The plate tectonics (initially called continental drift ) is the model current inner working of the Ground. It is the expression on the surface of the Convection which is held in the terrestrial coat.
The Lithosphere, layer external of the Ground is cut out in rigid plates which float and move on the Asthénosphère, more ductile. The first concepts, stammered as of the 18th century, were scientifically formulated in 1912 by the German climatologist Alfred Wegener starting from considerations cartographic, structural, paleontological and paleoenvironmental.
It is admitted now that the tectonic plates are carried by the movements of the subjacent coat asthenospheric and undergo interactions whose three principal types are:
the divergence : of a movement moving away two plates one is said from the other, letting the coat go up between them. Their divergent border corresponds to a oceanic wrinkle or dorsal, place of creation of oceanic Lithosphère and theater of intense volcanicity. Volcanicity on the level of the dorsals is generally basaltic, with a tholeiitic Géochimie . It is through this movement that creates for itself the crust lithospheric (rigid layer located at the top of the higher coat):
the convergence : of a movement bringing closer two plates one is said to the other, thus compensating for the oceanic expansion in other zones of the sphere. Three types of convergent border of plates adapt the bringing together:
the transcurrence : horizontal slip of two plates is said, one at side and along the other.
With these three types of interaction the three big families with Faille S are associated:
a normal Faille is divergent (extensive);
The origin of the force which makes the plates mobile is discussed: it can be related on the constraint shearing between the crust and the asthenosphere (related to the importance of the coupling between the two), to the weight of the crust subductante (which “draws” all the plate) or with pushed with the wrinkle (the weight of the young crust in top of the wrinkle “pushes” all the plate). These possibilities are not exclusive, but the relative contributions in the movement are very discussed and depend on the studies.
The plate tectonics is perfectly valid for the oceanic plates (or for the oceanic parts of the mixed plates). Indeed, the oceanic plates are thin and rigid; their limits are very clear (médio-oceanic Ride, Faille S transforming or zones of Subduction). On the other hand, the continental plates are much thicker and less rigid. The limits of plates are thus much fuzzier, and one can regard as limit the paleogeographic joining (the old ocean), or the zone which currently becomes deformed (in the cases of the the Himalayas - Tibet, the difference is of several thousands of km). De more, this lack of rigidity induces the presence of a multitude of " blocs" or of " microplaques" , more or less independent. The mosaic in the Mediterranean in is an good example, with a multitude of systems in extension (Tyrrhenian Sea, Mer of Alboran, Aegean Sea) in a compressive context (bringing together of the African and European plates). The model of plate tectonics finds its limits here, and certain model can better explain certain structures without the plate tectonics (in the East of the plate Tibetan, for example).
The list of the current plates is, alphabetically (smaller units exist; they are called “blocks” or “microplaques”):
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