Magnetic fabric of Araguainha complex impact structure (Central Brazil): Implications for deformation mechanisms and central uplift formation


Autoria(s): Yokoyama, E.; Trindade, R. I. F.; Lana, C.; Souza Filho, C. R.; Baratoux, D.; Marangoni, Y. R.; Tohver, E.
Contribuinte(s)

UNIVERSIDADE DE SÃO PAULO

Data(s)

05/11/2013

05/11/2013

2012

Resumo

The weakening mechanisms involved in the collapse of complex impact craters are controversial. The Araguainha impact crater, in Brazil, exposes a complex structure of 40 km in diameter, and is an excellent object to address this issue. Its core is dominated by granite. In addition to microstructural observations, magnetic studies reveal its internal fabric acquired during the collapse phase. All granite samples exhibit impact-related planar deformation features (PDFs) and planar fractures (PFs), which were overprinted by cataclasis. Cataclastic deformation has evolved from incipient brittle fracturing to the development of discrete shear bands in the center of the structure. Fracture planes are systematically decorated by tiny grains (<10 mu m) of magnetite and hematite, and the orientation of magnetic lineation and magnetic foliation obtained by the anisotropies of magnetic susceptibility (AMS) and anhysteretic remanence (AAR) are perfectly coaxial in all studied sites. Therefore, we could track the orientation of deformation features which are decorated by iron oxides using the AMS and AAR. The magnetic fabrics show a regular pattern at the borders of the central peak, with orientations consistent with the fabric of sediments at the crater's inner collar and complex in the center of the structure. Both the cataclastic flow revealed from microstructural observations and the structural pattern of the magnetic anisotropy match the predictions from numerical models of complex impact structures. The widespread occurrence of cataclasis in the central peak, and its orientations revealed by magnetic studies indicate that acoustic fluidization likely operates at all scales, including the mineral scales. The cataclastic flow made possible by acoustic fluidization results in an apparent plastic deformation at the macroscopic scale in the core. (C) 2012 Elsevier B.V. All rights reserved.

Sao Paulo State Science Foundation (FAPESP)

Sao Paulo State Science Foundation (FAPESP) [05/51530-3]

Brazilian Research Council (CNPq)

Brazilian Research Council (CNPq)

Identificador

EARTH AND PLANETARY SCIENCE LETTERS, AMSTERDAM, v. 331, n. 1, Special Issue, supl. 4, Part 1, pp. 347-359, MAY 15, 2012

0012-821X

http://www.producao.usp.br/handle/BDPI/41705

10.1016/j.epsl.2012.01.005

http://dx.doi.org/10.1016/j.epsl.2012.01.005

Idioma(s)

eng

Publicador

ELSEVIER SCIENCE BV

AMSTERDAM

Relação

EARTH AND PLANETARY SCIENCE LETTERS

Direitos

restrictedAccess

Copyright ELSEVIER SCIENCE BV

Palavras-Chave #COMPLEX IMPACT CRATER #WEAKENING MECHANISM #MICROSTRUCTURES #MAGNETIC ANISOTROPY #ARAGUAINHA #ACOUSTIC FLUIDIZATION #CATACLASTIC FLOW #CRATER COLLAPSE #UPHEAVAL DOME #NOJIMA FAULT #MATO-GROSSO #SUSCEPTIBILITY #ANISOTROPY #SUDBURY #REMANENCE #GEOCHEMISTRY & GEOPHYSICS
Tipo

article

original article

publishedVersion