Plate Tectonics

Overview

The theory of plate tectonics explains that the majority of Earth's geological features—from mountain ranges to ocean trenches—result from interactions between slabs of rock that make up Earth's outer shell. The slabs—collectively called tectonic plates—vary in size, composition, and movement, and have been dragged by convection currents, or continuous circular flows of material, in Earth's mantle for at least 3 billion years.

The theory began with rock, fossil, and climatic records suggesting that all land was once part of a single, interconnected supercontinent that broke apart. Decades later, measurements of the seafloor suggested that it steadily moved away from mid-ocean ridges—vast underwater mountain ranges with near-continuous volcanic activity. These movements cause oceanic plates to push into continental plates, resulting in earthquakes and volcanoes as the denser oceanic plate sinks beneath the continental plate and forms ocean trenches.

Mapping the locations of these and other geological features has enabled scientists to outline tectonic plates, identify types of plate boundaries, and model Earth's surface history.

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