IR @ Goa University

The ~1.4 Ga A-type granitoids in the "Chottanagpur crustal block" (India), and its relocation from Columbia to Rodinia?

Show simple item record

dc.contributor.author Sequeira, N.
dc.contributor.author Bhattacharya, A.
dc.contributor.author Bell, E.
dc.date.accessioned 2021-02-02T04:20:02Z
dc.date.available 2021-02-02T04:20:02Z
dc.date.issued 2021
dc.identifier.citation Geoscience Frontiers. 13(2); 2022; ArticleID_101138. en_US
dc.identifier.uri https://doi.org/10.1016/j.gsf.2020.12.017
dc.identifier.uri http://irgu.unigoa.ac.in/drs/handle/unigoa/6362
dc.description.abstract In paleogeographic reconstructions of the Columbia and Rodinia Supercontinents, the position of the Greater India landmass is ambiguous. This, coupled with a limited understanding of the tectonic evolution of the mobile belts along which the mosaic of crustal domains in India accreted, impedes precise correlation among the dispersed crustal fragments in supercontinent reconstructions. Using structural, metamorphic phase equilibria, chronological and geochemical investigations, this study aims to reconstruct the tectonic evolution of the Chottanagpur Gneiss Complex (CGC) as a distinct crustal block at the eastern end of the Greater Indian Proterozoic Fold Belt (GIPFOB) along which the North India Block (NIB) and the South India Block (SIB) accreted. The study focuses on two issues, e.g. dating the Early Neoproterozoic (0.92 Ga) accretion of the CGC with the NIB contemporaneous with the assembly of Rodinia, and documenting the widespread (less than 24,000 square km) plutonism of 1.5-1.4 Ga weakly peraluminous, calc-alkalic to alkali-calcic and ferroan A-type granitoids (plus or minus garnet) devoid of mafic microgrannular enclaves and coeval mafic emplacements in the crustal block. These dominantly within-plate granitoids arguably formed by asthenospheric upwelling induced partial melting of garnet-bearing anatectic quartzofeldspathic gneisses that dominate the Early Mesoproterozoic basement of the block. The major and trace element chemistry of the granitoids is similar to the 1.35-1.45 Ga A-type granitoids in Laurentia/Amazonia emplaced contemporaneous with the 1.5-1.3 Ga breakup of the Columbia Supercontinent. This study suggests the Chottanagpur Gneiss Complex occured as a fragmented crustal block following the breakup of the Columbia Supercontinent; the crustal block was subsequently integrated within India during the Early Neoproterozoic oblique accretion between the NIB and SIB contemporaneous with the Rodinia Supercontinent assembly. en_US
dc.publisher Elsevier en_US
dc.subject Earth Sciences en_US
dc.title The ~1.4 Ga A-type granitoids in the "Chottanagpur crustal block" (India), and its relocation from Columbia to Rodinia? en_US
dc.type Journal article en_US
dc.identifier.impf y


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search IR


Advanced Search

Browse

My Account