Page 381 - Global Tectonics
P. 381

364   CHAPTER 11



           (Condie, 2000). On the basis of available data, Condie                PRIMITIVE MANTLE
                                                          4
                                                                                 (=ASTHENOSPHERE)
           (2005b) concluded that 39% of the continental crust                E. China
           formed in the Archean, 31% in the Early Proterozoic,   YOUNGER    Vitim  +
           12% in the Middle–Late Proterozoic, and 18% in the        Phanerozoic    + +  Zabargad
                                                          3          Spinel
           Phanerozoic.                                              Peridotite     PHANEROZOIC
             Two of the most important mechanisms of Late         European  +
           Archean and Early Proterozoic continental growth and   % CaO  2  Massifs  +  PROTEROZOIC
           cratonic root evolution were magma addition (Section         +  S.Australia  + Xenolith
           9.8) and terrane accretion (Section 10.6). Several authors   Kaapvaal       averages
           (e.g. Condie, 1998; Wyman & Kerrich, 2002) have sug-  1  +                 Gnt-SCLM
                                                                         ARCHEAN       Archean
           gested that the ascent of buoyant mafic material in                          Proterozoic

           mantle plumes may have initiated crust formation and                        Phanerozoic
                                                          0

           may have either initiated or modified root formation   0  1   2     3      4     5
           during periods of rapid net growth (Section 11.3.3).             % Al 2 O 3
           Schmitz et al. (2004) linked the formation and stabiliza-
                                                        Fig. 11.14 CaO-Al 2 O 3  plot showing the range of
           tion of the Archean Kaapvaal craton in South Africa to
                                                        subcontinental lithospheric mantle (SCLM) compositions
           subduction, arc magmatism, and terrane accretion at
                                                        for selected cratons that have been matched with ages
           2.9 Ga. In this and most of the other cratons, isotopic
                                                        of the youngest tectonothermal events in the overlying
           ages from mantle xenoliths and various crustal assem-  crust (after O’Reilly et al., 2001, with permission from the
           blages indicate that chemical depletion in the mantle   Geological Society of America). Compositions have
           lithosphere was coupled to accretionary processes in   been calculated from garnet xenocrysts (Gnt). Xenolith
           the overlying crust (Pearson  et al., 2002). This broad   averages shown for comparison. Plot shows that newly
           correspondence is strong evidence that the crust and   formed subcontinental lithospheric mantle has become
           the underlying lithospheric mantle formed more or less   progressively less depleted in Al and Ca contents from
           contemporaneously and have remained mechanically   Archean through Proterozoic and Phanerozoic time.
           coupled since at least the Late Archean. A progressive   Garnet peridotite xenoliths from young extensional
           decrease in the degree of depletion in the lithospheric   areas (e.g. eastern China, Vitim in the Baikal region of
           mantle since the Archean (Fig. 11.14) indicates that the   Russia, and Zabargad Island in the Red Sea) are
           Archean–Proterozoic boundary represents a major shift   geochemically similar to primitive mantle, indicating
           in the nature of lithosphere-forming processes, with   very low degrees of melt depletion.
           more gradual changes occurring during the Phanero-
           zoic (O’Reilly et al., 2001). The most obvious driving
           mechanism of this change is the secular cooling of the   derived from laboratory measurements (Lenardic et al.,
           Earth (Section 11.2). In addition, processes related to   2003). These issues, and the extent to which the cratonic

           subduction, collision, terrane accretion, and magma   mantle interacts with and influences the pattern of
           addition also helped to form and stabilize the con-  mantle convection, presently are unsolved. Improved
           tinental lithosphere.                        resolution of the structure, age and geochemical evolu-
             Whereas these and many other investigations have   tion of the continental crust and lithospheric mantle
           identified some of the processes that contributed to the   promise to help geoscientists resolve these problems in

           formation and stabilization of Archean cratons, numer-  the future.
           ous questions still remain. Reconciling the composition
           of craton roots determined from petrologic studies
           with the results of seismic velocity studies is problem-  11.4.3 Proterozoic
           atic (King, 2005). There are many uncertainties about
           how stability can be achieved for billions of years   plate tectonics
           without suffering mechanical erosion and recycling in
           the presence of subduction and mantle convection.   Early tectonic models of Proterozoic lithosphere envis-
           Another problem is that the strength of mantle materi-  aged that the Archean cratons were subdivided by
           als required to stabilize craton roots in numerical exper-  mobile belts in which deformation was wholly ensialic,
           iments exceeds the strength estimates of these materials   with no rock associations that could be equated with
   376   377   378   379   380   381   382   383   384   385   386