Abstract
JOURNAL OF GEOPHYSICAL RESEARCH,
VOL. 113,
B08S12,
21 PP., 2008
doi:10.1029/2007JB005467
Venting of a separate CO2-rich gas phase from submarine arc volcanoes: Examples from the Mariana and Tonga-Kermadec arcs
Pacific Marine Environmental Laboratory, NOAA, Newport, Oregon, USA
School of Oceanography, University of Washington, Seattle, Washington, USA
JISAO, University of Washington, Seattle, Washington, USA
CIMRS, Oregon State University, Newport, Oregon, USA
Pacific Marine Environmental Laboratory, NOAA, Newport, Oregon, USA
Institute of Geological and Nuclear Sciences, Lower Hutt, New Zealand
Institute of Geological and Nuclear Sciences, Lower Hutt, New Zealand
National Institute of Advanced Science and Technology, Tsukuba, Japan
Institute of Geosciences, University of Kiel, Kiel, Germany
Submersible dives on 22 active submarine volcanoes on the Mariana and Tonga-Kermadec arcs have discovered systems on six of these volcanoes that, in addition to discharging hot vent fluid, are also venting a separate CO2-rich phase either in the form of gas bubbles or liquid CO2 droplets. One of the most impressive is the Champagne vent site on NW Eifuku in the northern Mariana Arc, which is discharging cold droplets of liquid CO2 at an estimated rate of 23 mol CO2/s, about 0.1% of the global mid-ocean ridge (MOR) carbon flux. Three other Mariana Arc submarine volcanoes (NW Rota-1, Nikko, and Daikoku), and two volcanoes on the Tonga-Kermadec Arc (Giggenbach and Volcano-1) also have vent fields discharging CO2-rich gas bubbles. The vent fluids at these volcanoes have very high CO2 concentrations and elevated C/3He and δ 13C (CO2) ratios compared to MOR systems, indicating a contribution to the carbon flux from subducted marine carbonates and organic material. Analysis of the CO2 concentrations shows that most of the fluids are undersaturated with CO2. This deviation from equilibrium would not be expected for pressure release degassing of an ascending fluid saturated with CO2. Mechanisms to produce a separate CO2-rich gas phase at the seafloor require direct injection of magmatic CO2-rich gas. The ascending CO2-rich gas could then partially dissolve into seawater circulating within the volcano edifice without reaching equilibrium. Alternatively, an ascending high-temperature, CO2-rich aqueous fluid could boil to produce a CO2-rich gas phase and a CO2-depleted liquid. These findings indicate that carbon fluxes from submarine arcs may be higher than previously estimated, and that experiments to estimate carbon fluxes at submarine arc volcanoes are merited. Hydrothermal sites such as these with a separate gas phase are valuable natural laboratories for studying the effects of high CO2 concentrations on marine ecosystems.
Received 26 October 2007; accepted 1 April 2008; published 15 July 2008.
Citation: (2008), Venting of a separate CO2-rich gas phase from submarine arc volcanoes: Examples from the Mariana and Tonga-Kermadec arcs, J. Geophys. Res., 113, B08S12, doi:10.1029/2007JB005467.
Cited By
