Estimating the paleo-elevation and isostatic rebound of the Ebro Basin since its drainage opening.
The animation to the right shows the calculated paleotopography of the Ebro basin since the time of drainage opening (endorheic-exorheic transition) until today. Blue lines indicate isostatic rebound (meters) in response to sediment removal by erosion. Lower panel shows a section along the dated places located in red.
Drainage evolution of the Ebro Basin, TISC model
The Ebro foreland basin (Pyrenees, NE Iberia) started forming about 65 million years ago, during the Palaeocene, as a result of the tectonic collision and subduction of the Iberian plate underneath the European plate. The basin became landlocked in late Eocene (37 Ma) by the Pyrenees, the Catalan Coastal Ranges (CCR) and the Iberian Range, and was subsequently filled with alluvial, fluvial and lacustrine sediments. During the Miocene, the Catalan Coastal Ranges underwent a tectonic extension that opened the Western Mediterranean. Although the topographic barrier constituted by the CCR was significantly reduced, the Ebro Basin remained closed at least until late Miocene times, when the endorheic fluvial system opened through the present Ebro River to the Mediterranean initiating the formation of the delta.
The causes for this major drainage changes are the interplay between erosion and climatic processes, since there is no evidence for tectonism coeval in space and time with the breakthrough of the Ebro River across the CCR. Accerelated CCR erosion due to the lowering of the sea level in the Mediterranean during the Messinian Salinity Crisis had been proposed as a possible triggering mechanism, but regional isostatic behaviour of the lithosphere cannot be dismissed, since it controls the vertical movements during both crustal compression and extension.
We found that basin overfilling with sediments and the changes in the hydrological balance in terms of precipitation/evaporation (which controlled the water level in the closed basin) were equally relevant for the final overspilling of the basin. We linked quantitative approaches to these processes in a 3D numerical model of drainage evolution constrained by well logs, geological cross sections and fission track data.
The models shown here and in the publications are the result of developing and using the software TISC to quantitatively relate lithospheric, crustal and surface processes. The numerical model links quantitatively the drainage evolution with the tectonic evolution, using as a constraint the erosion deduced from isotopic composition and the sediment accumulation dferived from seismic and borehole surveys.
Note that the overspill of the lacustrine basin is predicted at 10 Myr before present, approximately coinciding with the youngest lacustrine sediments found in the basin.
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