Cool, alkaline serpentinite formation fluid regime with scarce microbial habitability and possible abiotic synthesis beneath the South Chamorro Seamount

dc.contributor.author Kawagucci, Shinsuke
dc.contributor.author Miyazaki, Junichi
dc.contributor.author Morono, Yuki
dc.contributor.author Seewald, Jeffrey S.
dc.contributor.author Wheat, C. Geoffrey
dc.contributor.author Takai, Ken
dc.date.accessioned 2018-11-29T16:58:31Z
dc.date.available 2018-11-29T16:58:31Z
dc.date.issued 2018-11-14
dc.description © The Author(s), 2018. This article is distributed under the terms of the Creative Commons Attribution License. The definitive version was published in Progress in Earth and Planetary Science 5 (2018): 74, doi:10.1186/s40645-018-0232-3. en_US
dc.description.abstract South Chamorro Seamount (SCS) is a blueschist-bearing serpentinite mud volcano in the Mariana forearc. Previous scientific drilling conducted at SCS revealed highly alkaline, sulfate-rich formation fluids resulting from slab-derived fluid upwelling combined with serpentinization both beneath and within the seamount. In the present study, a time-series of ROV dives spanning 1000 days was conducted to collect discharging alkaline fluids from the cased Ocean Drilling Program (ODP) Hole 1200C (hereafter the CORK fluid). The CORK fluids were analyzed for chemical compositions (including dissolved gas) and microbial community composition/function. Compared to the ODP porewater, the CORK fluids were generally identical in concentration of major ions, with the exception of significant sulfate depletion and enrichment in sulfide, alkalinity, and methane. Microbiological analyses of the CORK fluids revealed little biomass and functional activity, despite habitable temperature conditions. The post-drilling sulfate depletion is likely attributable to sulfate reduction coupled with oxidation of methane (and hydrogen), probably triggered by the drilling and casing operations. Multiple lines of evidence suggest that abiotic organic synthesis associated with serpentinization is the most plausible source of the abundant methane in the CORK fluid. The SCS formation fluid regime presented here may represent the first example on Earth where abiotic syntheses are conspicuous with little biotic processes, despite a condition with sufficient bioavailable energy potentials and temperatures within the habitable range. en_US
dc.description.sponsorship This work was partly supported by JSPS KAKENHI Grant Number 25701004 (SK). en_US
dc.identifier.citation Progress in Earth and Planetary Science 5 (2018): 74 en_US
dc.identifier.doi 10.1186/s40645-018-0232-3
dc.identifier.uri https://hdl.handle.net/1912/10737
dc.language.iso en_US en_US
dc.publisher Springer en_US
dc.relation.uri https://doi.org/10.1186/s40645-018-0232-3
dc.rights Attribution 4.0 International *
dc.rights.uri http://creativecommons.org/licenses/by/4.0/ *
dc.subject Forearc serpentinite mud volcano en_US
dc.subject South Chamorro Seamount en_US
dc.subject Limit of biosphere en_US
dc.subject Present-days’ chemical evolution en_US
dc.subject Radio-isotope-tracer carbon assimilation estimation en_US
dc.title Cool, alkaline serpentinite formation fluid regime with scarce microbial habitability and possible abiotic synthesis beneath the South Chamorro Seamount en_US
dc.type Article en_US
dspace.entity.type Publication
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