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Geological Society, London, Special Publications; 2002; v. 199; p. 65-90;
DOI: 10.1144/GSL.SP.2002.199.01.04
© 2002 Geological Society of London

Geophysical and Petrological Constraints on Archaean Lithosphere

The development of lithospheric keels beneath the earliest continents: time constraints using PGE and Re-Os isotope systematics

D. G. Pearson1, G. J. Irvine1, R. W. Carlson2, M. G. Kopylova3 & D. A. Ionov4

1 Department of Geological Sciences, Durham University, South Road, Durham DH1 3LE, UK d.g.pearson{at}durham.ac.uk
2 Department of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad Branch Road, NW, Washington DC 20015, USA
3 Geological Sciences Division, Earth and Ocean Sciences, The University of British Columbia, 6339 Stores Road, Vancouver, B.C. V6T 1R9, Canada
4 Department of Earth and Environmental Sciences, Université Libre de Bruxelles, 50 Roosevelt av., B-1050 Brussels, Belgium

Continued studies of xenolith suites found in kimberlites on and around the Kaapvaal Craton, together with those from newly discovered localities on other cratons, are providing new insights into the generation and evolution of the Earth’s oldest continents. Comparison of modal abundance data with melt depletion models, together with trace element and isotope systematics in Kaapvaal low-temperature peridotites, suggest that much or all of the diopside and garnet in these rocks may have formed significantly after initial melt depletion. The Re-Os isotope system has been instrumental in providing an improved understanding of the timing of the formation of cratonic lithospheric keels. New studies that focus on carefully selected whole-rock peridotites and use combined platinum group element (PGE) and Re-Os isotope analysis provide better constraints on the significance of Re-Os model ages. The large database of Re-Os isotope analyses for peridotites for the Kaapvaal Craton indicate formation of significant amounts of lithospheric mantle in Neoarchaean time, associated with voluminous mafic magmatism. Formation of lithospheric mantle in Neoarchean time (3.0–2.5 Ga) follows the cessation of major crustal differentiation events at c. 3.1 Ga and marks the onset of craton stabilization. Some lithospheric mantle was produced in Palaeo- to Mesoarchaean time (3.8–3.0 Ga) in southern Africa, which preserved ancient crustal fragments. Large-scale preservation of Archaean continental masses was effective only after the formation of substantial, buoyant, rigid, deep lithospheric keels and their stabilization in Neoarchean time. Formation of lithospheric mantle beneath the surrounding Proterozoic crustal regions occurred in Mesoproterozoic time, with lower degrees of mantle melting than associated with the cratonic peridotites. This circum-cratonic mantle is of similar age to the oldest overlying crust and has been coupled to the margins of the craton since its formation. Major magmatic events, some coincident with the formation of circumcratonic mantle, added new lithosphere to the Kaapvaal mantle root but failed to destroy it. The mechanically strong, buoyant lithospheric keels beneath cratons protect their crust from subduction and recycling over 3 Ga time periods.





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