Deformed sediments collected from drilling at the Cascadia forearc were examined using optical and electron microscopy. A wide range of microstructures was encountered in a sample suite consisting mainly of fine-grained sediments. Most of the samples were recovered from the Oregon sector of the accretionary wedge, at Site 891, located at the deformation front, and Site 892, located on the second thrust ridge. For purposes of comparison, we also examined a small number of samples from the undeformed Cascadia Basin (Site 888) and from behind the second thrust ridge at the Vancouver Margin (Sites 889 and 890).Within each site, there is a strong compositional control on the style of deformation. Diatomaceous silts tend to show a more brittle style of deformation than either clay-rich silts or sands. Arrays of subparallel shear zones and incipiently scaly textures are developed in clay-rich sediments.At Site 891, intense deformation is largely confined to the vicinity of fault zones, where thick (tens of meters) intervals of incipiently scaly fabric and thin (tens of centimeters) zones of fault gouge are developed. Chaotic, small-scale folding is present at several horizons, and, in some cases, is overprinted by shear zones.Deformation at Site 892 is much more pervasive, with widespread fracturing producing a mosaic-like microstructure of angular blocky fragments. We interpret the blocky fractured texture as evidence for previous high pore fluid pressures and natural hydraulic fracturing within the Cascadia accretionary prism. Intervals of intense fracturing are transitional into a "pillowin-matrix" structure consisting of subrounded blocks of intact sediment within a sheared, clay-rich matrix. Darkened zones of gouge and broken formation, several meters thick, are interpreted as the main fault zones that have previously conducted fluids from depth, so that the fault rocks were chemically altered and mineralized.