Numerous studies have considered the perturbations in pressure, temperature, pore water salinity, and other conditions that may cause breakdown of natural gas hydrates in marine sediments (e.g., Kennett et al., 2003; Mienert et al., 2005; Reagan and Moridis, 2008; Biastoch et al., 2011; Ruppel, 2011; Phrampus and Hornbach, 2012; Ferre et al., 2012). In contrast, only a few studies—most notably the work of McGinnis and co-workers [McGinnis et al., 2006; Greinert and McGinnis, 2009; Greinert et al., 2010)—have focused on the fate of non-catastrophically-released individual methane bubbles once they enter the water column that act as the critical buffer between the sediment and the atmosphere. In recent years, it has become widely accepted that the water column may itself be an important chemical sink for methane [Reeburgh, 2007; Mau et al., 2007; Kessler et al., 2011; Ruppel and Kessler, 2017]. Less widely understood are the physics of bubble rise; the controls on and timescales of the formation of bubble-encasing hydrate shells; the role that hydrate formation around rising bubbles may play in mitigating their dissolution and allowing methane to reach shallow parts (e.g., upper mixed layer) of the water column; and how modern shipboard imagery of methane plumes can be used to estimate bubble size, height of final bubble rise, and methane flux from the seafloor on both a local and regional basis.
This research project will in part constrain the conditions under which this relatively direct injection path from the seafloor to the atmosphere might be expected to operate. Currently, this direct injection path appears to be limited to shallow water settings [McGinnis et al., 2006] and catastrophic methane release events [Leifer et al., 2006]. The numerical modeling and the laboratory experiments to be undertaken in this research program will permit the project team to assess whether other conditions (including pre-existing methane supersaturation of the water column or formation of a hydrate shell around a rising bubble) also permit relatively direct injection of methane into the upper mixed layer of the ocean, where methane can more easily access the atmosphere.