SZO Seminar Notes - April 8, 2015: Heat, fluid and methane on the Washington segment of the Cascadia margin

 

Discussion leader: Paul Johnson

Paper: Hautala, S. L., E. A. Solomon, H. P. Johnson, R. N. Harris, and U. K. Miller (2014), Dissociation of Cascadia margin gas hydrates in response to contemporary ocean warming, Geophys. Res. Lett., 41, doi:10.1002/2014GL061606.

 

The discussion highlighted the many types of intertwined studies being conducted along Cascadia margin.  While Paul focused on one topic, the distribution and evolution of hydrates, the topic has direct and indirect links to numerous subduction processes (e.g., faulting, accretionary wedge structure, turbidites). 

 

Paul gave an overview of gas hydrates and why they are important, particularly with respect to their impact on climate change.  Hydrates release methane, and the methane flux off the WA margin is same amount per year as released in the Deepwater Horizon spill.  At the current rates of flux increase, by 2100 the annual rate of methane release will be equivalent to 6 Deepwater Horizon spills.  This would completely change the biology of the entire coastal region.  Evidence of such massive impacts of methane release come from the Eocene, when a massive plume event warmed all of the oceans, causing all the hydrates to decompose and release their methane.  This further raised the planet’s temperatures, ultimately leading to massive extinctions.

 

Cascadia’s hydrates - background

 

Hydrates form cages of water molecules that enclose guest gas molecules, mostly methane.  When hydrates decompose they release the gas, thus they sometimes are called ‘the ice that burns’. Hydrate stability depends on pressure, temperature, and CH4 concentration.  When temperature rises it becomes unstable.  Along much of Cascadia margin the stability boundary is at ~500 m depth.

 

Cascadia sediments have an unusually high percentage of organic material, which are heated by the warm young incoming plate, leading to hydrate formation.  Methane-rich gases and fluids travel upward from within accretionary wedge along faults.  Along much of the Cascadia margin hydrates form 200-300 m thick layers that coat the sediments until they reach the stability boundary at ~500 m depth where they decompose, releasing methane.

 

The above processes may lead to over-steepened slopes that are stabilized by the hydrates, and that may fail as they warm.  This could explain some of turbidites.

 

High latitudes warming more than anywhere else.  As seabed temperature increase 2-3˚C over 30 years, hydrates become unstable – big hydrate plums.

 

Cascadia’s hydrates and climate change

 

Paul and colleagues analyzed 6,596 CTD (conductivity/temperature/salinity/depth) profiles along Washington margin and inferred a 0.3˚C  temperature rise over the last 40 years at the hydrate stability depth of ~500 m.  This warming is not apparent at the surface, but its existence at depth makes sense as deeper waters come from Sea of Okotsk.  Data from Sea of Okotsk show they have warmed significantly, consistent with broader studies showing warming is most profound at polar latitudes. 

 

Their working hypothesis is that the inferred increase of 0.3˚C  is like moving hydrate stability downward ~50 m and seaward ~1 km (depends on slope), causing the hydrates between the old and new effective boundaries to decompose and release methane via increased plume activity.  Methane plumes exist at all depths above the stability boundary because methane escapes on its own for other reasons than warming, so this hypothesis predicts an increase in plume activity near the stability boundary.  To demonstrate likely causality between warming waters and increased activity requires independent evidence that the gases released originate near the stability boundary and not from greater depths.

 

Methane plumes can be detected using imaging techniques and by following the fish; i.e., fishermen report fishing hot spots, which when checked turn out to be where plumes attract microbes that fish feed on.  Plumes have been mapped, after normalizing for density and activity (necessary because of the high variability in slope), it appears that in the interval between 400-500 m, the number of emission sites is anomalously high.  This result is somewhat ambiguous because the sampling is non-uniform.  Nonetheless, it is at least consistent with the hypothesis.

 

The final step in testing this hypothesis is to show that the increased plume activity is sourced by decomposing hydrates due to warming.  One way to do this is to show that the chemistry of emitted methane is consistent with hydrate decomposition (e.g., the methane did not come from deeper sources).  This is work in progress.