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dc.contributor.authorCawood, Peter A.
dc.contributor.authorZhao, Guochun
dc.contributor.authorYao, Jinlong
dc.contributor.authorWang, Wei
dc.contributor.authorXu, Yajun
dc.contributor.authorWang, Yuejun
dc.date.accessioned2018-07-03T10:00:34Z
dc.date.available2018-07-03T10:00:34Z
dc.date.issued2018-11
dc.identifier.citationCawood , P A , Zhao , G , Yao , J , Wang , W , Xu , Y & Wang , Y 2018 , ' Reconstructing South China in Phanerozoic and Precambrian supercontinents ' , Earth Science Reviews , vol. 186 , pp. 173-194 . https://doi.org/10.1016/j.earscirev.2017.06.001en
dc.identifier.issn0012-8252
dc.identifier.otherPURE: 250418479
dc.identifier.otherPURE UUID: 7a6d2108-5d4f-41c2-8563-df9fa577eed2
dc.identifier.otherRIS: urn:79E8AA73D7C936CE68115873C06C7060
dc.identifier.otherScopus: 85023638975
dc.identifier.otherWOS: 000453642800008
dc.identifier.urihttps://hdl.handle.net/10023/14834
dc.descriptionThis paper is financially supported by a NSFC Major Program (41190070) entitled “Reconstruction of East Asian Blocks in Pangea”. PAC acknowledges support from the Australian Research Council grant FL160100168 and WW thanks the support from “Thousand Youth Talents Plan”.en
dc.description.abstractThe history of the South China Craton and the constituent Yangtze and Cathaysia blocks are directly linked to Earth's Phanerozoic and Precambrian record of supercontinent assembly and dispersal. Exposed Archean rocks are limited to isolated fragments in the Yangtze Block that preserve a record of Meso- to Neo-Archean magmatism, sedimentation and metamorphism associated with a period of global craton formation and stabilization that corresponds with the assembly of the Kenor supercontinent/supercraton. However, there are insufficient data to link its history with other similar aged cratons. The tectonostratigraphic record in South China in the Paleoproterozoic, corresponding with the assembly of Nuna, suggests that rock units in the Yangtze Block were spatially linked with northwestern Laurentia and possibly Siberia, whereas Cathaysia was joined to northern India. During the formation of Rodinia at the end of the Mesoproterozoic through to that of Pangea in the mid-Paleozoic, Cathaysia remained joined to northern India. Early Neoproterozoic supra-subduction zone magmatic arc-back arc assemblages ranging in age from ~ 1000 Ma to 810 Ma occur within Cathaysia, along its northwestern margin, and along the southeastern margin of the Yangtze Block. These rocks provide a record of convergent plate interaction, which continued along the western margin of the Yangtze Block until around 700 Ma and correlates with similar along strike subduction zone magmatism in northwest India, Seychelles and Madagascar. During the final assembly of Gondwana in the early Paleozoic suturing of India-South China with the Western Australia-Mawson blocks along the Kuunga Orogen resulted in the accretion of the Sanya Block of Hainan Island with the rest of Cathaysia. The accretion of Laurussia to Gondwana in the mid-Paleozoic to form Pangea corresponds with the initiation of lithospheric extension along the northern margin of Gondwana and the separation of a number of continental blocks, including South China, which then drifted northward across the Paleo-Tethys to collide with the Asian segment of Pangea in the Permo-Triassic.
dc.language.isoeng
dc.relation.ispartofEarth Science Reviewsen
dc.rights© 2017 Elsevier Ltd. All rights reserved. This work has been made available online in accordance with the publisher’s policies. This is the author created, accepted version manuscript following peer review and may differ slightly from the final published version. The final published version of this work is available at https://doi.org/10.1016/j.earscirev.2017.06.001en
dc.subjectSupercontinenten
dc.subjectPangeaen
dc.subjectGondwanaen
dc.subjectRodiniaen
dc.subjectNunaen
dc.subjectGE Environmental Sciencesen
dc.subjectDASen
dc.subject.lccGEen
dc.titleReconstructing South China in Phanerozoic and Precambrian supercontinentsen
dc.typeJournal articleen
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews. School of Geography and Geosciencesen
dc.contributor.institutionUniversity of St Andrews. School of Earth & Environmental Sciencesen
dc.contributor.institutionUniversity of St Andrews. Scottish Oceans Instituteen
dc.contributor.institutionUniversity of St Andrews. St Andrews Isotope Geochemistryen
dc.identifier.doihttps://doi.org/10.1016/j.earscirev.2017.06.001
dc.description.statusPeer revieweden
dc.date.embargoedUntil2018-07-03


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