Detailed analysis of ODP Leg 110 cores provides evidence for a complex structural evolution of the frontal thrust system of the Barbados Ridge accretionary wedge. Thrust faulting and back rotation are the dominant thickening mechanisms within 5 km of the toe of the wedge. Folding and duplex formation are only secondary thickening processes at this point. Estimates of shortening across the frontal 5 km of the wedge vary depending on the balancing technique used. Ignoring the affects of compaction, line-balanced sections suggest 26-36% tectonic shortening, whereas simple volume balanced sections indicate 32% shortening. When a potential average 14% volume loss is considered, the volume-balance estimates of shortening rise to nearer 40%.By 12 km from the front (Site 673), large-scale folding, with the development of overturned sections, becomes a significant thickening process. This folding is followed by the development of low-angle faults that cut out stratigraphic section at around 18 km from the toe (Site 674). These faults are interpreted as out-of-sequence thrusts that cross-cut and dismember an already complexly deformed wedge. The out-of-sequance thrusts are found in a region of the wedge where arc-dipping, low-angle reflectors become prominent on seismic reflection profiles.The current basal decollement zone (to the east of Site 674) lies in the lower Miocene section. Oligocene and Eocene strata are thrust undeformed beneath the wedge for at least 12-18 km (and perhaps farther). The presence of Oligocene and Eocene material within the wedge is, therefore, evidence of a different basal decollement geometry in the past. This different geometry could have entailed either: (1) an earlier phase of frontal off-scraping, with a decollement zone at a lower stratigraphic level; or (2) duplex formation and underplating of part of the Oligocene and Eocene section. We suggest that a mechanism of underplating is the best explanation for the general structural configuration observed at Site 674. If this is the case, then on ODP Leg 110 we made the first penetration of an underplated section in ODP or DSDP history.The overall progression in structural style across the accretionary wedge reflects the need for continuous shape adjustments to maintain a stable critical taper during progressive accretion. Erosion of material from the slope of the wedge at Sites 673 and 674 may have had an important affect on the structural development of the wedge. It is important to note that erosion becomes significant in the region of the wedge where underplating and out-of-sequence thrusting is proposed to have occurred.