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流体地球化学、当地水文学和代谢活动决定了深海热液喷口甲烷菌群落的大小和组成。

Fluid geochemistry, local hydrology, and metabolic activity define methanogen community size and composition in deep-sea hydrothermal vents.

机构信息

Department of Microbiology, University of Massachusetts, Amherst, MA, 01003, USA.

GNS Science, Wellington, 5010, New Zealand.

出版信息

ISME J. 2019 Jul;13(7):1711-1721. doi: 10.1038/s41396-019-0382-3. Epub 2019 Mar 6.

DOI:10.1038/s41396-019-0382-3
PMID:30842565
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC6776001/
Abstract

The size and biogeochemical impact of the subseafloor biosphere in oceanic crust remain largely unknown due to sampling limitations. We used reactive transport modeling to estimate the size of the subseafloor methanogen population, volume of crust occupied, fluid residence time, and nature of the subsurface mixing zone for two low-temperature hydrothermal vents at Axial Seamount. Monod CH production kinetics based on chemostat H availability and batch-culture Arrhenius growth kinetics for the hyperthermophile Methanocaldococcus jannaschii and thermophile Methanothermococcus thermolithotrophicus were used to develop and parameterize a reactive transport model, which was constrained by field measurements of H, CH, and metagenome methanogen concentration estimates in 20-40 °C hydrothermal fluids. Model results showed that hyperthermophilic methanogens dominate in systems where a narrow flow path geometry is maintained, while thermophilic methanogens dominate in systems where the flow geometry expands. At Axial Seamount, the residence time of fluid below the surface was 29-33 h. Only 10 methanogenic cells occupying 1.8-18 m of ocean crust per m of vent seafloor area were needed to produce the observed CH anomalies. We show that variations in local geology at diffuse vents can create fluid flow paths that are stable over space and time, harboring persistent and distinct microbial communities.

摘要

由于采样限制,海底生物圈在海洋地壳中的大小和生物地球化学影响在很大程度上仍然未知。我们使用反应传输建模来估计海底产甲烷菌种群的大小、地壳所占体积、流体停留时间以及轴向海山两个低温热液喷口的地下混合区的性质。基于恒化器 H 可用性的单 CH 生产动力学和嗜热甲烷球菌 Methanocaldococcus jannaschii 和嗜热甲烷球菌 Methanothermococcus thermolithotrophicus 的分批培养 Arrhenius 生长动力学,开发并参数化了一个反应传输模型,该模型受到 20-40°C 热液中 H、CH 和宏基因组产甲烷菌浓度估计的现场测量的约束。模型结果表明,在保持狭窄流路几何形状的系统中,嗜热产甲烷菌占主导地位,而在流路几何形状扩展的系统中,嗜热产甲烷菌占主导地位。在轴向海山,表面以下流体的停留时间为 29-33 小时。仅需 10 个产甲烷细胞,每个喷口海底面积 1.8-18 m 的海洋地壳就可以产生观察到的 CH 异常。我们表明,弥散喷口的局部地质变化可以产生在空间和时间上稳定的流体流动路径,容纳持久而独特的微生物群落。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/95bf/6776001/51ac202bdaf4/41396_2019_382_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/95bf/6776001/eebea4ff3ac4/41396_2019_382_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/95bf/6776001/d329c92aa7bb/41396_2019_382_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/95bf/6776001/226ed465a83e/41396_2019_382_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/95bf/6776001/229751043cd6/41396_2019_382_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/95bf/6776001/51ac202bdaf4/41396_2019_382_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/95bf/6776001/eebea4ff3ac4/41396_2019_382_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/95bf/6776001/d329c92aa7bb/41396_2019_382_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/95bf/6776001/226ed465a83e/41396_2019_382_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/95bf/6776001/229751043cd6/41396_2019_382_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/95bf/6776001/51ac202bdaf4/41396_2019_382_Fig5_HTML.jpg

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