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      Patterns of in situ Mineral Colonization by Microorganisms in a ~60°C Deep Continental Subsurface Aquifer

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          Abstract

          The microbial ecology of the deep biosphere is difficult to characterize, owing in part to sampling challenges and poorly understood response mechanisms to environmental change. Pre-drilled wells, including oil wells or boreholes, offer convenient access, but sampling is frequently limited to the water alone, which may provide only a partial view of the native diversity. Mineral heterogeneity demonstrably affects colonization by deep biosphere microorganisms, but the connections between the mineral-associated and planktonic communities remain unclear. To understand the substrate effects on microbial colonization and the community response to changes in organic carbon, we conducted an 18-month series of in situ experiments in a warm (57°C), anoxic, fractured carbonate aquifer at 752 m depth using replicate open, screened cartridges containing different solid substrates, with a proteinaceous organic matter perturbation halfway through this series. Samples from these cartridges were analyzed microscopically and by Illumina (iTag) 16S rRNA gene libraries to characterize changes in mineralogy and the diversity of the colonizing microbial community. The substrate-attached and planktonic communities were significantly different in our data, with some taxa (e.g., Candidate Division KB-1) rare or undetectable in the first fraction and abundant in the other. The substrate-attached community composition also varied significantly with mineralogy, such as with two Rhodocyclaceae OTUs, one of which was abundant on carbonate minerals and the other on silicic substrates. Secondary sulfide mineral formation, including iron sulfide framboids, was observed on two sets of incubated carbonates. Notably, microorganisms were attached to the framboids, which were correlated with abundant Sulfurovum and Desulfotomaculum sp. sequences in our analysis. Upon organic matter perturbation, mineral-associated microbial diversity differences were temporarily masked by the dominance of putative heterotrophic taxa in all samples, including OTUs identified as Caulobacter, Methyloversatilis, and Pseudomonas. Subsequent experimental deployments included a methanogen-dominated stage ( Methanobacteriales and Methanomicrobiales) 6 months after the perturbation and a return to an assemblage similar to the pre-perturbation community after 9 months. Substrate-associated community differences were again significant within these subsequent phases, however, demonstrating the value of in situ time course experiments to capture a fraction of the microbial assemblage that is frequently difficult to observe in pre-drilled wells.

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          QIIME allows analysis of high-throughput community sequencing data.

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            Ultra-high-throughput microbial community analysis on the Illumina HiSeq and MiSeq platforms

            DNA sequencing continues to decrease in cost with the Illumina HiSeq2000 generating up to 600 Gb of paired-end 100 base reads in a ten-day run. Here we present a protocol for community amplicon sequencing on the HiSeq2000 and MiSeq Illumina platforms, and apply that protocol to sequence 24 microbial communities from host-associated and free-living environments. A critical question as more sequencing platforms become available is whether biological conclusions derived on one platform are consistent with what would be derived on a different platform. We show that the protocol developed for these instruments successfully recaptures known biological results, and additionally that biological conclusions are consistent across sequencing platforms (the HiSeq2000 versus the MiSeq) and across the sequenced regions of amplicons.
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              The biomass distribution on Earth

              Significance The composition of the biosphere is a fundamental question in biology, yet a global quantitative account of the biomass of each taxon is still lacking. We assemble a census of the biomass of all kingdoms of life. This analysis provides a holistic view of the composition of the biosphere and allows us to observe broad patterns over taxonomic categories, geographic locations, and trophic modes.
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                Author and article information

                Contributors
                Journal
                Front Microbiol
                Front Microbiol
                Front. Microbiol.
                Frontiers in Microbiology
                Frontiers Media S.A.
                1664-302X
                19 November 2020
                2020
                : 11
                : 536535
                Affiliations
                [1] 1Division of Geological and Planetary Sciences, California Institute of Technology , Pasadena, CA, United States
                [2] 2Jet Propulsion Laboratory , Pasadena, CA, United States
                [3] 3Division of Hydrologic Sciences, Desert Research Institute , Las Vegas, NV, United States
                [4] 4Department of Microbiology, Southern Illinois University Carbondale , Carbondale, IL, United States
                [5] 5Department of Earth Sciences, University of Southern California , Los Angeles, CA, United States
                Author notes

                Edited by: Trinity L. Hamilton, University of Minnesota Twin Cities, United States

                Reviewed by: Matthew Schrenk, Michigan State University, United States; Christen Lynn Grettenberger, University of California, Davis, United States

                *Correspondence: Victoria J. Orphan, vorphan@ 123456gps.caltech.edu

                Present address: Greg Wanger, Oberland Agriscience Inc., Halifax, NS, Canada

                Rohit Bhartia, Photon Systems, Inc., Covina, CA, United States

                This article was submitted to Microbiological Chemistry and Geomicrobiology, a section of the journal Frontiers in Microbiology

                Article
                10.3389/fmicb.2020.536535
                7711152
                33329414
                7dc1d9c7-5906-4377-846a-24a195c45b37
                Copyright © 2020 Mullin, Wanger, Kruger, Sackett, Hamilton-Brehm, Bhartia, Amend, Moser and Orphan.

                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) and the copyright owner(s) 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.

                History
                : 20 February 2020
                : 24 September 2020
                Page count
                Figures: 5, Tables: 1, Equations: 1, References: 109, Pages: 19, Words: 16706
                Funding
                Funded by: NASA Astrobiology Institute 10.13039/100012627
                Award ID: NNA13AA92A
                Funded by: Center for Dark Energy Biosphere Investigations (C-DEBI) 10.13039/100013505
                Funded by: NIH
                Funded by: NASA Space Grant Consortium Fellowship
                Categories
                Microbiology
                Original Research

                Microbiology & Virology
                microbial ecology,deep biosphere,fractured rock,mineral colonization,microbial succession,carbonate,pyrite,methanogenesis

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