Abstract

AbstractThe South Pyrenean triangle zone represents the southernmost front of the Pyrenees at its central portion deforming the Upper Eocene‐Miocene Ebro Basin deposits. Two main structures characterize its western termination, the Barbastro anticline and the San Román backthrust, which detached on the Barbastro Formation (and lateral equivalents), an Upper Eocene‐Lower Oligocene syntectonic evaporite‐rich formation that acted as a multidetachment unit. Northward, the south directed Pyrenean thrust unit (i.e., Gavarnie‐Sierras thrust sheet) detached along the Middle‐Upper Triassic evaporitic rocks to finally ramp up and glide along the same Upper Eocene‐Lower Oligocene multidetachment unit. A multidisciplinary approach allowed constructing a detailed structural and stratigraphic model of the study area. The workflow consisted of (1) constraining the geometry and structural architecture based on surface geology, interpretation of seismic lines (>900 km), and wells and (2) obtaining the 3‐D density distribution of the multidetachment unit using gravity stochastic inversion (more than 7,000 gravity stations and 1,500 density data). The geometry of the sole thrust of the Gavarnie‐Sierras thrust sheet was controlled by the distribution of the evaporite‐rich units of the Barbastro Fm. Weak detachments promoted thrust salient formation and thrust flat geometries. The western termination of the South Pyrenean triangle zone is defined as a westward transition from a ramp‐dominated and multiple triangle zone to a detachment‐dominated one. Its geometry, kinematics, and location were controlled by the heterogeneous lithology of the Barbastro Fm. and its basal, halite‐based detachment southern pinch‐out.

Highlights

  • The occurrence of multiple detachments impacts the style of deformation in fold‐and‐thrust belts (e.g., Bonini, 2001; Cobbold et al, 2009; Cobbold & Rodrigues, 2007; Couzens‐Schultz et al, 2003)

  • Two main structures characterize its western termination, the Barbastro anticline and the San Román backthrust, which detached on the Barbastro Formation, an Upper Eocene‐Lower Oligocene syntectonic evaporite‐rich formation that acted as a multidetachment unit

  • A combined and integrated workflow including the interpretation of seismic reflection profiles supported by surface geology and exploration well data together with the interpretation of the gravity anomalies and 3‐D stochastic inversion has proven to be a powerful approach to study deformed multidetachment evaporitic units and the western termination of the South Pyrenean triangle zone

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Summary

Introduction

The occurrence of multiple detachments (i.e., a stratigraphic pile involving two or more décollement units) impacts the style of deformation in fold‐and‐thrust belts (e.g., Bonini, 2001; Cobbold et al, 2009; Cobbold & Rodrigues, 2007; Couzens‐Schultz et al, 2003). The geometry, orientation and extent of the South Pyrenean triangle zone vary along strike, controlled by the thickness and distribution of the involved foreland syntectonic evaporitic units (Sans et al, 1996; Figure 2a). These units were deposited in the Ebro foreland basin, in marine and lacustrine areas laterally related to alluvial systems sourced in northern struc-. The western sector of the South Pyrenean triangle zone is mainly characterized by a continuous structure whose geometry changes along strike, the Barbastro anticline (Gil & Jurado, 1998; Martínez‐Peña & Pocoví, 1988; Pardo & Villena, 1979; Riba et al, 1983; Sans, 2003; Senz & Zamorano, 1992). We discuss the kinematic and mechanical implications of the new definition of the Barbastro anticline structure

Geological Setting
Stratigraphy
The Barbastro Anticline and the San Román Backthrust
Data and Methods
Seismic Reflection Profiles and Well Data
Time‐to‐Depth Conversion and 3‐D Reconstruction of the Study Area
Bouguer and Residual Gravity Anomaly Map
Seismic Stratigraphy
Main Structural Features in Map View and 3‐D
The Western Termination of the South Pyrenean Triangle Zone
The South Pyrenean Sole Thrust and the Gavarnie‐Sierras Thrust Sheet
Gravity Inversion
Discussion
Findings
Conclusions
Data Availability Statement
Full Text
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