Geochemistry of siltstones from the Permian Corumbatai Formation from the Parana Basin(State of Sao Paulo, Brazil): Insights of provenance, tectonic and climatic settings

The Corumbatai Formation is a Permian sedimentary unity comprising siltstones, claystones and very fine sandstones, deposited above calcific shales, bituminous shales and dolomitic limestones from the Irati Formation, indicating severe changes in tectonic and climatic conditions in a short span duri...

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Detalhes bibliográficos
Autores: Montibeller, Cibele Carolina [UNESP], Beltran Navarro, Guillermo Rafael [UNESP], Zanardo, Antenor [UNESP], Rohn, Rosemarie [UNESP], Del Roveri, Carolina, Rocha, Rogers Raphael da [UNESP], Conceicao, Fabiano Tomazini da [UNESP]
Formato: artículo
Estado:Versión publicada
Fecha de publicación:2020
País:Brasil
Recursos:Universidade Estadual Paulista (UNESP)
Repositorio:Repositório Institucional da UNESP
Idioma:inglés
OAI Identifier:oai:repositorio.unesp.br:11449/197122
Acesso em linha:http://dx.doi.org/10.1016/j.jsames.2020.102582
http://hdl.handle.net/11449/197122
Access Level:acceso abierto
Palavra-chave:Lithogeochemistry
Pangea
Intracratonic basin
Gondwana I Supersequence
Major elements geochemistry
Sedimentary geochemistry
Descrição
Resumo:The Corumbatai Formation is a Permian sedimentary unity comprising siltstones, claystones and very fine sandstones, deposited above calcific shales, bituminous shales and dolomitic limestones from the Irati Formation, indicating severe changes in tectonic and climatic conditions in a short span during the evolution of the Parana Basin. Through geochemical analysis of major elements, it is possible to observe that some characteristics of the Corumbatai Formation indicate that the climate on the period of deposition was arid or semiarid, with low contribution of fluvial and pluvial waters, and that, as expected, the chemical signature of the sediments are similar to the adjacent orogenic belts, despite that no tectonically active areas or magmatic arcs were registered in the surroundings of the Parana Basin during Permian. These aspects suggest that the aridization of the Pangea Supercontinent started earlier than considered so far, and that the source areas for this sedimentary unity most probably were distant from the basin, being that the main possible transportation process of the detritic grains should be aeolian.