Nonequilibrium magma degassing: Results from modeling of the ca. 1340 A.D. eruption of Mono Craters, California

We present results from a numerical conduit model of nonequilibrium magma degassing. We show that CO2/H2O concentration ratios in pyroclastic obsidian from the ca. 1340 A.D. Mono Craters eruption may record nonequilibrium degassing during magma ascent. Our results also indicate that permeability-controlled, open-system gas loss is consistent with obsidian formation and promotes nonequilibrium degassing at shallow depths. Because of the low diffusivity of CO2 relative to H2O, we find that CO2 concentrations can remain above equilibrium during magma ascent. To reproduce Mono Craters volatile concentrations, our model does not require volatile supersaturation, or an exsolved gas phase, prior to magma eruption. We estimate magmatic volatile contents of approximately 400 ppm CO2 and 4.6 wt.% H2O. However, nonequilibrium is contingent upon low rates of bubble nucleation to shallow depths, so that average bubble number densities are of order 10 11 m -3 during most of the magma ascent. If bubble number densities during ascent of the Mono Craters magma were greater than 1011 m � 3