Reproducing geological
processes in the laboratory has been of a great interest among scientists for
years. Laboratory experiments, scaled in time and space, may help us to improve
our knowledge of some geological processes that are impossible to study in nature.
For example, we may reproduce large tectonic processes and study their evolution
in the order of millions of years.
This study is based on laboratory
simulations of a specific tectonic process, called double polarity subduction. In
a subduction system, which occurs on convergent margins of plate boundaries,
two plates collide and one moves under the other (overriding plate). In the
Mediterranean Vergés and Fernàndez (2012) hypothesized the presence of two
subductions retreating in opposite directions since 30 million years.
Our experiments consist in
simulating in the laboratory the evolution of a double polarity subduction
process, but without taking into account the overriding plate. We realized the
experiments in a square Plexiglas tank full of high viscous syrup, representing
the mantle. The setup contains two oceanic plates (Figure 1), made with silicone putty,
and subduction is started by deflecting manually the leading edge of the
plates. Each centimeter corresponds to 60 km. The experiments are monitored
with two cameras that take photographs in time intervals of 30 seconds from the
top of the experiment and from an oblique position, so we can study
the system in function of time. Different setups were designed to test the
influence of two variables in the system: i) the width of the plates and ii)
the lateral distance between the two subducting plates.
The evolution of the models
is characterized by three different phases: (1) initial stage of subduction,
corresponding to the evolution of the system until the plates reach the base of
the model box; (2) approaching trenches, until they pass each other; (3)
diverging trenches, until the retreating of plates is over.
Our results indicate
that velocities of the trench (marking the position at which the subducting
plate begins to descend) increase during phase 2 and then decrease during phase
3. We explain this trendline as due to the interaction of the mantle flow
induced by both plates in the contact area. When plates are wider the same
process is active. Nevertheless, when lateral distance between plates increases
we do not observe any change of the velocities during the evolution and the
interaction of the two plates become negligible when they are 10 cm spaced (600
km in nature).
This work is supervised by Manel Fernandez (ICTJA-CSIC) and Sergio Zlotnik (UPC, Barcelona). The experiments have been carried out in collaboration with Ágnes Király, Francesca Funiciello and Claudio Faccenna from the Laboratory of Experimental Tectonics (Roma Tre University, Italy). This study is part of the Project “Testing the geodynamic evolution of the Western Mediterranean (We-Me) financed by CSIC (PIE-CSIC-201330E111). We also thank to the project AECT-2016-1-0002 of the Barcelona Supercomputing center (BSC-CNS).
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