ORIGINAL RESEARCH article
Front. Mar. Sci.
Sec. Marine Pollution
Volume 12 - 2025 | doi: 10.3389/fmars.2025.1589660
This article is part of the Research TopicDisturbances at Hydrothermal Vents/Cold Seeps from the Deep to the Marine Shallows: an Holistic Approach to Marine LifeView all 3 articles
The Abundance, Diversity, and Assemblage Structure of the Macrobenthos at the South Georgia Shelf Methane Seeps
Provisionally accepted- 1British Antarctic Survey (BAS), Cambridge, United Kingdom
- 2School of Natural and Environmental science, Newcastle University, Newcastle upon Tyne, North East England, United Kingdom
- 3Scottish Universities Environmental Research Centre, University of Glasgow, Glasgow, Scotland, United Kingdom
- 4Center for Marine Environmental Sciences, University of Bremen, Bremen, Bremen, Germany
- 5Faculty of Geosciences, University of Bremen, Bremen, Bremen, Germany
- 6Alfred Wegener Institute Helmholtz Centre for Polar and Marine Research (AWI), Bremerhaven, Bremen, Germany
- 7School of Ocean Sciences, College of Environmental Sciences and Engineering, Bangor University, Bangor, United Kingdom
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A quarter of all marine methane, a potent greenhouse gas, is estimated to be hosted in Southern Ocean sediments. Climate change-induced ocean warming and ice shelf melting risk the stability of sedimentary gas hydrates, resulting in potential degassing and establishment of marine methane seeps. While methane seeps can originate from various sources, the destabilisation of gas hydrates may contribute to the formation and persistence of some active seeps. The impact of these seeps and their risks to the diverse sub-Antarctic and Antarctic benthic shelf fauna is uncertain. As a sentinel for change in the sub-Antarctic and wider Antarctic region, this study explores South Georgia's continental shelf macrobenthic methane seep assemblages, for their diversity, richness, and abundance, and their environmental drivers influencing macrofaunal community composition. Seven of South Georgia's shelf troughs hosting active methane seeps were investigated during RV METEOR's M134 expedition in 2017. Species richness at 11 stations ranged from 19-51 species from a total of 103 species discovered across all sites. Station abundance ranged from 3,303–30,326 m². Diversity was higher at stations with greater methane-and sulfate-flux, and hydrogen sulfide at 25 cm depth. Abundance and richnesswere lowerdecreasedwhere surface sediment had high hydrogen sulfide concentrations. Abundance and species richnesswere lowerdecreaseat stations dominated by iron-reduction in the sediment. Assemblages were characterized by the presence of Southern Ocean species and by the absence of megafaunal chemosynthetic taxa. Arthropods, mostly crustacean, and annelid species made up three quarters of overall species richness, while molluscan and echinoderm species were depauperate with only 15 species. Compared with Southern Ocean macrobenthic assemblages, the South Georgia seep assemblages from sediments with gas hydrates present in the near-surface showed a lower species richness and change in taxon composition, also accompanied by lower numbers of calcium-carbonate shell bearing taxa. The current diverse benthic Antarctic biodiversity, especially the diversity of calcifiers, is likely at risk when methane seeps become established on Southern Ocean continental shelvesas the reduction in habitat diversity leads to the decline in taxonomic diversity and species richness.
Keywords: Hydrocarbon seafloor emission, Sub-Antarctic, microbial mats, Polychaeta, Remotely operated vehicle (ROV), Multicorer samples
Received: 07 Mar 2025; Accepted: 25 Aug 2025.
Copyright: © 2025 Anderson, Reid, Bohrmann, Dohrmann, Hollyman, Kasten, Pape, Römer, Newton, Wigham and Linse. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) or licensor are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.
* Correspondence: Madeline Patricia Brenda Couny Anderson, British Antarctic Survey (BAS), Cambridge, CB3 0ET, United Kingdom
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