GSA Annual Meeting in Seattle, Washington, USA - 2017

Paper No. 150-4
Presentation Time: 2:15 PM

LIMITED SEDIMENT UNDERTHRUSTING AND A STRONG, DRAINED CENTRAL CASCADIA ACCRETIONARY WEDGE: ANALYSIS OF SEISMIC REFLECTION IMAGING OFF WASHINGTON


WEBB, Susanna I. and TOBIN, Harold J., Dept. of Geoscience, University of Wisconsin - Madison, 1215 W. Dayton St, Madison, WI 53706, htobin@wisc.edu

The central Cascadia subduction zone forearc in the region offshore Washington, where a hot, young incoming plate is covered by a 2-3 km thick sedimentary sequence, features a wide, very narrowly-tapered outer accretionary wedge composed of landward vergent thrust sheets. Longstanding questions for this region include the position and host-rock environment of the plate boundary décollement fault, the thickness of sedimentary strata underthrust beneath the wedge with the downgoing plate, and the effective stress or pore fluid pressure condition in the wedge and along its base. We have analyzed nine multichannel seismic lines of the 2012 COAST multi-channel seismic reflection survey using both time- and depth- migrated seismic sections for structural interpretation. Results show that there is evidence for two parallel décollement levels, with up to 200 - 500 meters thickness of a mostly-underthrust sequence in places, but which is absent entirely in others. This patchy distribution is mapped and related to features of the overlying wedge structure. We also analyzed the seismic interval velocity distribution produced during pre-stack depth migration imaging, and used it to compute porosity, pore fluid pressure, and effective stress via empirical physical properties transforms. We find that the wedge shows evidence for at most only modest, localized excess pore pressure, and instead most of the wedge appears to be at near-hydrostatic, drained condition. Modest overpressure ratios of up to only ~0.15 are detected, localized in the footwalls of thrust splays. We find no evidence for overpressure zones in the underthrust sequence below the upper décollement, in contrast to findings from several other wedges worldwide. Taken together, the accretionary wedge structure and apparent low pore pressure condition here is consistent with a mechanically strong wedge overlying a base that is very weak, at least transiently. By analogy with recent work from Sumatra, Tohoku, and elsewhere, we speculate that this is potentially conducive to efficient propagation of megathrust slip to the deformation front in large earthquakes.