively (Fig. 5A). We also expect limited changes of the margin geodynamic setting near the Euler pole (Central America and Eastern Australia) (Fig. ...
Context 2
... et al., 1999;Golonka, 2007;Torsvik et al., 2012), we expect synchronous and opposite changes in tectonic/magmatic settings north and south of the Euler pole, in the Laurentia and Gondwana margin, respectively (Fig. 5A). We also expect limited changes of the margin geodynamic setting near the Euler pole (Central America and Eastern Australia) (Fig. ...
Context 3
... the eastern Gondwana, including eastern Australia and New-Guinea, was facing the Pan- thalassa ocean with a trench roughly striking NNW-SSE (Cawood et al., 2011). This implies that, with respect to the Permian- Triassic Euler pole rotation of Pangea, strike-slip movements controlled the tectonic regime of eastern Gondwana during Pangea rotation (Fig. 5a). However, because the trench orientation was roughly parallel to the drifting direction of the margin it is difficult to assess how the rotation of Pangea affected the convergence ve- locity and the stress-strain conditions in these areas. Nevertheless, the rapid changes in the strain regime from transtensive to trans- pressive at ...

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... In the case of SW Gondwana, a major shift in the tectonic regime occurred in the turn from the Paleozoic to the Mesozoic era. Absolute counterclockwise rotation of Pangea since the Middle Permian (Marcano et al., 1999) with a rotation pole in northern South America (Torsvik et al., 2012) caused a decrease in the convergence velocity at the SW Gondwana margin (inducing retroarc extension) and, on the contrary, compression along the Laurentian margin (Riel et al., 2018). The Mesozoic was an era of overall continental dispersion, with continuous subduction of the paleo-Pacific plate (Panthalassa) below SW Gondwana. ...
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... The emplacement of the SLIP has been the most widely hypothesized trigger of the terrestrial and marine EPME since the early 1990s due to their temporal coincidence (3,5). However, sediments related to felsic volcanism developed extensively along the convergent margins of southern Pangea and around the Tethyan Ocean during the Permian-Triassic transition (21,43,(75)(76)(77) (Fig. 1), introducing another possible stressor for the EPME. Mercury spikes during this interval have been reported globally and are thought to be derived from the SLIP (6), but they are not correlative between different sections based on the high-resolution geochronologic framework presented here, which could be generated from different stages of the SLIP or affected by local sedimentological processes (Fig. 5). ...
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... The middle Triassic (ca. 240-230 Ma) extensional phase related to the separation between western Gondwana and Laurasia (Spikings et al. 2015) occurred due to modifications in the Panthalassa-oceanic crust subduction (Riel et al. 2018) and was also characterized by the presence of transpressive to transtensive phases in the outboard margin of western Gondwana (Bustamante et al., 2012;Riel et al. 2018 Zartman and Doe (1981). (c) initial εHf vs. age (Ma). ...
... The middle Triassic (ca. 240-230 Ma) extensional phase related to the separation between western Gondwana and Laurasia (Spikings et al. 2015) occurred due to modifications in the Panthalassa-oceanic crust subduction (Riel et al. 2018) and was also characterized by the presence of transpressive to transtensive phases in the outboard margin of western Gondwana (Bustamante et al., 2012;Riel et al. 2018 Zartman and Doe (1981). (c) initial εHf vs. age (Ma). ...
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The issue about the Sabzevar Oceanic Basin (SOB) lifetime and its paleogeographic position, as a branch of the NeoTethyan oceanic system in Northeast Iran, has long been debated. In the present work, we carried out a full reconstruction of the evolutionary geologic history of the SOB using detailed geological evidence to build a schematic descriptive model. The model describes the historical development of the SOB spanning from the Late Triassic up to Neogene; including continental rifting leading to the opening and development of an oceanic basin, magmatism and metamorphism resulting from subductional events, and finally collision to post-collisional magmatic episodes. The evidence testifies that the SOB formed as an intra-continental independent basin over the Central Iran Cadomian basement during Late Triassic-Early Jurassic times as a result of extensional movements following the subduction initiation of the Iranian sector of the NeoTethys in the Zagros orogenic belt and closed in the Paleocene after NeoTethyan early continental collision. Magmatic activity in the SOB represents a progressive spatio-temporal evolution from south to north at various time intervals during different tectonic processes with having distinct ranges of magma series including rift-related alkaline, subduction-related tholeiitic to calc-alkaline arc magmas, and post-collisional high-K to shoshonitic magmas respectively. This review indicates that the SOB experienced a classic Wilson Cycle, operating over a period of approximately 130 million years (185–55 Ma).
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Article
The evolution of the Neo-Tethys realm had a significant impact on the Phanerozoic paleogeography of the Iran Plateau. However, there remains significant debate regarding the timing of the opening and closure of the Neo-Tethys ocean, as well as the initial stages of subduction and the style of subduction. In this paper, we review the geological data relevant to the Zagros sector of the Neo-Tethys and the associated arc zones (SaSZ and UDMA) in order to update our understanding of the geodynamic history of this region, from early rifting to final closure. Our analysis of Late Devonian-Early Permian rift-related rocks and subsequent subsidence and shallow marine sedimentation through the Triassic period provides compelling evidence for the occurrence of rifting and the formation of a passive margin in the Late Paleozoic. The Late Triassic closure of the Paleo-Tethys ocean in northern Iran marks the inception of Neo-Tethys ocean subduction. Our revised perspective on the subduction style suggests that subduction of the Neo-Tethys oceanic slab began simultaneously across the entire zone in the Late Triassic-Early Jurassic, leading to the production of intraoceanic arc magmatic rocks. However, the variable rates of magma production and the change in the geochemical signature of magmatic rocks from oceanic to continental type observed in the northern domain during the Middle-Late Jurassic indicate a shift from intraoceanic arc to continental arc subduction. In the southern segment, intraoceanic subduction was still ongoing during this time period. While the early Cretaceous in the southern segment is characterized by the initial obduction of ophiolites, the Late Cretaceous in the entire zone is marked by the underthrusting of the Arabian passive margin, coinciding with the obduction of Cretaceous ophiolites on the overriding plate and the subsequent subduction of stretched and denser continental Arabian lithosphere with overlying ophiolites. Our tectonic reconstruction highlights the asynchronous nature of the final closure of the Neo-Tethys, which occurred first along the northern margin during the Late Eocene-Early Oligocene and then along the southern margin during the Miocene.