Formation of Archaean continental lithosphere and its diamonds: the root of the problem

被引:244
作者
Pearson, D. G. [1 ]
Wittig, N. [1 ]
机构
[1] Univ Durham, Dept Earth Sci, No Ctr Isotop & Elemental Tracing, Durham DH1 4QE, England
关键词
D O I
10.1144/0016-76492008-003
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Cratonic lithospheric mantle plays an integral role in defining the physical behaviour of ancient continents and their mineral potential. Bulk compositional data show that modern-day melting residues from a variety of tectonic settings can be as depleted in Al and Ca as cratonic peridotites. Cratonic peridotites are strongly affected by secondary introduction of pyroxenes and garnet such that the extent and depth of melting cannot be reliably determined. Olivine compositions are probably the most reliable tracer of the original melting process and indicate that typical cratonic peridotites have: experienced 40% or more melt extraction. Homogeneous levels of depletion indicated by olivine compositions, combined with mildly incompatible trace element evidence, indicate that melting took place at shallow depths, dominantly in the spinel stability field. Consideration of melt production models shows that shallow (<3 GPa) anhydrous melting is not capable of producing residues dominated by large degrees of melt extraction. Instead, a critical role for water is indicated, implicating the formation of cratonic peridotites within Archaean subduction zones. This melting occurred in the Ncoarchaean in some cratonic blocks, initially forming dunitic residues that are still evident ill the xenolith inventory of some cratons. Release and migration up-section of siliceous melt produced during orthopyroxene breakdown metasomatizes the proto-lithospheric via re-enrichment in orthopyroxene crystallizing from this hydrous Si-rich melt, forming the variably orthopyroxene-rich refractory harzburgites typical of most cratonic roots. Melting in Archaean subduction zones is followed by subduction stacking to form the cratonic root. Gravitational forces may then be responsible for the loss of imbricated matic crust during periods of transient thermal and physical disturbances prior to final long-term tectonic stability. Most diamonds form in the base of these cratonic roots during pulses of thermal or tectonic activity, initially during root construction and subsequently associated with large-scale regional lithospheric events that may be correlated to pulses ill global mantle dynamic evolution.
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收藏
页码:895 / 914
页数:20
相关论文
共 131 条
[111]   The significance of U-Pb zircon dates in lower crustal xenoliths from the southwestern margin of the Kaapvaal craton: southern Africa [J].
Schmitz, MD ;
Bowring, SA .
CHEMICAL GEOLOGY, 2001, 172 (1-2) :59-76
[112]   CONSTRAINTS ON THE ABUNDANCE OF ECLOGITE IN THE UPPER MANTLE [J].
SCHULZE, DJ .
JOURNAL OF GEOPHYSICAL RESEARCH-SOLID EARTH AND PLANETS, 1989, 94 (B4) :4205-4212
[113]   CALCIUM ANOMALIES IN THE MANTLE AND A SUBDUCTED METASERPENTINITE ORIGIN FOR DIAMONDS [J].
SCHULZE, DJ .
NATURE, 1986, 319 (6053) :483-485
[114]  
Shimizu N, 1997, GEOL GEOFIZ+, V38, P194
[115]   Diamond genesis, seismic structure, and evolution of the Kaapvaal-Zimbabwe craton [J].
Shirey, SB ;
Harris, JW ;
Richardson, SH ;
Fouch, MJ ;
James, DE ;
Cartigny, P ;
Deines, P ;
Viljoen, F .
SCIENCE, 2002, 297 (5587) :1683-1686
[116]   Archean emplacement of eclogitic components into the lithospheric mantle during formation of the Kaapvaal Craton [J].
Shirey, SB ;
Carlson, RW ;
Richardson, SH ;
Menzies, A ;
Gurney, JJ ;
Pearson, DG ;
Harris, JW ;
Wiechert, U .
GEOPHYSICAL RESEARCH LETTERS, 2001, 28 (13) :2509-2512
[117]   Ultra-refractory domains in the oceanic mantle lithosphere sampled as mantle xenoliths at ocean islands [J].
Simon, Nina S. C. ;
Neumann, Else-Ragnhild ;
Bonadiman, Costanza ;
Coltorti, Massimo ;
Delpech, Guillaume ;
Gregoire, Michel ;
Widom, Elisabeth .
JOURNAL OF PETROLOGY, 2008, 49 (06) :1223-1251
[118]   The origin of garnet and clinopyroxene in "depleted" Kaapvaal peridotites [J].
Simon, NSC ;
Irvine, GJ ;
Davies, GR ;
Pearson, DG ;
Carlson, RW .
LITHOS, 2003, 71 (2-4) :289-322
[119]  
SMITH CB, 2008, 9 INT KIMB C FRANKF
[120]   The origin of cratonic diamonds - Constraints from mineral inclusions [J].
Stachel, T. ;
Harris, J. W. .
ORE GEOLOGY REVIEWS, 2008, 34 (1-2) :5-32