Éditeur(s) : HAL CCSD
Résumé : International audience
The Jaca basin is a thrust-sheet top basin transported southward andunderlain by basement and cover thrusts separated by a Triassic décollement.Basin-fill upper Cretaceous to lower Oligocene synorogenic sequencesrecord a southward depocenter migration, while growth stratadate a shift of deformation from the mid-Eocene in the N to the earlyMiocene in the S (S-Pyrenean front). However, the deep geometry andkinematic relationships between the cover and basement thrusts remainnon-consensual. We present a new structural and kinematic interpretationfor the eastern Jaca basin, based on subsurface structural maps andcross-sections constructed using industrial seismic reflection profiles.Raman Spectroscopy of Carbonaceous Material (RSCM), vitrinite reflectanceand apatite fission track (AFT) thermochronology data givefurther constraints for the restoration of the deformation and burialexhumationsequence. We define 3 main basement thrusts under thenorthern part of the basin, from N to S the Broto, Fiscal and Guargathrusts. The study also clarifies the deep structure of the cover thrustsand their links with these basement thrusts and those located more tothe north in the Axial Zone (AZ), which altogether define the timing ofthe basement thrust sequence as follows : the Lakoura-Eaux Chaudesthrust system (northern AZ) active up to the end Bartonian, the Gavarnie(central AZ) and Broto thrusts during the Priabonian-Rupelian andthe Fiscal and Guarga thrusts during the late Oligocene-early Miocene.AFT results in the basin fill and AZ date the exhumation of the basinto the late Oligocene-early Miocene, in relation to the Fiscal-Guargathrusting. AFT partial reset argues for a maximum burial < 6 km forthe base of the Eocene detrital sequence (Hecho Group turbidites). Bycontrast, RSCM and vitrinite thermometry at the same level indicatesTmax around 180°C, locally up to 240°C, attesting to a temperature anomalypossibly related to transient fluid circulation.
24 ème Réunion des sciences de la Terre 2014
Pau, France

insu-01080836
https://hal-insu.archives-ouvertes.fr/insu-01080836

Éditeur(s) : HAL CCSD Elsevier
Résumé : International audience
Orogenic wedges locally present chaotic tectonostratigraphic units that contain exotic blocks of various size, origin, age and lithology, embedded in a sedimentary matrix. The occurrence of ophiolitic blocks, sometimes huge, in such “mélanges” raises questions on (i) the mechanisms responsible for the incorporation of oceanic basement rocks into an accretionary wedge and (ii) the mechanisms allowing exhumation and redeposition of these exotic elements in “mélanges” during wedge growth.To address these questions, we present the results of a series of analogue experiments performed to characterize the processes and parameters responsible for accretion, exhumation and tectonosedimentary reworking of oceanic basement lithospheric fragments in an accretionary wedge.The experimental setup is designed to simulate the interaction between tectonics, erosion and sedimentation. Different configurations are applied to study the impact of various parameters, such as irregular oceanic floor due to structural inheritance, or the presence of layers with contrasted rheology that can affect deformation partitioning in the wedge (frontal accretion vs basal accretion) influencing its growth. Image correlation technique allows extracting instantaneous velocity field, and tracking of passive particles. By retrieving the particle paths determined from models, the pressure-temperature path of mélange units or elementary blocks can be discussed. The experimental results are then compared with observations from ophiolite-bearing mélanges in Taiwan (Lichi and Kenting mélanges) and Raman spectroscopy of carbonaceous material (RSCM) Thermometry data on rocks from the northern Apennines (Casanova mélange). A geological scenario is proposed following basic observations. The tectonic evolution of the retroside of doubly vergent accretionary wedges is mainly controlled by backthrusting and backfolding. The retro wedge is characterized by steep slopes that are prone to gravitational instabilities. It triggers submarine landslides inducing huge mass transfers. This erosion combined with backthrusting could favour exhumation of the ophiolitic fragments formerly accreted at the base of the wedge along the rough seafloor-sediments interface. Such an exhumed material can be reworked and deposited as debris- flows in proximal basins located at the foot of the retrowedge slope forming a tectono-sedimentary mélange. These syntectonic basins are continuously deformed and involved in prograding backthrusting-induced deformation.
ISSN: 0264-3707

hal-01395127
https://hal.archives-ouvertes.fr/hal-01395127
DOI : 10.1016/j.jog.2016.05.008

Éditeur(s) : HAL CCSD Elsevier
Résumé : International audience
Alpine Corsica consists of a stack of variably metamorphosed units of continental and Tethys-derived rocks. It represents an excellent example of high-pressure (HP) orogenic belt, such as the Western Alps, exposed over a small and accessible area. Compared to the Western Alps, the geology of Alpine Corsica is poorly unraveled. During the 1970s-80s, based on either lithostratigraphic or metamorphic field observations, various classifications of the belt have been proposed, but these classifications have been rarely matched together. Furthermore, through time, the internal complexity of large domains has been progressively left aside in the frame of large-scale geodynamic reconstructions. As a consequence, major open questions on the internal structure of the belt have remained unsolved. Apart from a few local studies, Alpine Corsica has not benefited of modern developments in petrology and basin research. This feature results in several uncertainties when combining lithostratigraphic and metamorphic patterns and, consequently, in the definition of an exhaustive architecture of the belt. In this paper we provide a review on the geology of Alpine Corsica, paying particular attention to the available lithostratigraphic and metamorphic classifications of the metamorphic terranes. These data are completed by a new and exhaustive metamorphic dataset obtained by means of thermometry based on Raman Spectroscopy of Carbonaceous Material (RSCM). This technique provides reliable insights on the peak temperature of the metamorphic history for CM-bearing metasediments. A detailed metamorphic characterization of metasediments, which have been previously largely ignored due to retrogression or to the lack of diagnostic mineralogy, is thus obtained and fruitfully coupled with the available lithostratigraphic data. Nine main tectono-metamorphic units are defined, from subgreenschist (ca. 280-300 °C) to the lawsonite-eclogite-facies (ca. 500-550 °C) condition. These units are homogeneous in metamorphism, laterally continuous and have characteristic lithostratigraphic features. This study also suggests a direct link between the pre-orogenic extensional setting and the present-day compressional structure of Alpine Corsica, indicating that large sections of subducted lithosphere were subducted and exhumed as coherent domains. These features provide important insight on the mechanism of stacking and exhumation of HP rocks, and make Alpine Corsica a unique reference for mountain-building processes in Tethyan-type orogens.
ISSN: 0012-8252

hal-00814433
https://hal.archives-ouvertes.fr/hal-00814433
DOI : 10.1016/j.earscirev.2012.10.003