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Archean Magmatism and Crustal Thickening

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TLDR
This article showed that the Archean crust closely approached its present-day thickness before or during emplacement of Archean granitic rocks and that the crust has not significantly changed in thickness since that time.
Abstract
Exposed stratigraphic thicknesses in Archean greenstone belts, high P-T mineral assemblages in Archean granulite-facies terranes, and K, Rb, and Sr geochemical polarity indices in Archean volcanic rocks suggest that large portions of the Archean crust were ≥25 km in thickness, and corresponding depths to subduction zone were ≥85 km prior to the emplacement of widespread Archean granitic rocks at 2.5 to 3.0 b.y. The polarity indices also suggest that the crust thickened to ≳30 km during emplacement of Archean granite. Compositional data suggest that at least some of the granitic rocks are not intrusive equivalents of greenstone volcanic rocks (at the same silica level). The thickness and seismic velocity distribution in the present crust do not appreciably change as a function of mean crustal age from terranes ≲225 m.y. to those >2,500 m.y. in age. A decrease in the range of crustal thickness with age is observed, however, probably reflecting an increasing degree of cratonization with age. Most data suggest that the Archean crust closely approached its present-day thickness before or during emplacement of Archean granitic rocks and that the crust has not significantly changed in thickness since that time.

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Journal ArticleDOI

Phanerozoic addition rates to the continental crust and crustal growth

Arthur Reymer, +1 more
- 01 Feb 1984 - 
TL;DR: In this paper, the authors used seismic profiles through magmatic arcs to measure the crustal volumes added during the active lifespans of the arcs and deduced a worldwide addition rate of 1.65 km³ a−1 after adding other contributions to the formation of the continental crust, e.g., from hot spot volcanism.
Journal ArticleDOI

The persistent myth of crustal growth

TL;DR: From the extraterrestrial telescopic, space probe, meteorite and returned sample studies of planetary evolution, and terrestrial evidence for early differentiation of core and fluid spheres and continental crust, the authors feel the conclusion is inescapable that large terrestrial planets of our solar system underwent essentially immediate differentiation into relatively constant volume core, depleted mantle, enriched crust and fluid reservoirs.
Journal ArticleDOI

Geochemical Constraints on the Growth of the Continental Crust

TL;DR: In this paper, it was shown that the Archean upper crust was considerably more mafic than the present-day upper crust, and that if there have been any additions to the post-Archean crust, they must have had similar composition to the upper crust itself.
Journal ArticleDOI

Hydrothermal Plumes and the Delivery of Iron to Banded Iron Formation

TL;DR: Most of the iron in banded iron formation (BIF) was deposited during the period 2.7-1.8 Ga as mentioned in this paper and peak deposition occurred between 2.4-2.3 Ga.
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