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Plate tectonics is the scientific theory that Earth’s lithosphere—the rigid outer shell made of the crust and upper mantle—is broken into large tectonic plates (plus smaller platelets) that move slowly over geologic time. Plate motion is driven by processes in the mantle and is expressed at plate boundaries, where relative movement produces three main boundary types: convergent (plates move toward each other, often forming subduction zones or collisions), divergent (plates move apart, creating new crust via seafloor spreading), and transform (plates slide past each other along transform faults). These boundary interactions are strongly linked to earthquakes, volcanism, mountain building, and the formation of ocean trenches. The lithosphere rides on the underlying asthenosphere, which is hotter and flows more easily. Heat transfer and mechanical behavior differ between these layers: the lithosphere is cooler and more rigid, while the asthenosphere is hotter and can deform ductilely. Tectonic plates include oceanic lithosphere (typically thinner, denser, and formed at mid-ocean ridges) and thicker continental lithosphere (less dense). Oceanic crust generally forms at spreading centers, cools and thickens with age, and is later consumed at subduction zones, balancing creation of new crust and helping maintain Earth’s overall surface area in a “conveyor belt” cycle. Evidence supporting plate tectonics included validation of seafloor spreading in the mid- to late 1960s, along with observations such as mid-ocean ridges, oceanic crustal composition and thickness, and patterns of earthquake activity (e.g., Wadati–Benioff zones) that trace subducting slabs. Mantle convection and related mantle dynamics—along with gravity-driven effects like slab pull and ridge push—are key proposed mechanisms for plate motion, while other ideas (such as plume or surge tectonics) have been debated as additional or modifying influences.
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