2013
DOI: 10.1146/annurev-earth-050212-124208
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Initiation and Evolution of Plate Tectonics on Earth: Theories and Observations

Abstract: The inception of plate tectonics on Earth and its subsequent evolution are discussed on the basis of theoretical considerations and observational constraints. The likelihood of plate tectonics in the past depends on what mechanism is responsible for the relatively constant surface heat flux that is indicated by the likely thermal history of Earth. The continuous operation of plate tectonics throughout Earth's history is possible if, for example, the strength of convective stress in the mantle is affected by th… Show more

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Cited by 431 publications
(293 citation statements)
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“…A gradual change from shallow subduction in the Archaean, to steep subduction after 1 Ga, is compatible with the record of metamorphic gradients (Brown 2014;Sizova et al 2014). As discussed by Korenaga (2013), however, the role of water in the mantle is not always accounted for in numerical models, and if dry enough, a hot mantle may also allow for slab subduction.…”
Section: The Onset Of Plate Tectonicssupporting
confidence: 54%
“…A gradual change from shallow subduction in the Archaean, to steep subduction after 1 Ga, is compatible with the record of metamorphic gradients (Brown 2014;Sizova et al 2014). As discussed by Korenaga (2013), however, the role of water in the mantle is not always accounted for in numerical models, and if dry enough, a hot mantle may also allow for slab subduction.…”
Section: The Onset Of Plate Tectonicssupporting
confidence: 54%
“…Korenaga, 2013, and references therein). Davies (1992;2006) argued that the presence of early depleted mantle would have resulted in oceanic crust thinner than modern oceanic crust (< 3 km on average), and a thinner oceanic crust would increase the viability of subduction.…”
Section: Implications For Crust-mantle Interactions Through Timementioning
confidence: 99%
“…Moreover, most of the cratons became stable during Archean (2500-3750 Ma) 53,54 , when mantle heat flux was higher to support more vigorous convection 55 . There could be two end-member solutions to this problem 56 : (a) either cratons could resist deformation, or (b) they were avoided by the deforming agent (like mantle convection).…”
Section: Stability Of Cratonsmentioning
confidence: 99%