The persistence and role of basin structures on the 3D architecture of the Mara帽贸n Fold-Thrust Belt, Peru

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• 作者：Arne F. Scherrenberg ; ^{arne.scherrenberg@gmail.com" class="auth_mail} ; Rodney J. Holcombe ^{rod@holcombe.net.au" class="auth_mail} ; Gideon Rosenbaum ^{g.rosenbaum@uq.edu.au" class="auth_mail}
• 关键词：Marañ ; ó ; n Fold-Thrust Belt ; Thin-skinned deformation ; Thick-skinned deformation ; Peru ; Andes
• 刊名：Journal of South American Earth Sciences
• 出版年：April, 2014
• 年：2014
• 卷：51
• 期：Complete
• 页码：45-58
• 全文大小：5682 K

文摘

The 3D architecture of fold-thrust belts commonly involves thin-skinned and thick-skinned deformation. Both thick- and thin-skinned deformation styles have been suggested to occur in the Mara帽贸n Fold-Thrust Belt (MFTB) in Peru, but the relative timing and strain partitioning associated with them are not well understood. We demonstrate that inherited basement structures along the Peruvian convergent margin reactivated during the evolution of the MFTB. We present results from field mapping, interpretation of remote sensing imagery, and cross section construction and restoration. The results show that the Chonta Fault, a median pre-folding basin normal fault, was inverted and acted as a mechanical buttress during initial east-vergent contraction of the fold-thrust belt. This fault separates the belt into two domains of distinctly different structural styles. During the Eocene, units to the west of the Chonta Fault deformed by folding, using the fault as a buttress, and subsequently propagated eastward by thin-skinned thrusting. This was followed in the Miocene by west-vergent, basement-involved deformation, which overprinted the earlier east-vergent, thin-skinned structures. The proposed tectonic model of the MFTB highlights the role of basement-fault reactivation during orogenesis and the involvement of deep structures in partitioning deformation styles.