摘要

Multichannel seismic (MCS) profiles and bathymetric data from the central Mariana and Izu-Bonin subduction systems image the subducting Pacific Plate from the outer trench slope to beneath serpentinite seamounts on the outer fore arc. Subducting oceanic crust varies along the Mariana margin from 5.3 to 7 km thick and is covered by 0.5-2 km thick sediments and numerous seamounts. Oceanic crustal thickness east of the Izu-Bonin Trench is similar to 6 km. Faulting resulting from flexure of the incoming Pacific Plate begins up to 100 km east of the trench axis, near the 6 km depth contour. The plate is cut by normal faults that reactivate inherited tectonic fabric where that fabric strikes <25 degrees to the trench. Where the strike is >25 degrees, incoming crust breaks along new faults with a trench-parallel strike. The Mariana Trench axis is commonly a graben that accommodates an abrupt change (within <25 km) of plate dip from <4 degrees (commonly <= 2 degrees) on the incoming plate to >8 degrees beneath the outer fore arc. We infer that the plate fails there rather than simply bends under the applied loads. Along portions of the Mariana margin, subducting seamounts displace the trench axis westward and uplift the toe of the slope. Surprisingly, west of the toe, there is no geophysical evidence of disturbance of the upper plate in response to seamount subduction, nor of significant subduction erosion or sediment underplating. MCS profiles across the base of the Mariana inner trench slope provide evidence for both complete subduction and small-scale accretion of Pacific Plate sediments; however, we found no evidence for long-term sediment accretion. The subducting plate dips 912 degrees beneath serpentinite seamounts on the Izu-Bonin and Mariana fore arcs. Along the Mariana margin, the majority of these seamounts are located similar to 50-70 km west of the trench where the mantle wedge is 3-7 km thick between 8-10 km thick fore-arc crust and the top of the subducting plate. The apparent lack of significant deformation of the Mariana fore arc crust by subducting seamounts may be the result of a weak serpentinized mantle wedge and/or progressive fracturing as the subducting plate increases in dip as it passes through the trench graben.

  • 出版日期2008-6-10