MASSIVE SULFIDE DEPOSITS AT MODERN SEDIMENTED OCEANIC RIFTS: GEOLOGICAL SETTING AND GENETIC PROCESSES
The internal architecture, as discerned from ODP drilling of the Bent Hill-ODP deposits, is characterized by stacked massive sulfide lenses of mostly vent complexes underlain by a sulfide stringer zone and overlain by chimneys, sulfide rubble and clastic sulfides shed off of mounds. The Bent Hill deposit is at least 104 m thick and contains approximately 15-20 million tonnes of massive sulfides. The vent complexes consist of a high-temperature pyrrhotite-sphalerite-isocubanite/chalcopyrite assemblage that is variably replaced by pyrite, marcasite, magnetite, sphalerite and Cu-Fe-sulfides. The sulfide stringer zone cuts silicified and chloritized sediments and is rooted in a laterally extensive stratabound copper zone composed of pyrrhotite-isocubanite-chalcopyrite that infills and replaces turbiditic sediments 170-200 m below the seafloor.
The Middle Valley and Escanaba hydrothermal systems have evolved from high-temperature (>300°C), metal-rich fluids that formed the massive sulfide deposits to moderate-temperature (<276°C), metal-poor fluids that are actively venting in both areas. Sr, C and S isotope compositions indicate sediment contamination of MORB-equilibrated fluids. The sediments have played an important role in capping the hydrothermal system and focusing fluid discharge at off-axis and long-lived vent sites in the case of the Bent Hill-ODP deposits. This probably explains why deposits formed in sedimented rifts are generally fewer in number but significantly larger on average than those formed at sediment-bare oceanic ridges.