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Plate tectonics

Geology is the study of Earth’s crust and the processes that have shaped its surface throughout history. (Although geo - means “related to Earth,” astronomers and planetary scientists also talk about the geology of other planets.) Heat escaping from the interior provides energy for the formation of our planet’s mountains, valleys, volcanoes, and even the continents and ocean basins themselves. But not until the middle of the twentieth century did geologists succeed in understanding just how these landforms are created.

Plate tectonics is a theory that explains how slow motions within the mantle of Earth move large segments of the crust, resulting in a gradual “drifting” of the continents as well as the formation of mountains and other large-scale geological features. Plate tectonics is a concept as basic to geology as evolution by natural selection is to biology or gravity is to understanding the orbits of planets. Looking at it from a different perspective, plate tectonics is a mechanism for Earth to transport heat efficiently from the interior, where it has accumulated, out to space. It is a cooling system for the planet. All planets develop a heat transfer process as they evolve; mechanisms may differ from that on Earth as a result of chemical makeup and other constraints.

Earth’s crust and upper mantle (to a depth of about 60 kilometers) are divided into about a dozen tectonic plates that fit together like the pieces of a jigsaw puzzle ( [link] ). In some places, such as the Atlantic Ocean, the plates are moving apart; in others, such as off the western coast of South America, they are being forced together. The power to move the plates is provided by slow convection    of the mantle, a process by which heat escapes from the interior through the upward flow of warmer material and the slow sinking of cooler material. (Convection, in which energy is transported from a warm region, such as the interior of Earth, to a cooler region, such as the upper mantle, is a process we encounter often in astronomy—in stars as well as planets. It is also important in boiling water for coffee while studying for astronomy exams.)

Earth’s continental plates.

Diagram of Earth’s Continental Plates. The outlines of the various plates are drawn in red. The plate names are given in black. Subduction zones are shown as converging arrows, and rift zones are shown as diverging arrows. At far-left is the Pacific plate, with the San Andreas fault and East Pacific Rise labeled. Next, straddling the equator are the Cocos, Caribbean, and Nazca plates. North and to the east of these are the North and South American plates. Adjacent to the North American plate is the Eurasian plate, and next to the South American plate is the African Plate. The Mid-Atlantic ridge (rift zone) is the boundary of the American plates and the African and Eurasian plates. Between Eurasia and Africa is the Arabian plate. Below the eastern part of the Eurasian plate is the Australia-Indian plate (subduction zone). The African plate and the Australia-Indian plate are bounded by a rift zone. At far-right between the western Pacific plate and the eastern Eurasian plate is the Phillipine plate. Dominating the bottom of the illustration is the Antarctic plate, with the Pacific-Antarctic rise (rift zone), Atlantic-Indian rise, and the Southeast Indian Rise (rift zone) indicated.
This map shows the major plates into which the crust of Earth is divided. Arrows indicate the motion of the plates at average speeds of 4 to 5 centimeters per year, similar to the rate at which your hair grows.

As the plates slowly move, they bump into each other and cause dramatic changes in Earth’s crust over time. Four basic kinds of interactions between crustal plates are possible at their boundaries: (1) they can pull apart, (2) one plate can burrow under another, (3) they can slide alongside each other, or (4) they can jam together. Each of these activities is important in determining the geology of Earth.

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Source:  OpenStax, Astronomy. OpenStax CNX. Apr 12, 2017 Download for free at http://cnx.org/content/col11992/1.13
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