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32   CHAPTER 2



           most closely approaches its melting point (Section   pressure studies have shown that olivine, the dominant
           2.12, Fig. 2.36).                            mineral in mantle peridotite, undergoes transforma-
             Only a very small amount of melt is required to   tions to the spinel structure at the pressure/tempera-
           lower the seismic velocity of the mantle to the observed   ture conditions at 410 km depth and then to perovskite
           values and to provide the observed attenuation proper-  plus magnesiowüstite at 660 km (Table 2.4) (Helffrich &
           ties. A liquid fraction of less than 1% would, if distrib-  Wood, 2001). Within subducting lithosphere, where the

           uted along a network of fissures at grain boundaries,   temperature at these depths is colder than in normal
           produce these effects (O’Connell & Budiansky, 1977).   mantle, the depths at which these discontinuities occur
           The melt may also be responsible for the high electrical   are displaced exactly as predicted by thermal modeling
           conductivity of this zone. For the partial melting to   and high-pressure experiments (Section 9.5). This lends
           occur, it is probable that a small quantity of water is   excellent support to the hypothesis that the upper and
           required to lower the silicate melting point, and that this   lower bounds of the transition zone are defi ned  by
           is supplied from the breakdown of hydrous mantle   phase transformations. The other components of
           phases. The base of the low velocity zone and even its   mantle peridotite, pyroxene and garnet, also undergo
           existence may be controlled by the availability of water   phase changes in this depth range but they are gradual
           in the upper mantle (Hirth & Kohlstedt, 2003).  and do not produce discontinuities in the variation of
             The mantle low velocity zone is of major impor-  seismic velocity with depth. Pyroxene transforms into
           tance to plate tectonics as it represents a low viscosity   the garnet structure at pressures corresponding to 350–
           layer along which relative movements of the lithosphere   500 km depth; at about 580 km depth Ca-perovskite
           and asthenosphere can be accommodated.       begins to exsolve from the garnet, and at 660–750 km
                                                        the remaining garnet dissolves in the perovskite phase
                                                        derived from the transformation of olivine. Thus the
           2.8.5 The mantle                             lower mantle mostly consists of phases with perovskite
                                                        structure.
           transition zone


           There are two major velocity discontinuities in the
           mantle at depths of 410 km and 660 km. The former   2.8.6  The lower mantle
           marks the top of the transition zone and the latter its
           base. The discontinuities are rarely sharp and occur   The lower mantle represents approximately 70% of the

           over a finite range in depth, so it is generally believed   mass of the solid Earth and almost 50% of the mass of
           that they represent phase changes rather than changes   the entire Earth (Schubert et al., 2001). The generally
           in chemistry. Although these discontinuities could be   smooth increase in seismic wave velocities with depth
           due to changes in the chemical composition of the   in most of this layer led to the assumption that it is
           mantle at these depths, pressure induced phase changes   relatively homogeneous in its mineralogy, having mostly
           are considered to be the more likely explanation. High-  a perovskite structure. However, more detailed seismo-



           Table 2.4  Phase transformations of olivine that are thought to define the upper mantle transition zone (after Helffrich

           & Wood, 2001).

             Depth                  Pressure
             410 km                13–14 GPa                (Mg,Fe) 2 SiO 4  = (Mg,Fe) 2 SiO 4
                                                             Olivine    Wadsleyite (β-spinel structure)
             520 km                  18 GPa                 (Mg,Fe) 2SiO 4 = (Mg,Fe) 2SiO 4
                                                             Wadsleyite   Ringwoodite (γ-spinel structure)
             660 km                  23 GPa                 (Mg,Fe) 2 SiO 4  = (Mg,Fe)SiO 3  + (Mg,Fe)O
                                                             Ringwoodite  Perovskite Magnesiowüstite
   40   41   42   43   44   45   46   47   48   49   50