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144   CHAPTER 6



                                                 km
                              4    3    2    1   0    1    2    3    4
                                                                     Small volcano
                           0

                           1
                           2                                           New magma

                          km  3                                        body

                           4

                           5
                                                                   Brittle – ductile
                           6       Plutons                            transition

           Fig. 6.18  Model for the construction of oceanic crust at a slow-spreading ridge. Transient magma bodies rise to the
           brittle–ductile transition within the crust and shoulder aside and depress older plutons. Part of the magma body erupts

           through a fissure to produce a volcano or hummocky lava flow on the sea floor and the remainder solidifies to form



           part of the main crustal layer (redrawn from Smith & Cann, 1993, with permission from Nature 365, 707–15. Copyright
           © 1993 Macmillan Publishers Ltd).
           overlying, hydrothermally altered dikes into the magma   sient. In this case the alternative model derived from
           chamber.                                     early reinterpretations of ophiolites in terms of sea

             The two gabbro units, isotropic and layered, are   floor spreading may be more applicable. This invoked
           often correlated with seismic layers 3A and 3B, respec-  multiple small magma chambers within the main crustal

           tively (Section 2.4.7). The ultramafic cumulates, rich in   layer in the light of the multiple intrusive relationships
           olivine and pyroxene, would then account for the sub-  observed at all levels in the Troodos ophiolite of south-
           Moho seismic velocities. Thus, the Moho occurs within   ern Cyprus (Moores & Vine, 1971) (Section 2.5). Smith
           the crystallized magma chamber at the base of the   & Cann (1993) favor such a model for the creation of
           mafic section. Off axis, however, in a lower temperature   oceanic crust at slow-spreading ridge crests (Fig. 6.18).


           environment, the uppermost ultramafics may become   However away from segment centers, and particularly
           partially hydrated (i.e. serpentinized) and as a result   in the vicinity of transform faults, the magma supply
           acquire lower seismic velocities more characteristic of   may be greatly reduced, and serpentinized mantle peri-
           layer 3B. The seismic Moho would then occur at a   dotite appears to be a common constituent of the
           somewhat greater depth, within the ultramafi c section.   thinned oceanic crust. This type of crust becomes even
           As a result of this uncertainty in defining the seismic   more common on very slow-spreading ridges and ulti-


           Moho, petrologists have tended to define the base of   mately most of the crust is effectively exposed mantle
           the crust as the base of the presumed magma chamber,   with or without a thin carapace of basalts. On the ultra-
           that is, the dunite/chromitite horizon. Hence, this level   slow Gakkel Ridge the crust is essentially serpentinized
           is termed the “petrologic Moho”.             and highly tectonized mantle peridotite with volcanic
             The model of Cann (1974) and Kidd (1977) has met   centers at intervals of 100 × 50 km.
           with considerable success in explaining the known   An alternative approach to understanding the accre-
           structure and petrology of oceanic crust created at fast-  tionary processes at mid-ocean ridge crests is by way of
           spreading ridge crests, where there is a steady state   thermal modeling (Sleep, 1975; Kusznir & Bott, 1976;
           magma chamber. At slow-spreading ridge crests,   Chen & Morgan, 1990). Chen & Morgan (1990) made
           however, the zone of crustal accretion is wider and it   significant improvements to such models by including

           seems probable that magma chambers are only tran-  the effects of hydrothermal circulation at ridge crests
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