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The generation and evolution of the Archean continental crust: The granitoid story in southeastern Brazil
Institution:1. Depto. de Geologia, IGEO, Universidade Federal do Rio de Janeiro, UFRJ, Rio de Janeiro, RJ, Brazil;2. School of Earth Sciences, University of Bristol, Bristol, United Kingdom;3. Instituto de Geociências, Universidade de Brasília, UnB, Brasília, DF, Brazil;4. Instituto de Geociências, Universidade de São Paulo, USP, São Paulo, SP, Brazil;5. Instituto de Geociências e Ciências Exatas, Universidade Estadual Paulista, Rio Claro, SP, Brazil;6. Institute of Geology, Mineralogy and Geophysics, Ruhr-Universität Bochum, Universitätsstraße 150, 44801 Bochum, Germany;7. ISOTOPIA Lab, School of Earth, Atmosphere and Environment, Monash University, Wellington Rd, Clayton, VIC 3800, Australia;8. Programa de Pós-Graduação em Geociências, IG, Universidade Federal do Rio Grande do Sul, UFRGS, Porto Alegre, RS, Brazil
Abstract:The Archean Eon was a time of geodynamic changes. Direct evidence of these transitions come from igneous/metaigneous rocks, which dominate cratonic segments worldwide. New data for granitoids from an Archean basement inlier related to the Southern São Francisco Craton (SSFC), are integrated with geochronological, isotopic and geochemical data on Archean granitoids from the SSFC. The rocks are divided into three main geochemical groups with different ages: (1) TTG (3.02–2.77 Ga); (2) medium- to high-K granitoids (2.85–2.72 Ga); and (3) A-type granites (2.7–2.6 Ga). The juvenile to chondritic (Hf-Nd isotopes) TTG were divided into two sub-groups, TTG 1 (low-HREE) and 2 (high-HREE), derived from partial melting of metamafic rocks similar to those from adjacent greenstone belts. The compositional diversity within the TTG is attributed to different pressures during partial melting, supported by a positive correlation of Dy/Yb and Sr/Zr, and batch melting calculations. The proposed TTG sources are geochemically similar to basaltic rocks from modern island-arcs, indicating the presence of subduction processes concomitant with TTG emplacement. From ~2.85 Ga to 2.70 Ga, the dominant rocks were K-rich granitoids. These are modeled as crustal melts of TTG, during regional metamorphism indicative of crustal thickening. Their compositional diversity is linked to: (i) differences in source composition; (ii) distinct melt fractions during partial melting; and (iii) different residual mineralogies reflecting varying P–T conditions. Post-collisional (~2.7–2.6 Ga) A-type granites reflect rifting in that they were closely followed by extension-related dyke swarms, and they are interpreted as differentiation or partial melting products of magmas derived from subduction-modified mantle. The sequence of granitoid emplacement indicates subduction-related magmatism was followed by crustal thickening, regional metamorphism and crustal melting, and post-collisional extension, similar to that seen in younger Wilson Cycles. It is compelling evidence that plate tectonics was active in this segment of Brazil from ~3 Ga.
Keywords:Granitoid petrogenesis  Archean geodynamics  Crustal evolution  TTGs  A-types  Batch melting calculations
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