Page 36 - Global Tectonics
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THE INTERIOR OF THE EARTH  23



            changes in chemical composition, while more grada-  middle crust is some 11 km thick and ranges in depth
            tional velocity boundaries are normally associated   from 12 km, at the top, to 23 km at the bottom (Rudnick
            with phase changes that occur over a discrete vertical   & Fountain, 1995; Gao et al., 1998). The average lower
            interval.                                    crust thus begins at 23 km depth and is 17 km thick.
               Models for the bulk chemical composition of the   However, the depth and thickness of both middle and
            continental crust vary widely because of the diffi culty   lower crust vary considerably from setting to setting. In
            of making such estimates. McLennan & Taylor (1996)   tectonically active rifts and rifted margins, the middle and

            pointed out that the flow of heat from the continental   lower crust generally are thin. The lower crust in these
            crust (Section 2.13) provides a constraint on the abun-  settings can range from negligible to more than 10 km
            dance of the heat producing elements, K, Th, and U,   thick (Figs 7.5, 7.32a). In Mesozoic–Cenozoic orogenic
            within it, and hence on the silica content of the crust.   belts where the crust is much thicker, the lower crust may
            On this basis they argue that on average the continental   be up to 25 km thick (Rudnick & Fountain, 1995).
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            crust has an andesitic or granodioritic composition with   The velocity range of the lower crust (6.8–7.7 km s ,
            K 2O no more than 1.5% by weight. This is less silicic   Section 2.2) cannot be explained by a simple increase of
            than most previous estimates. The abundance of the   seismic velocity with depth. Consequently, either the

            heat producing elements, and other “incompatible” ele-  chemical composition must be more mafic, or denser,
            ments, in the continental crust is of great importance   high-pressure phases are present. Information derived
            because the degree to which they are enriched in the   from geologic studies supports this conclusion, indicat-
            crust reflects the extent to which they are depleted in   ing that continental crust becomes denser and more


            the mantle.                                  mafic with depth. In addition, the results from these
                                                         studies show that the concentration of heat-producing
                                                         elements decreases rapidly from the surface down-
                                                         wards. This decrease is due, in part, to an increase in
            2.4.2  Upper continental crust               metamorphic grade but is also due to increasing propor-
                                                         tions of mafi c lithologies.
            Past theories of crustal construction suggested that the   In areas of thin continental crust, such as in rifts and
            upper continental crust was made up of rocks of granitic   at rifted margins, the middle and lower crust may be
            composition. That this is not the case is evident from   composed of low- and moderate-grade metamorphic
            the widespread occurrence of large negative gravity   rocks. In regions of very thick crust, such as orogenic
            anomalies over granite plutons. These anomalies   belts, the middle and lower crust typically are com-
            demonstrate that the density of the plutons (about   posed of high-grade metamorphic mineral assem-
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                    −3
            2.67 Mg m ) is some 0.10–0.15 Mg m  lower than the   blages. The middle crust in general may contain more
            average value of the upper crust. The mean composition   evolved and less mafic compositions compared to the

            of the upper crust can be estimated, albeit with some   lower crust. Metasedimentary rocks may be present in
            uncertainty due to biasing, by determining the mean   both layers. If the lower crust is dry, its composition
            composition of a large number of samples collected   could correspond to a high-pressure form of granulite
            worldwide and from analyses of sedimentary rocks that   ranging in composition from granodiorite to diorite
            have sampled the crust naturally by the process of   (Christensen & Fountain, 1975; Smithson & Brown,
            erosion (Taylor & Scott, 1985; Gao et al., 1998). This   1977), and containing abundant plagioclase and pyrox-
            composition corresponds to a rock type between grano-  ene minerals. In the overthickened roots of orogens,
            diorite and diorite, and is characterized by a relatively   parts of the lower crust may record the transition to
            high concentration of the heat-producing elements.  the eclogite facies, where plagioclase is unstable and

                                                         mafic rocks transform into very dense, garnet-, pyrox-
                                                         ene-bearing assemblages (Section 9.9). If the lower
            2.4.3  Middle and lower                      crust is wet, basaltic rocks would occur in the form of
                                                         amphibolite. If mixed with more silicic material, this
            continental crust                            would have a seismic velocity in the correct range.
                                                         Studies of exposed sections of ancient lower crust
            For a 40 km thick average global continental crust   suggest that both dry and wet rock types typically are
            (Christensen & Mooney, 1995; Mooney et al., 1998), the   present (Oliver, 1982; Baldwin et al., 2003).
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