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OCEAN RIDGES  127



                                                         (iii) a temperature-dependent phase change. The high
                                                         temperatures beneath ocean ridge crests might cause a
                                                         transition to a mineralogy of lower density.
                                                            Suppose the average temperature to a depth of
                                                         100 km below the Moho is 500°C greater at the ridge

                                                         crest than beneath the flanking regions, the average
                                                                                    −3
                                                         density to this depth is 3.3 Mg m  and the volume
                                                                                        −5

                                                         coefficient of thermal expansion is 3 × 10  per degree.
                                                         In this case the average mantle density to a depth of
                                                                               −3
                                                         100 km would be 0.05 Mg m  less than that of the

                                                         flanking ocean basins. If isostatic equilibrium were
                                                         attained, this low-density region would support a

                                                         ridge elevated 2.2 km above the flanking areas. If the
                                                         degree of partial melting were 1%, the consequent
                                                                                                 −3
                                                         decrease in density would be about 0.006 Mg m .
                                                         Extended over a depth range of 100 km this density
                                                         contrast would support a relative ridge elevation of
            Fig. 6.7  Alternative model of the structure beneath the   0.25 km. The aluminous minerals within the upper

            Mid-Atlantic Ridge from gravity modeling. Profile at   mantle that might transform to a lower density phase
                             −3
            46°N. Densities in Mg m  (redrawn from Keen &   are also the minerals that enter the melt that forms
            Tramontini, 1970, with permission from Blackwell   beneath the ridge crest. They are absent therefore in
            Publishing).                                 the bulk of the mantle volume under consideration,
                                                         which consists of depleted mantle; mantle from which
                                                         the lowest melting point fraction has been removed.
                                                         It is unlikely then that a phase change contributes
            members of a suite of possible interpretations. They   significantly to the uplift.

            demonstrate without ambiguity, however, that ridges   Partial melting of the upper mantle clearly is a
            are underlain by large, low-density bodies in the upper   reality because of the magmatic activity at ridge crests,
            mantle whose upper surfaces slope away from the ridge   but its extent was a matter of conjecture. However, in
            crests.                                      the mid-1990s a very large-scale experiment, the Mantle
                                                         Electromagnetic and Tomography (MELT) experiment,
                                                         was carried out on the crest of the East Pacifi c  Rise

                                                         specifically to define the vertical and lateral extent of

            6.3 ORIGIN OF                                the region of partial melting beneath it (MELT seismic
                                                         team, 1998). Fifty-one ocean bottom seismometers and
            ANOMALOUS UPPER                              47 instruments that measure changes in the Earth’s

                                                         magnetic and electric fields were deployed across the
            MANTLE BENEATH                               ridge, between 15° and 18°S, in two linear arrays each
                                                         approximately 800 km long. This location was chosen
            RIDGES                                       because it is in the middle of a long, straight section of

                                                         the ridge between the Nazca and Pacific plates, and has
                                                                                          −1
                                                         one of the fastest spreading rates: 146 mm a  at 17°S.
                                                         The extent of any partial melt in the mantle should
            There are three possible sources of the low-density   therefore be well developed in terms of low seismic
            regions which underlie ocean ridges and support them   velocities and high electrical conductivity. Seismic waves
            isostatically (Bott, 1982): (i) thermal expansion of upper   from regional and teleseismic earthquakes, and varia-
            mantle material beneath the ridge crests, followed by   tions in the Earth’s electric and magnetic fi elds, were

            contraction as sea floor spreading carries it laterally   recorded for a period of approximately 6 months. Anal-
            away from the source of heat, (ii) the presence of   ysis of the data revealed an asymmetric region of low
            molten material within the anomalous mantle,   seismic velocities extending to a depth of 100 km, with
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