Microbial biofilms associated with fluid chemistry and megafaunal colonization at post-eruptive deep-sea hydrothermal vents
Introduction
Studies of diffuse-flow hydrothermal vents at 9°50′N on the East Pacific Rise (hereafter referred to as EPR) following seafloor volcanic eruptions (in 1991 and 2006) have provided information about processes controlling the initial colonization by microbial biofilms and subsequent succession of vent metazoans (Shank et al., 1998, Govenar, 2012, Sievert and Vetriani, 2012). While, in general, metazoan colonization correlates with temperature and hydrothermal fluid chemistry (Shank et al., 1998, Luther et al., 2001, Luther et al., 2012), biological interactions may also play a role in colonization patterns (e.g., Mullineaux et al., 2003; Govenar et al., 2012). Many vent invertebrates rely on chemosynthetic microorganisms that convert the energy of the reduced chemical species dissolved in the hydrothermal fluids into biochemical energy (ATP) to fix carbon dioxide. Also, in other marine habitats, microbial cues of metazoan settlement are critically important. Dispersive larvae respond not only to the texture and composition of microorganisms in biofilms, but also to chemicals produced by microbial consortia or individual microbial species (reviewed by Underwood and Keough, 2001, Hadfield, 2011). In addition, metamorphosis from the free-swimming larval stage to the sessile adult stage can be initiated by a different composition of the biofilms (Tebben et al., 2011, Yang et al., 2013).
Hence, chemosynthetic microorganisms may provide useful cues that indicate habitat quality for metazoan colonizers. Indeed, biologists have long hypothesized that microbial biofilms at deep-sea hydrothermal vents may interact with vent larvae to induce settlement and metamorphosis (Van Dover, 2000, Adams et al., 2012). However, this hypothesis remains largely untested.
Direct observation of the colonization of diffuse-flow vents following a volcanic eruption on the EPR has shown that microbial biofilms are the pioneer colonizers of newly-formed vents (Lutz et al., 2001, Sievert and Vetriani, 2012). Further, small subunit rRNA gene surveys of vent microbial communities indicated that Epsilonproteobacteria were the dominant microorganisms associated with the colonization of substrates, as well as the most abundant primary producers at diffuse-flow hydrothermal vents (Lopez-Garcia et al., 2003, Alain et al., 2004, Campbell et al., 2006, Sievert and Vetriani, 2012).
In December 2003, we initiated colonization studies at diffuse-flow vents located on the EPR to examine the correlation between microbial and megafaunal colonizers. In late 2005/early 2006, a volcanic seafloor eruption buried many of the pre-existing benthic communities in fresh lava (Cowen et al., 2007). The eruption also created more than 20 nascent vent habitats, establishing a time-zero for subsequent biological colonization and community development. While previous studies have documented post-eruptive changes in the chemistry of diffuse-vent fluids (Shank et al., 1998, Von Damm and Lilley, 2004), an integrated investigation that simultaneously examined the structure of early microbial colonists, megafaunal colonization and fluid chemistry in diffuse-flow vents had not been conducted.
Here we conducted time-series in situ experiments to examine patterns of microbial community structure and composition, fluid temperature and chemistry and megafaunal colonization at various post-eruptive diffuse-flow vents on the EPR. The goal of this study was to examine for the first time co-located linkages between hydrothermal fluid chemistry, microbial biofilms and megafaunal colonization. Specifically, amongst newly-formed, post-eruptive vents, we aimed to: (1) characterize the composition of microbial colonizers; (2) correlate patterns of microbial colonization in response to different geochemical regimes; and (3) examine patterns of megafaunal colonization. Our findings revealed marked differences in the composition of microbial biofilms and vent-endemic megafaunal colonization at hydrothermally active (in-flow) and inactive (no-flow) areas.
Section snippets
Site description and sampling strategy
To investigate patterns of microbial and megafaunal colonization at post-eruptive hydrothermal vents in relationship to different thermal and geochemical regimes, we designed and deployed experimental colonization substrates that allow the coordination and integration of these data. The substrates, hereafter referred to as TAMS (Temporal Autonomous Multi-disciplinary Substrates), were designed to allow hydrothermal fluids to pass through the colonization surface. Each surface was constructed
Fluid temperature and chemistry
Temperature, oxygen and sulfide concentration were measured in situ on TAMS during deployment and recovery using the solid-state microelectrodes and the temperature sensor. Additionally, temperatures were recorded using VEMCO data loggers directly above the mesh of each TAMS for the entire duration of the deployment. The results of the in situ measurements are reported in Table 2. The temperatures measured with the manipulator-held sensor during the deployment and recovery of the TAMS were
Discussion
Microbial biofilms are important for marine invertebrate recruitment in a variety of habitats. While early evidence suggested that it was the texture or the composition of micoorganisms that increased habitat suitability for settling larvae, additional work has demonstrated the importance of chemical signals produced by microbial consortia or individual species of bacteria that indicate a particular area as suitable for colonization (reviewed by Underwood and Keough, 2001, Hadfield, 2011).
Acknowledgements
This work was supported by National Science Foundation grants MCB-0456676 and OCE-1136451 to CV, OCE-0327353 and OCE-0937371 to RAL and CV, OCE-0326434 and OCE-0937324 to GWL, OCE-0327261 to TMS, OCE-0937395 to TMS and BG, by grant NA04OAR4600084 from the Office of Ocean Exploration (National Oceanic and Atmospheric Administration) to TMS, by a grant from the Deep Ocean Exploration Institute (Woods Hole Oceanographic Institution) to TMS, a Postdoctoral Fellowship from the Institute of Marine
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