Abstract

Marine pockmarks are globally widespread seabed depressions, conventionally thought to be formed by the accumulation and expulsion of microbial and thermogenic gas. However, other putative fluids and processes have been implicated in pockmark formation and gas escape to the atmosphere may be underestimated. Given the complex spectrum of aquatic settings, morphologies and sizes, there may also exist a spectrum of physical, chemical and biological processes that form pockmarks. Pockmarks in shallow coastal waters are now understood to be widespread, but the influence of physical dynamics (e.g. tides, storms, etc.), terrestrial processes and anthropogenic activities add considerable spatiotemporal complexity and uncertainty to our understanding of these features. Here, we revisit a field of small (ca. 2 m diameter), shallow (<1 m depth) pockmarks in Dunmanus Bay, Ireland. The presence of muddy surface sediments overlying sand in the pockmarked area indicates that gas accumulation within fine-grained surface sediments contributes to formation of the features. Previous work indicates that CH4 is an important seepage fluid in Dunmanus and neighbouring bays. However, based on evidence from multiple surveys, we observe considerable spatiotemporal complexity, and the transient nature of the gas within sediments points to the potential for fluids other than traditional microbial or thermogenic CH4, migrating from sources tens to hundreds of metres below the seafloor. We observed atypical porewater profiles where millimolar concentrations of H2S concentrations are observed in surface sediments in the absence of SO42− depletion, together with NH4+ build-up from ammonification of sedimentary organic matter. Archaeal methanogens, anaerobic methanotrophic archaea and SO42--reducing Deltaproteobacteria co-occur in surface sediments in the pockmark field and NMR revealed the presence of non-competitive substrates for methanogens. We hypothesize that in-situ methanogenesis and production of other volatile metabolites besides CH4 (e.g. CO2, dimethyl disulfide) from microbial degradation of organic matter are potential gaseous fluids and could contribute to the formation of small pockmarks.

Highlights

  • Pockmarks are circular or sub-circular seabed depressions, which may reach diameters of hundreds of metres and depths of tens of metres (Judd and Hovland, 2007; King and MacLean, 1970)

  • Archaeal metha­ nogens, anaerobic methanotrophic archaea and SO42--reducing Deltaproteobacteria co-occur in surface sediments in the pockmark field and NMR revealed the presence of non-competitive substrates for methanogens

  • Sedimentary CH4 is produced by microbial methanogenesis during degradation of organic matter, or from thermogenic gas produced by high-temperature cracking of organic matter at considerable burial depths (Reeburgh, 2007)

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Summary

Introduction

Pockmarks are circular or sub-circular seabed depressions, which may reach diameters of hundreds of metres and depths of tens of metres (Judd and Hovland, 2007; King and MacLean, 1970). Low when considering the overall CH4 atmospheric flux from all sources - 5–20% of net modern atmospheric flux (20–100 Tg CH4 yr − 1, Valentine and Reeburgh, 2000) shallow coastal waters dominate oceanic CH4 contributions (Weber et al, 2019) This is because CH4 is consumed in the water column as gas bubbles rise, so seabed seepage in shallow water is more likely to be released to the atmosphere than CH4 from deepwater pockmarks and seeps (Judd, 2004). Given the sparsity of surveys and lack of curated databases on seafloor fluid expulsion (Phrampus et al, 2020), the atmospheric flux of CH4 and other greenhouse gases from coastal marine settings could be substantially underestimated

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