Análise de fácies e petrografia de uma seção do Membro Crato em Nova Olinda (CE): contribuições à história deposicional e diagenética do neoaptiano na Bacia do Araripe

• Autor(a) principal: Santos, Felipe Holanda dos
• Data de Publicação: 2017
• Outros Autores: Azevedo, Juan Moreira de, Nascimento Junior, Daniel Rodrigues do, Souza, Ana Clara Braga de, Mendes, Marcio, Bezerra, Irineudo, Limaverde, Saulo
• Tipo de documento: Artigo
• Idioma: por
• Título da fonte: Repositório Institucional da Universidade Federal do Ceará (UFC)
• Texto Completo: http://www.repositorio.ufc.br/handle/riufc/65253
• topic: Bacia do Araripe; Membro Crato; Análise de fácies; Diagênese

The Crato Member is one of the most important stratigraphic units of the Araripe Basin due to its fossil content, its context analogous to the Brazilian “Pre-Salt Layers”, and its use as covering stone. Facies and petrographic analyses were combined in our study of a section of the Crato Member in Nova Olinda (State of Ceará, Brazil), aiming to investigate its depositional and diagenetic history. Thus, we analysed the faciology of a continuous columnar section ca. 70 m thick, and collected 13 samples of limestones, sandstones and evaporites. The collected samples were analysed by optical petrography. Five depositional facies were described: massive marly mudstone (Lm), laminated calcilutite (Cl), almost-massive arenite (Am), siltite with climbing ripple lamination (Scc), and columnar evaporite (Ec). The thickest and recurrent facies were interpreted as lacustrine (Lm, Cl), followed by alluvial successions (Am, Scc) interbedded between the lacustrine ones. The succession finishes with faciological evidences for extreme arid conditions (Ec) reached at the end of the interval. The petrography, here focused on rocks of facies Cl, Aqm, and Scc, reinforces the idea of an arid lacustrine system for the local Aptian Stage, and that this system was fed by immature alluvial flows coming from close source areas. Particularly, the very low grade of mechanical compaction and incipient cementation of the terrigenous rocks suggest that the succession as a whole was barely affected by diagenesis after burial that, for this reason, was shallow. The resemblance of the Crato Member terrigenous intervals to the ones of the final of the underlying Barbalha Formation suggests contemporaneity and transitional retrograding passage from one unit to another.