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craton

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craton
NameCraton
CaptionSchematic cross-section of a craton showing its deep lithospheric root.

craton. A craton is an ancient, stable, and thick segment of the Earth's continental lithosphere that has survived the cycles of plate tectonics and supercontinent assembly and breakup over billions of years. These geological fortresses, often considered the continental nuclei, are characterized by a thick, cold, and buoyant lithospheric mantle root, known as a tectosphere, which extends deep into the asthenosphere. Their stability makes them remarkably resistant to deformation, in stark contrast to more active orogenic belts and rift valleys.

Definition and characteristics

The defining characteristic of a craton is its long-term stability, often dating back to the Archean Eon or early Proterozoic Eon. This stability is physically manifested in a thick, rigid lithosphere that can exceed 200 kilometers in depth, providing a buoyant foundation that shields the overlying crust from being recycled into the Earth's mantle. The crustal portion of a craton typically consists of a Precambrian crystalline basement (geology) of igneous and metamorphic rock, which is often overlain by a thin, relatively undeformed cover of sedimentary rock known as a platform (geology). Internally, cratons are seismically distinct, with high-velocity structures detected by techniques like seismic tomography, indicating their cold and depleted nature. The Kaapvaal Craton in southern Africa and the Siberian Craton beneath much of Russia exemplify these enduring features.

Formation and evolution

Cratons are thought to have formed primarily during the Archean Eon through processes distinct from modern plate tectonics. Early theories involved the amalgamation of microcontinents and volcanic island arcs through intense magmatic and tectonic activity. A key process was likely the extraction of large volumes of komatiite, a high-temperature mantle plume-derived magma, which left behind a residue of buoyant, depleted peridotite that formed the strong lithospheric root. Over the eons, this mantle root underwent further strengthening through metasomatism and the incorporation of minerals like diamond, as sampled by kimberlite eruptions from deep within the Earth's mantle. Subsequent events, such as the Pan-African orogeny or the assembly of Pangaea, could weld younger terrains to these ancient cores without destroying them, as seen with the Amazonian Craton in South America.

Types and examples

Cratons are broadly classified into two types based on the age of their basement rocks. An Archaean craton is one where the crystalline basement formed during the Archean Eon, such as the Yilgarn Craton in Western Australia and the Superior Craton, which forms the core of the Canadian Shield. A Proterozoic craton has a basement primarily formed during the Proterozoic Eon, like the Saharan Metacraton in North Africa. Geographically, major cratons include the East European Craton underlying much of Baltic and Eastern Europe, the North China Craton, and the Dharwar Craton in India. Some, like the Wyoming Craton, are partially buried by younger Phanerozoic strata. The stability of these regions is often interrupted by narrow, mobile belts like the Namaqua-Natal Belt in southern Africa.

Economic importance

The exceptional stability and ancient geology of cratons make them premier hosts for a variety of world-class mineral deposits. They are the primary source of diamond, which forms under extreme pressure in the deep cratonic root and is brought to the surface by volatile-rich kimberlite and lamproite pipes, famously exploited in the Kimberley region of the Kaapvaal Craton and the Mir mine in the Siberian Craton. Cratons also contain major deposits of gold, particularly in greenstone belts like those in the Superior Craton's Abitibi greenstone belt, and vast formations of banded iron formation, which are the foundation of global iron ore mining in regions such as the Hamersley Basin on the Pilbara Craton. Additionally, they host significant resources of nickel, copper, and platinum group elements.

Cratons and plate tectonics

Within the framework of plate tectonics, cratons act as the rigid, interior cores of continental plates. Their profound buoyancy and strength mean they are rarely subducted, though they can be rifted at their margins, as seen with the separation of the Brazilian Shield from the West African Craton during the breakup of Gondwana. The deep roots of cratons can influence mantle convection patterns and may deflect or anchor the motion of overlying plates. However, some cratons have experienced significant modification or destruction through processes like mantle plume impingement, which may have triggered the loss of the root beneath the North China Craton, or through delamination during continental collision, as hypothesized for parts of the Tanzania Craton. Their long-term survival remains a key area of study in understanding Earth's dynamic history.

Category:Geology Category:Tectonics Category:Continental crust