THE ROLE OF ANHYDRITE DEPOSITION IN SUB-SEAFLOOR SILL-DRIVEN HYDROTHERMAL SYSTEMS
Numerical models of this convection allow us to study the evolution of the system with permeability changes based on the diagenesis and redissolution of anhydrite in the sub-seafloor. Previous models using an infinite heated base to approximate a mid-ocean ridge show the system being "choked" by a barrier produced by the anhydrite precipitation front, with venting temperatures not exceeding 80 degrees Celsius (Fontaine, et al., 2001). This leads to the conclusion that other factors such as tectonism or subsequent volcanism are required to alter the permeability profile and allow the hotter venting required to produce black smokers. In our calculations, the heat source intrusion or magma chamber is modeled with a thickness and an edge, as in an isolated sill emplacement, and the free convection at that edge dominates the system and vents at temperatures greater than 300 degrees Celsius. In this system, the anhydrite effectively "sheathes" the hydrothermal plumes, and allows them to vent at hotter temperatures for longer than in simulations without anhydrite calculations.
References
Fontaine, F., M. Rabinowicz, and J. Boulegue. 2001. Permeability changes due to mineral diagenesis in fractured crust: implications for hydrothermal circulation at mid-ocean ridges. Earth Planet. Sci. Lett., 184: 407-425.
Haymon, R.M. 1983. The growth history of hydrothermal black smoker chimneys. Nature, 301: 695-696.