Subduction zones give rise to a range of magmas. In subduction zones, a cool slab of oceanic lithosphere sinks beneath an accretionary sedimentary prism, which, in turn, often lies beneath a forearc basin. (image - Cascadia subduction zone, courtesy USGS, larger image)
Ta and Nb are present in anomalously low concentrations in magmas associated with subduction zones, a feature that is considered diagnostic of subduction-related volcanism. Depletion of high-field-strength trace elements (mid-ocean ridge basalts (N-MORB) is the most distinctive geochemical fingerprint of subduction magmatism. Computer modeling image (or compare to image to right) of the thermal structure of a subduction zone, with convergence at 6 cm/year, suggests that rocks cool as the slab pass to great depths, only warming gradually. This type of model is consistent with seismic velocity information, and suggests that the ocean crust of the subducted slab would only melt at depths greater than 600 km.
Volcanic island arcs lie above the slab where it has sunk to depths of 120-140 km. Some computer modeling indicates that the temperature here is merely 200-300ÂșC, which would be far too cool for melting of the ocean crust, but would be sufficiently warm to drive fluid into the overlying mantle wedge, hydrating the overlying mantle. Other computer models, however, suggest that the isotherms are somewhat hotter.
Hydration of the mantle wedge depresses the melting temperature of the mantle wedge, which can partially melt to produce a basaltic magma, leaving a harzbergite residue. Alternatively, hydrated mantle could rise bouyantly to melt at shallower depths. The complexity of magma is increased by fractional crystallization as magma ascends or ponds in magma chambers. Rising magma can undergo fractional crystallization through partial solidification of more refractory minerals, or can become contaminated from the material through which it ascends. Contamination of basaltic magmas by partial contact-melting of felsic continental crust would increase the Si level of the melt, generating andesitic and rhyolitic magmas of Cordilleran composite volcanoes (compare island arc with Andean). The more recently that the rocks of subducting oceanic crust have formed, then the warmer those rocks are (graph), and the more easily they could melt upon subduction. The greater the rate of subduction of oceanic crust, then the lower the temperature of the mantle rocks that have received the subducted material (graph). The base of the subducting oceanic crust is initially hotter, but the top of the subducting crust eventually becomes hotter due to heat conducted from the mantle wedge (graph). The impact of cooling by the subducting slab is very important, rapidly dropping the temperature of the mantle wedge, in the absence of convection, below temperatures at which magmas could be generated. However, induced convection in the mantle wedge could retain temperatures above 950 °C as the wedge material is dragged down, rendering hydrous melting possible (graph). So, it is likely that arc magmas are derived from the mantle wedge and that conditions for slab melting are very restricted. However, not only pure mantle material undergoes partial melting. The subducting slab and its transported sediments may also melt, and the mantle above the subduction zone can be modified by repeated episodes of partial melting. In general, the magmas generated in subduction zones have higher volatiles and higher silica content (60% +) than the basaltic magmas formed at divergent plate boundaries. Thus, active subduction zones are crowned by an arc of explosive composite volcanoes. |