Shaping of intraplate mountain patterns: The Cantabrian orocline legacy in Alpine Iberia

Author:

Fernández-Lozano J.1,Gutiérrez-Alonso G.23,Willingshofer E.4,Sokoutis D.45,de Vicente G.6,Cloetingh S.4

Affiliation:

1. Department of Earth Sciences and Physics of Condensed Matter, Faculty of Sciences, University of Cantabria, Avenida de los Castros s/n, 39007 Santander, Spain

2. Geology Department, Facultad de Ciencias, University of Salamanca, Plaza de la Merced s/n, 37008 Salamanca, Spain

3. Geology and Geography Department, Tomsk State University, Lenin Street 36, Tomsk 634050, Russian Federation

4. Department of Earth Sciences, Utrecht University, Budapestlaan 4, 3584 CD Utrecht, Netherlands

5. Department of Geosciences, University of Oslo, P.O. Box 1047 Blindern, N-0316 Oslo, Norway

6. Departamento de Geodinámica, Estratigrafía y Paleontología, and Institute of Geosciences (IGEO CSIC-UCM), Universidad Complutense de Madrid, c/ José Antonio Novais, no. 12, 28040 Madrid, Spain

Abstract

AbstractThe present-day topography in Iberia is related to geodynamic processes dealing with lithospheric-scale deformation. However, little attention has been paid to the role of inherited crustal- or lithospheric-scale structures involved in the recent observed large-scale topographic patterns. Whereas the analysis of brittle structures focuses on the evolution of Mesozoic sedimentary basins and their subsequent response to tectonic inversion, their contribution to mountain building has been underestimated. Large numbers of structures, from ductile to brittle, which affected the whole lithosphere, were developed during the evolution of the Cantabrian orocline (ca. 310–300 Ma). The contribution of these Paleozoic post-Variscan structures, together with lithospheric mantle evolution and replacement during orocline development in the Mesozoic and Cenozoic geological evolution of Iberia, remains unexplored. To explore the role of these inherited structures on the final configuration of topography during N-S Pyrenean shortening, we carried out a series of analogue experiments complemented by surface velocity field analyses. Our experiments indicate that strain was concentrated along preexisting crustal- to lithospheric-scale discontinuities, and they show several reactivation events marked by differences in the velocity vector field. Differences in fault displacement were also observed in the models depending upon preexisting fault trends. The obtained results may explain the different amount of displacement observed during the reactivation of some of the post-orocline structures in Iberia during the Cenozoic, indicating the key role of unveiled structures, which probably have accommodated most of the Alpine shortening.

Publisher

GeoScienceWorld

Subject

Geology

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