The 2.26 to 2.18 Ga Arc-Related Magmatism of the Almas-Conceicao do Tocantins Domain: An Early Stage of the Sao Francisco Paleocontinent Assembly in Central Brazil
Abstract
Paleoproterozoic (Rhyacian) rocks dominate within the basement of the Neoproterozoic Brasilia Belt and their genesis has been attributed to the orogenic amalgamation event that assembled the Sao Francisco-Congo paleocontinent from 2.18 to 2.07 Ga. However, the tectonic framework and genesis of the building blocks involved in this continent-wide amalgamation event are unclear, particularly in relation to terranes from the Almas-Conceicao do Tocantins Domain, in the Goi ' as Massif, central Brazil. This work provides new whole-rock chemical and geochronological data, which indicate the generation of felsic to intermediate magmatism around 2.29 and 2.28 Ga corresponding to the Monzogranitic Unit and the Quartz-dioritic Suite, respectively. Later magmatic events occurred in a continental arc setting, around 2.26 to 2.2 Ga represented by metaluminous to peraluminous I-type magmatism of the Granodioritic to Tonalitic Suite (GTS) and the Serra do Boqueirao Suite. Around 2.2 to 2.18 Ga a peraluminous I-type magmatism took place and generated the Peraluminous Suite (PS). Our data show that after an earlier Siderian magmatic event around 2.45-2.34 Ga, reported in previous works, the Almas do Conceicao do Tocantins Domain oversaw additional Rhyacian events of magmatic activity around 2.29 Ga to 2.18 Ga. Regional geotectonic correlations with the Sao Francisco Craton and other pericratonic belts indicate coeval magmatic events taking place during the early stages of the Columbia Supercontinent amalgamation.
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Título según WOS: | The 2.26 to 2.18 Ga Arc-Related Magmatism of the Almas-Conceicao do Tocantins Domain: An Early Stage of the Sao Francisco Paleocontinent Assembly in Central Brazil |
Título de la Revista: | JOURNAL OF SOUTH AMERICAN EARTH SCIENCES |
Volumen: | 104 |
Editorial: | Pergamon |
Fecha de publicación: | 2020 |
DOI: |
10.1016/j.jsames.2020.102757 |
Notas: | ISI |