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Wedge tectonics in South China: constraints from new seismic data. Sci Bull (Beijing) 2022; 67:1496-1507. [PMID: 36546193 DOI: 10.1016/j.scib.2022.05.007] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/16/2021] [Revised: 04/28/2022] [Accepted: 05/05/2022] [Indexed: 01/07/2023]
Abstract
Collisional orogens form when tectonic forces amalgamte fragments of Earth's continental lithosphere. The sutures between individual fragments, or terranes, are potential sites of weakness that facilitate subsequent continental breakup. Therefore, the lithospheric architecture of collisional orogens provides key information for evaluating the long-term evolution of the continental interior: for example, the South China Block (SCB), where the tectonic history is severely obscured by extensive surface deformation, magmatism, and metamorphism. Using new passive-source seismic models, we show a contrasting seismic architecture across the SCB, with three prominent crustal dipping structures across the Jiangnan Orogen. Combined with constraints from multi-disciplinary regional geophysical datasets, these pronounced dipping patterns are interpreted as relict wedge-like lithospheric deformation zones initiated in the fossil collisions that assembled the Yangtze Block and the SCB. The overall trend of these tectonic wedges implies successive crustal growth along paleo-continental margins and is indicative of northward subduction and docking of accretional terranes. In contrast, no such dipping structures are preserved in the Cathaysia Block, indicating a weak and reorganized lithosphere. The variations in the deformation responses across the SCB reflect the long-term modifications of the lithosphere caused by prolonged collision and extension events throughout the tectonic history of the SCB. Our results demonstrate the critical roles that suture zones played in the successive growth and evolution of the continental lithosphere.
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Fiorentini ML, O'Neill C, Giuliani A, Choi E, Maas R, Pirajno F, Foley S. Bushveld superplume drove Proterozoic magmatism and metallogenesis in Australia. Sci Rep 2020; 10:19729. [PMID: 33184371 PMCID: PMC7665188 DOI: 10.1038/s41598-020-76800-0] [Citation(s) in RCA: 11] [Impact Index Per Article: 2.8] [Reference Citation Analysis] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/23/2020] [Accepted: 10/20/2020] [Indexed: 11/21/2022] Open
Abstract
Large-scale mantle convective processes are commonly reflected in the emplacement of Large Igneous Provinces (LIPs). These are high-volume, short-duration magmatic events consisting mainly of extensive flood basalts and their associated plumbing systems. One of the most voluminous LIPs in the geological record is the ~ 2.06 billion-year-old Bushveld Igneous Complex of South Africa (BIC), one of the most mineralised magmatic complexes on Earth. Surprisingly, the known geographic envelope of magmatism related to the BIC is limited to a series of satellite intrusions in southern Africa and has not been traced further afield. This appears inconsistent with the inferred large size of the BIC event. Here, we present new radiometric ages for alkaline magmatism in the Archean Yilgarn Craton (Western Australia), which overlap the emplacement age of the BIC and indicate a much more extensive geographic footprint of the BIC magmatic event. To assess plume involvement at this distance, we present numerical simulations of mantle plume impingement at the base of the lithosphere, and constrain a relationship between the radial extent of volcanism versus time, excess temperature and plume size. These simulations suggest that the thermal influence of large plume events could extend for thousands of km within a few million years, and produce widespread alkaline magmatism, crustal extension potentially leading to continental break-up, and large ore deposits in distal sectors. Our results imply that superplumes may produce very extensive and diverse magmatic and metallogenic provinces, which may now be preserved in widely-dispersed continental blocks.
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Affiliation(s)
- Marco L Fiorentini
- School of Earth Sciences, University of Western Australia, 35 Stirling Hwy, Crawley, WA, 6009, Australia.
| | - Craig O'Neill
- Department of Earth and Environmental Sciences, Macquarie University, Sydney, NSW, 2109, Australia
| | - Andrea Giuliani
- Department of Earth Sciences, Institute of Geochemistry and Petrology, ETH Zurich, Clausiusstrasse 25, 8092, Zurich, Switzerland.,School of Earth Sciences, University of Melbourne, Parkville, VIC, 3010, Australia
| | - Eunjoo Choi
- School of Earth Sciences, University of Western Australia, 35 Stirling Hwy, Crawley, WA, 6009, Australia
| | - Roland Maas
- School of Earth Sciences, University of Melbourne, Parkville, VIC, 3010, Australia
| | - Franco Pirajno
- School of Earth Sciences, University of Western Australia, 35 Stirling Hwy, Crawley, WA, 6009, Australia
| | - Stephen Foley
- Department of Earth and Environmental Sciences, Macquarie University, Sydney, NSW, 2109, Australia
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