Abstract

The eastern side of the Dom Feliciano Belt consists of supracrustal rocks and granitic batholiths whose emplacements were controlled by the tectonic evolution of the belt. The evolution of this belt had both a tangential tectonic regime and a transcurrent one. The tangential regime, defined by low angle planar and linear structures with W-NW tectonic transport, was responsible for crustal thickening and tectonic imbrication and controlled the syn-kinematic injections of high-K calc-alkaline granitoid plutons of the Arroio Solidão Intrusive Suite about 800 Ma. The transcurrent regime is defined by high angle deformation sets of planar and linear structures, parallel to the elongation of the belt, and indicative of a N-NE tectonic transport. Its associated magmatism began about 672 Ma with the intrusion of the calc-alkaline granitoids of the Arroio Moinho Intrusive Suite, followed by basic dykes and the 630–617 Ma crustal melt granites of the Cordilheira Intrusive Suite. The transcurrent tectonics generated shear zones hundreds of meters in width, which probably extend deep into the mantle. At the end of this process, an extensional regime was installed and during this transition, late- to post-kinematic calc-alkaline granitoids of the Campinas Intrusive Suite were intruded. This magmatism developed during the extensive regime and is represented by the 585 Ma post-transcurrent calc-alkaline granitoids of the Canguçu Intrusive Suite. Alkaline-metaluminous granitoids of the Encruzilhada Intrusive Suite and a few small bodies of peralkaline granitoids represent the final episodes of the granitic magmatism in this region. The syn-tangential granitoids are high-K calc-alkaline and have similarities to those of a continental collision regime. The syn- to post-transcurrent high-K calc-alkaline granitoids are similar to the late- to post-orogenic injections of other orogenic belts. Peraluminous leucogranites of the Cordilheira Intrusive Suite occur also in this transcurrent tectonic setting. The main characteristics of the calc-alkaline magmatism can be related to the participation of a thick continental crust during its generation similar to the granitic systems of a continental collision. Their negative ɛNd values may reflect a magma source closely connected to the continental crust, with their igneous protoliths of relatively homogeneous composition related to a continental collision phase. This continental collision occurred concurrent with the closing of a passive platform-type basin, after the end of sedimentation and tholeiitic volcanic activities.

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