HOW LOW CAN YOU GO? THE EFFECTS OF RESIDUAL H2O ON THE ADVANCE OF OBSIDIAN LAVA FLOWS OF THE WESTERN UNITED STATES
Spatially well constrained samples were collected from three drill cores produced during the Continental Scientific Drilling Program (CSDP) in 1984. Two drill cores were collected from the ~0.6 ka Obsidian Dome, Inyo Craters, California, including one drill core near the vent (RDO-2B) and another near the flow margin (RDO-2A). The third drill core (VC-1) was collected from the ~68.3 ka Banco Bonito flow in Valles Caldera, New Mexico. The volatile content, apparent viscosity, and texture have been determined for samples using Fourier-transform infrared spectroscopy (FTIR), parallel-plate viscometry, and density measurements respectively.
We find that the water content of the three drill cores vary little as a function of depth in the lava flow with an average of 0.32 ± 0.35 (1σ) wt. % H2Otot (RDO-2B), 0.19 ± 0.09 (1σ) wt. % H2Otot (RDO-2A), and 0.27 ± 0.14 (1σ) wt. % H2Otot (VC-1). However, there is a significant difference (P = 0.001) between the average H2Otot from the vent proximal drill core, to the distal drill core from Obsidian Dome, suggesting additional degassing occurs during emplacement. Additionally, samples with low H2Otot (≥0.1 wt. %) can still vesiculate at ambient pressures and reasonable emplacement temperatures. Thus, pumiceous textures observed in obsidian lava flows can form at the surface, simultaneously removing water and increasing the viscosity by up to a factor of 4 to 5. Additionally, vesiculation introduces bubbles to the lava and increases the apparent viscosity by a factor of 3 to 30, when compared to a bubble-free melt with a comparable water content. We conclude that water contents as low as ~0.1 wt. % H2Otot can continue to influence the evolution and advance of obsidian lava flows.