Abstract

Abstract. The bacterial and archaeal community composition and the possible carbon assimilation processes and energy sources of microbial communities in oligotrophic, deep, crystalline bedrock fractures is yet to be resolved. In this study, intrinsic microbial communities from groundwater of six fracture zones from 180 to 2300 m depths in Outokumpu bedrock were characterized using high-throughput amplicon sequencing and metagenomic prediction. Comamonadaceae-, Anaerobrancaceae- and Pseudomonadaceae-related operational taxonomic units (OTUs) form the core community in deep crystalline bedrock fractures in Outokumpu. Archaeal communities were mainly composed of Methanobacteriaceae-affiliating OTUs. The predicted bacterial metagenomes showed that pathways involved in fatty acid and amino sugar metabolism were common. In addition, relative abundance of genes coding the enzymes of autotrophic carbon fixation pathways in predicted metagenomes was low. This indicates that heterotrophic carbon assimilation is more important for microbial communities of the fracture zones. Network analysis based on co-occurrence of OTUs revealed possible “keystone” genera of the microbial communities belonging to Burkholderiales and Clostridiales. Bacterial communities in fractures resemble those found in oligotrophic, hydrogen-enriched environments. Serpentinization reactions of ophiolitic rocks in Outokumpu assemblage may provide a source of energy and organic carbon compounds for the microbial communities in the fractures. Sulfate reducers and methanogens form a minority of the total microbial communities, but OTUs forming these minor groups are similar to those found in other deep Precambrian terrestrial bedrock environments.

Highlights

  • The microbial communities in deep terrestrial subsurface biosphere contribute significantly to the overall biomass on Earth (Whitman et al, 1998; McMahon and Parnell, 2014)

  • Chemolithoautotrophic organisms are thought to be the primary producers in deep crystalline rock environments, into which sunlight, organic carbon or oxygen produced in photosynthesis do not penetrate (Gold, 1992; Pedersen, 1997, 2000)

  • A similar trend was observed with the copy numbers of the bacterial 16S rRNA gene ranging from 5.13 × 106 in shallowest fracture to 9.00 × 102 in the deepest fracture

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Summary

Introduction

The microbial communities in deep terrestrial subsurface biosphere contribute significantly to the overall biomass on Earth (Whitman et al, 1998; McMahon and Parnell, 2014). Energy and carbon sources for deep biosphere have to be geochemical. The most important source of reducing power in deep subsurface is H2. It is produced in abiotic reactions such as through radiolysis of H2O and in water–rock interactions such as serpentinization, and by microbial activity (Pedersen, 2000; Lin et al, 2005; McCollom, 2013; Szponar et al, 2013). Carbon sources for microbes in deep subsurface are usually in the form of CO2, CH4 or other small hydrocarbons.

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