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An overview of plate tectonics, a geological theory explaining the earth's lithosphere as a collection of rigid plates with various types of boundaries. Learn about plate generation, deformation, and the three main types of plate boundaries: divergent, convergent, and conservative.
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Dr. Gavin Bell The basic concept of plate tectonics is that the Earth’s lithosphere is divided into a small number of nearly rigid plates (there are seven major plates and several more minor ones). Most of the deformation – stretching, folding and shearing – in the lithosphere takes place near the boundaries of the plates. Deformation well inside the plate boundaries is much smaller than deformations occurring at or near boundaries. A seismicity map neatly outlines many of the plate boundaries since most volcanism and earthquake activity occurs in regions of strong lithospheric deformation. The main points are: The generation of new plate material occurs by seafloor spreading, where new oceanic lithosphere is generated along active mid-ocean ridges. Once generated, the new ocean lithosphere forms part of a rigid plate which may or may not include continental material. The surface area of the Earth remains constant. Consequently, seafloor spreading must be balanced by the consumption of plate material elsewhere. The rigidity of the lithospheric plates means that they can transmit stress over great distances without buckling. The relative motion between plates is taken up almost entirely along plate boundaries. The continents can be considered as “rafts” of less dense material which remain on the surface, while the denser oceanic lithosphere is subducted beneath other oceanic or continental lithosphere. A single tectonic plate can comprise both continental and oceanic lithosphere, but the latter is created or destroyed far more easily.
Summary of tectonic activity at constructive and destructive plate boundaries (from Earth , Press and Siever). Boundaries between plates are of three basic types: