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OCEAN RIDGES  125



            6.2 BROAD                                    is slightly thinner than encountered in the main ocean
                                                         basins, and that the upper mantle velocity beneath the
            STRUCTURE OF THE                             crestal region is anomalously low (Fig. 6.4). Oceanic
                                                         layer 1 rocks (Section 2.4.5) are only present within
                                                         topographic depressions, but layers 2 and 3 appear to
            UPPER MANTLE                                 be continuous across the ridge except for a narrow
                                                         region at the crest. A similar structure has been
            BELOW RIDGES                                 determined for the Mid-Atlantic Ridge (Fig. 6.5). The
                                                         suggestion of this latter work that layer 3 is not con-
                                                         tinuous across the ridge was subsequently disproved
                                                         (Whitmarsh, 1975; Fowler, 1976).
            Gravity measurements have shown that free air anoma-  As the crust does not thicken beneath ridges, iso-
            lies are broadly zero over ridges (Figs 6.4, 6.5), indicat-  static compensation must occur within the upper
            ing that they are in a state of isostatic equilibrium   mantle by a Pratt-type mechanism (Section 2.11.3).
            (Section 2.11.6), although small-scale topographic fea-  Talwani et al. (1965) proposed that the anomalously low
            tures are uncompensated and cause positive and nega-  upper mantle velocities detected beneath ridges corre-
            tive free air anomalies. The small, long wavelength,   spond to the tops of regions of low density. The densi-
            positive and negative free air anomalies over the crests   ties were determined by making use of the Nafe–Drake
            and fl anks, respectively, of ridges are a consequence of   relationship between P wave velocity and density (Nafe
            the compensation, with the positives being caused by   & Drake, 1963), and a series of models produced that
            the greater elevation of the ridge and the negatives   satisfied both the seismic and gravity data. One of these


            from the compensating mass deficiency. The gravita-  is shown in Fig. 6.6, and indicates the presence beneath
            tional effects of the compensation dominate the gravity   the ridge of a body with a density contrast of
            field away from the ridge crest, and indicate that the   −0.25 Mg m  extending to a depth of some 30 km. This

                                                                  −3

            compensation is deep.                        large density contrast is difficult to explain geologically.
               Seismic refraction experiments by Talwani  et  al.   An alternative interpretation, constructed by Keen &

            (1965) over the East Pacific Rise showed that the crust   Tramontini (1970), is shown in Fig. 6.7. A much lower,



























            Fig. 6.4  Heat flow, free air gravity anomaly and crustal structure defined by seismic refraction across the East Pacific

                                          −1
            Rise at 15–17°S. P wave velocities in km s  (redrawn from Talwani et al., 1965, by permission of the American
            Geophysical Union. Copyright © 1965 American Geophysical Union).
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