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Journal of Petrology Advance Access originally published online on July 4, 2008
Journal of Petrology 2009 50(7):1185-1204; doi:10.1093/petrology/egn033
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© The Author 2008. Published by Oxford University Press. All rights reserved. For Permissions, please e-mail: journals.permissions@oxfordjournals.org

The Composition and Evolution of Lithospheric Mantle: a Re-evaluation and its Tectonic Implications

W. L. Griffin1,*, Suzanne Y. O’Reilly1, J. C. Afonso1,2 and G. C. Begg1,3

1Arc National Key Centre for Geochemical Evolution and Metallogeny of Continents, Department of Earth and Planetary Sciences, Macquarie University, N. S. W. 2109, Australia
2GDL, Institute of Earth Sciences ‘J. Almera’, C.S.I.C., Lluls Solé I SabarÍs S/N, 08028, Barcelona, Spain
3Minerals Targeting International, West Perth, W.A. 6005, Australia

RECEIVED JANUARY 27, 2008; ACCEPTED JUNE 12, 2008


   Abstract

The composition of the subcontinental lithospheric mantle (SCLM) is broadly related to the tectonothermal age of the overlying crust, suggesting a secular change in SCLM-forming processes. Most estimated compositions of Archean SCLM, based on well-studied suites of xenoliths and xenocrysts, are depleted garnet lherzolites with high orthopyroxene/olivine. However, these compositions make it difficult to account for the high shear-wave velocities measured in the cores of large cratons, and predict deeper geoid anomalies and higher elevations than are observed in most cratons. Global and regional seismic tomography indicates that most cratonic xenolith suites represent material from the lower-velocity margins of lithospheric blocks. This implies that previous compositional estimates are strongly biased toward metasomatized material. We suggest that most Archean SCLM originally consisted of highly depleted dunites/harzburgites, similar to the Archean orogenic massifs of western Norway. Incorporation of such rocks in the cold upper parts of the cratonic SCLM satisfies the seismic and gravity data, suggesting that large volumes of these rocks are preserved in the cores of cratons, but are poorly sampled by volcanic rocks. The roots of most Proterozoic shields probably consist of refertilized Archean SCLM; the juvenile SCLM beneath Proterozoic and Phanerozoic mobile belts reflects only moderate depletion of Primitive Mantle compositions. Rather than a gradual evolution in SCLM-forming processes, we suggest a sharp dichotomy between Archean and younger tectonic regimes. The differences in buoyancy and viscosity between these two types of SCLM have played a major role in the construction, preservation and recycling of continental crust. If originally Archean SCLM is more widespread than currently recognized, models of crustal growth rates and recycling may need to be revised.

KEY WORDS: subcontinental lithospheric mantle; mantle evolution; seismic tomography; mantle metasomatism; Archean lithosphere


*Corresponding author. Telephone: +61 2 9850 8954. Fax: +61 2 9850 8943. E-mail: wgriffin{at}els.mq.edu.au


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