TY - JOUR
T1 - A chemosynthetic ecotone—“chemotone”—in the sediments surrounding deep-sea methane seeps
AU - Ashford, Oliver S.
AU - Guan, Shuzhe
AU - Capone, Dante
AU - Rigney, Katherine
AU - Rowley, Katelynn
AU - Orphan, Victoria
AU - Mullin, Sean W.
AU - Dawson, Kat S.
AU - Cortés, Jorge
AU - Rouse, Greg W.
AU - Mendoza, Guillermo F.
AU - Lee, Raymond W.
AU - Cordes, Erik E.
AU - Levin, Lisa A.
N1 - Funding Information: We are thankful to the Ministerio de Ambiente y Energía of Costa Rica (Sistema Nacional de Áreas de Conservación/Comisión Nacional para la Gestión de la Biodiversidad) for granting collection permits (AT37‐13: SINAC‐CUS‐PI‐R‐035‐2017, AT42‐03: SINAC‐SE‐064‐2018). We are very grateful to the Captains, Crew, Science Party, and team of RV legs AT37‐13 and AT42‐03 for facilitating sample collection. We thank Jennifer Le and Odalisca Breedy, Lillian McCormick, Natalya Gallo, and Olivia Pereira for their help with sectioning and preserving push core samples. We thank Jennifer Gonzalez and Olivia Pereira for their help with processing specimens for stable isotope analysis. We thank Sujung Lim for their part in generating the geochemical data analyzed here. We are grateful to three anonymous reviewers, whose insightful and constructive comments helped to strengthen this article. This work was funded by National Science Foundation Ocean Sciences grant numbers 1634172 and 1635219. Author Oliver S. Ashford additionally received support from Scripps Institution of Oceanography as a Postdoctoral Scholar. Alvin Atlantis Funding Information: We are thankful to the Ministerio de Ambiente y Energía of Costa Rica (Sistema Nacional de Áreas de Conservación/Comisión Nacional para la Gestión de la Biodiversidad) for granting collection permits (AT37-13: SINAC-CUS-PI-R-035-2017, AT42-03: SINAC-SE-064-2018). We are very grateful to the Captains, Crew, Science Party, and Alvin team of RV Atlantis legs AT37-13 and AT42-03 for facilitating sample collection. We thank Jennifer Le and Odalisca Breedy, Lillian McCormick, Natalya Gallo, and Olivia Pereira for their help with sectioning and preserving push core samples. We thank Jennifer Gonzalez and Olivia Pereira for their help with processing specimens for stable isotope analysis. We thank Sujung Lim for their part in generating the geochemical data analyzed here. We are grateful to three anonymous reviewers, whose insightful and constructive comments helped to strengthen this article. This work was funded by National Science Foundation Ocean Sciences grant numbers 1634172 and 1635219. Author Oliver S. Ashford additionally received support from Scripps Institution of Oceanography as a Postdoctoral Scholar. Publisher Copyright: © 2021 Association for the Sciences of Limnology and Oceanography.
PY - 2021/5
Y1 - 2021/5
N2 - Ecotones have been described as “biodiversity hotspots” from myriad environments, yet have not been studied extensively in the deep ocean. While physiologically challenging, deep-water methane seeps host highly productive communities fueled predominantly by chemosynthetic pathways. We hypothesized that the biological and geochemical influence of methane seeps extends into background habitats, resulting in the formation of a “chemotone” where chemosynthesis-based and photosynthesis-based communities overlap. To investigate this, we analyzed the macrofaunal assemblages and geochemical properties of sediments collected from “active,” “transition” (potential chemotone), and “background” habitats surrounding five Costa Rican methane seeps (depth range 377–1908 m). Sediment geochemistry demonstrated a clear distinction between active and transition habitats, but not between transition and background habitats. In contrast, biological variables confirmed the presence of a chemotone, characterized by intermediate biomass, a distinct species composition (including habitat endemics and species from both active and background habitats), and enhanced variability in species composition among samples. However, chemotone assemblages were not distinct from active and/or background assemblages in terms of faunal density, biological trait composition, or diversity. Biomass and faunal stable isotope data suggest that chemotones are driven by a gradient in food delivery, receiving supplements from chemosynthetic production in addition to available photosynthetic-based resources. Sediment geochemistry suggests that chemosynthetic food supplements are delivered across the chemotone at least in part through the water column, as opposed to reflecting exclusively in situ chemosynthetic production in sediments. Management efforts should be cognisant of the ecological attributes and spatial extent of the chemotone that surrounds deep-sea chemosynthetic environments.
AB - Ecotones have been described as “biodiversity hotspots” from myriad environments, yet have not been studied extensively in the deep ocean. While physiologically challenging, deep-water methane seeps host highly productive communities fueled predominantly by chemosynthetic pathways. We hypothesized that the biological and geochemical influence of methane seeps extends into background habitats, resulting in the formation of a “chemotone” where chemosynthesis-based and photosynthesis-based communities overlap. To investigate this, we analyzed the macrofaunal assemblages and geochemical properties of sediments collected from “active,” “transition” (potential chemotone), and “background” habitats surrounding five Costa Rican methane seeps (depth range 377–1908 m). Sediment geochemistry demonstrated a clear distinction between active and transition habitats, but not between transition and background habitats. In contrast, biological variables confirmed the presence of a chemotone, characterized by intermediate biomass, a distinct species composition (including habitat endemics and species from both active and background habitats), and enhanced variability in species composition among samples. However, chemotone assemblages were not distinct from active and/or background assemblages in terms of faunal density, biological trait composition, or diversity. Biomass and faunal stable isotope data suggest that chemotones are driven by a gradient in food delivery, receiving supplements from chemosynthetic production in addition to available photosynthetic-based resources. Sediment geochemistry suggests that chemosynthetic food supplements are delivered across the chemotone at least in part through the water column, as opposed to reflecting exclusively in situ chemosynthetic production in sediments. Management efforts should be cognisant of the ecological attributes and spatial extent of the chemotone that surrounds deep-sea chemosynthetic environments.
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U2 - https://doi.org/10.1002/lno.11713
DO - https://doi.org/10.1002/lno.11713
M3 - Article
SN - 0024-3590
VL - 66
SP - 1687
EP - 1702
JO - Limnology and Oceanography
JF - Limnology and Oceanography
IS - 5
ER -