Thick-skinned and thin-skinned thrusting in the La Ramada fold and thrust belt:: crustal evolution of the High Andes of San Juan, Argentina (32°SL)

The Cenozoic structural evolution of the La Ramada fold and thrust belt in the High Andes of Argentina, between 32 degrees 00'S and 32 degrees 30'S, shows in time and space the interaction of thin-skinned and thick-skinned deformations. Based on geometric and kinematic constraints, three different deformation stages have been recognized. The first began with thin-skinned NNW-trending structures detached in Upper Jurassic gypsum. In the second stage, the basement was involved by tectonic inversion of Triassic normal faults producing a thick-skinned fold and thrust belt. This inversion, combined with the ductile rheology of the Jurassic gypsum, resulted in refolding of older structures. The uplift of the basement by high-angle reverse faults at the Ramada-Espinacito Massif, produced a sticking point in the foreland propagation of the thrust belt. This was responsible for the third stage of deformation characterized by thin-skinned NNW out-of-sequence thrusts developed in the westernmost sector. The total Andean shortening calculated in the area was 21-24 km (near 30%). The structure of the La Ramada fold and thrust belt was integrated into a crustal-scale cross-section at 32 degrees S latitude. Based on gravimetric models and surface geology, a crustal model is proposed for the Andes of Chile and Argentina. A shortening of 180 km was calculated between the Chile trench and the Sierra de Pie de Pale, This implies a mean deformation rate of 2.8 mm year(-1) during Cenozoic times. An initial crustal thickness of ca. 33 km was computed. A two-layer model with a middle detachment level is proposed to explain the spatial decoupling between maximum shortening at the surface and maximum crustal thickening. The upper layer was balanced based on surface structural information. The lower layer is interpreted to have been constructed by an imbricate thrust system controlled by the Mercedario rift master-shear and the Precordillera-Chilenia suture. (C) 2000 Elsevier Science B.V. All rights reserved.