| Full text | |
| Author(s): |
Yokoyama, E.
[1]
;
Trindade, R. I. F.
[1]
;
Lana, C.
[2]
;
Souza Filho, C. R.
[3]
;
Baratoux, D.
[4, 5]
;
Marangoni, Y. R.
[1]
;
Tohver, E.
[6]
Total Authors: 7
|
| Affiliation: | [1] Univ Sao Paulo, Inst Astron Geofis & Ciencias Atmosfer, BR-05508090 Sao Paulo - Brazil
[2] Univ Fed Ouro Preto, Dept Geol DEGEO, BR-35400000 Ouro Preto, MG - Brazil
[3] Univ Estadual Campinas, Dept Geol & Recursos Nat, Inst Geociencias, BR-13083970 Campinas, SP - Brazil
[4] Observ Midi Pyrenees, Lab Dynam Terr & Planetaire, UMR 5562, CNRS, F-31400 Toulouse - France
[5] Univ Toulouse 3, F-31400 Toulouse - France
[6] Univ Western Australia, Tecton Special Res Ctr, Crawley, WA 6009 - Australia
Total Affiliations: 6
|
| Document type: | Journal article |
| Source: | Earth and Planetary Science Letters; v. 331, p. 347-359, MAY 15 2012. |
| Web of Science Citations: | 4 |
| Abstract | |
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. (AU) | |