Concept information
Terme préférentiel
plate tectonic
Définition
- Plate tectonics (from Latin tectonicus, from Ancient Greek (tektonikós) 'pertaining to building') is the scientific theory that Earth's lithosphere comprises a number of large tectonic plates, which have been slowly moving since about 3.4 billion years ago. The model builds on the concept of continental drift, an idea developed during the first decades of the 20th century. Plate tectonics came to be accepted by geoscientists after seafloor spreading was validated in the mid-to-late 1960s. Earth's lithosphere, the rigid outer shell of the planet including the crust and upper mantle, is fractured into seven or eight major plates (depending on how they are defined) and many minor plates or "platelets". Tectonic plates are relatively rigid and float across the ductile asthenosphere beneath. Lateral density variations in the mantle result in convection currents, the slow creeping motion of Earth's solid mantle. (Adapted from: https://en.wikipedia.org/wiki/Plate_tectonics)
Concept générique
Traductions
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français
URI
http://data.loterre.fr/ark:/67375/QX8-H2V21N7T-3
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