I summarize results of active-source seismic investigations, including singlechannel seismic reflection, ocean-bottom seismic refraction, and vertical seismic profiles, from the Blake Ridge, offshore South Carolina. The Blake Ridge is a highly dynamic system, in which methane gas is being generated today at depths exceeding 700 m and migrates on the sub-Ma time scale. Seismic velocities indicate that hydrate occupies 3^4% of total rock volume (5-7% of porosity) in a 250-m-thick zone on the crest of the ridge and only about 1-2% of total rock volume 7 km off the crest of the ridge. A significant proportion of methane resides beneath the stability zone, where free gas comprises 1-10% of total rock volume in a zone at least 250 m thick. The impedance contrast responsible for the BSR is caused principally by gas, not hydrate: Site 994 shows that hydrate is not a sufficient condition for generation of a BSR, while Sites 995 and 997 suggest that free gas is a necessary condition. Zones of low reflectance beneath the BSR demonstrate that amplitude "blanking" is not required to explain low reflectance above the BSR on the Blake Ridge. Gas migrates along permeability contrasts at stratal boundaries and can be trapped by faults and at the base of the hydrate stability zone. The Blake Ridge collapse structure, which shows strong circumstantial evidence for expulsion of large quantities of methane into the ocean/atmosphere system, does not appear to have been a single catastrophic event. Rather, the collapse appears to be a relatively long-lived feature filled in the last 2 my at deposition rates of up to 300 m/my. Buried features similar to the collapse beneath the ridge suggest that episodic gas release is a fundamental, recurring part of the hydrate cycle on the Blake Ridge.