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THE INTERIOR OF THE EARTH  31



            of the transition zone. There is a further velocity discon-  bined into the crust. The latter, so called “incompatible”
            tinuity at a depth of 660 km, the base of the transition   elements, include the heat producing elements K, Th,
            zone.                                        and U. It is clear from the composition of mid-ocean
               Within the lower mantle velocities increase slowly   ridge basalts (MORB), however, that the mantle from
            with depth until the basal 200–300 km where gradients   which they are derived by partial fusion is relatively
            decrease and low velocities are present. This lower-  depleted in these elements. So much so that, if the
            most layer, at the core–mantle boundary, is known as   whole mantle had this composition, it would only

            Layer D″ (Section 12.8.4) (Knittle & Jeanloz, 1991).   account for a small fraction of the heat flow at the
            Seismic studies have detected strong lateral heteroge-  Earth’s surface emanating from the mantle (Hofmann,
            neities and the presence of thin (5–50 km thick) ultra-  1997). This, and other lines of geochemical evidence,
            low velocity zones at the base of Layer D″ (Garnero   have led geochemists to conclude that all or most of the
            et al., 1998).                               lower mantle must be more enriched in incompatible
                                                         elements than the upper mantle and that it is typically
                                                         not involved in producing melts that reach the surface.
            2.8.3 Mantle composition                     However, seismological evidence relating to the fate of
                                                         subducted oceanic lithosphere (Sections 9.4, 12.8.2) and
            The fact that much of the oceanic crust is made up of   the lateral heterogeneity of Layer D″ suggests mantle
            material of a basaltic composition derived from the   wide convection and hence mixing (Section 12.9).
            upper mantle suggests that the upper mantle is com-  Helffrich & Wood (2001) consider that the various lines
            posed of either peridotite or eclogite (Harrison &   of geochemical evidence can be reconciled with whole
            Bonatti, 1981). The main difference between these two   mantle convection if various small- and large-scale het-
            rock types is that peridotite contains abundant olivine   erogeneities in the lower mantle revealed by seismo-
            and less than 15% garnet, whereas eclogite contains   logical studies are remnants of subducted oceanic and
            little or no olivine and at least 30% garnet. Both possess   continental crust. They estimate that these remnants
            a seismic velocity that corresponds to the observed   make up about 16% and 0.3% respectively of the mantle
                                       −1
            upper mantle value of about 8 km s .         volume.
               Several lines of evidence now suggest very strongly   Although estimates of bulk mantle composition vary
            that the upper mantle is peridotitic. Beneath the ocean   in detail, it is generally agreed that at least 90% of the
            basins the P n velocity is frequently anisotropic, with   mantle by mass can be represented in terms of the
            velocities over 15% higher perpendicular to ocean   oxides FeO, MgO, and SiO 2 , and a further 5–10% is
            ridges. This can be explained by the preferred orienta-  made up of CaO, Al 2 O 3 , and Na 2 O.
            tion of olivine crystals, whose long  [100]  axes are
            believed to lie in this direction. None of the common
            minerals of eclogite exhibit the necessary crystal elon-  2.8.4 The mantle
            gation. A peridotitic composition is also indicated by
            estimates of Poisson’s ratio from P and S velocities, and   low velocity zone
            the presence of peridotites in the basal sections of
            ophiolite sequences and as nodules in alkali basalts.   The low velocity zone (Fig. 2.16) is characterized by
            The density of eclogites is also too high to explain the   low seismic velocities, high seismic attenuation, and a
            Moho topography of isostatically compensated crustal   high electrical conductivity. The seismic effects are
            structures.                                  more pronounced for S waves than for P waves. The
               The bulk composition of the mantle can be esti-  low seismic velocities could arise from a number of
            mated in several ways: by using the compositions of   different mechanisms, including an anomalously high
            various ultramafic rock types, from geochemical com-  temperature, a phase change, a compositional change,

            putations, from various meteorite mixtures, and by   the presence of open cracks or fissures, and partial

            using data from experimental studies. It is necessary to   melting. All but the latter appear to be unlikely, and it
            distinguish between undepleted mantle and depleted   is generally accepted that the lower seismic velocities
            mantle which has undergone partial melting so that   arise because of the presence of molten material. That
            many of the elements which do not easily substitute   melting is likely to occur in this region is supported
            within mantle minerals have been removed and com-  by the fact that it is at this level that mantle material
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