Microbial metabolism in deep terrestrial subsurface communities - amino acids as biosignatures

The deep terrestrial subsurface (DTS) harbours a striking diversity of microorganisms. However, systematic research on microbial metabolism, and how varying groundwater composition affects the bacterial communities and metabolites in these environments is lacking. In this study, DTS groundwater bacterial consortia from two Fennoscandian Shield sites were enriched and studied. We found that the enriched communities from the two sites consisted of distinct bacterial taxa, and alterations in the growth medium composition induced changes in cell counts. The lack of an exogenous organic carbon source (ECS) caused a notable increase in lipid metabolism in one community, while in the other, carbon starvation resulted in low overall metabolism, suggesting a dormant state. ECS supplementation increased CO2 production and SO4 2- utilisation, suggesting activation of a dissimilatory sulphate reduction pathway and sulphate-reducer-dominated total metabolism. However, both communities shared common universal metabolic features, most probably involving pathways needed for the maintenance of cell homeostasis (e.g., mevalonic acid pathway). Collectively, our findings indicate that the most important metabolites related to microbial reactions under varying growth conditions in enriched DTS communities include, but are not limited to, those linked to cell homeostasis, osmoregulation, lipid biosynthesis and degradation, dissimilatory sulphate reduction and isoprenoid production.

The terrestrial subsurface hosts microbial communities that, collectively, are predicted to comprise as many microbial cells as global surface soils. Although initially thought to be associated with deposited organic matter, deep subsurface microbial communities are supported by chemolithoautotrophic primary production, with hydrogen serving as an important source of electrons. Despite recent progress, relatively little is known about the deep terrestrial subsurface compared to more commonly studied environments. Understanding the composition of deep terrestrial subsurface microbial communities and the factors that influence them is of importance because of human-associated activities including long-term storage of used nuclear fuel, carbon capture, and storage of hydrogen for use as an energy vector. In addition to identifying deep subsurface microorganisms, recent research focuses on identifying the roles of microorganisms in subsurface communities, as well as elucidating myriad interactions—syntrophic, episymbiotic, and viral—that occur among community members. In recent years, entirely new groups of microorganisms (i.e. candidate phyla radiation bacteria and Diapherotrites, Parvarchaeota, Aenigmarchaeota, Nanoloarchaeota, Nanoarchaeota archaea) have been discovered in deep terrestrial subsurface environments, suggesting that much remains unknown about this biosphere. This review explores the historical context for deep terrestrial subsurface microbial ecology and highlights recent discoveries that shape current ecological understanding of this poorly explored microbial habitat. Additionally, we highlight the need for multifaceted experimental approaches to observe phenomena such as cryptic cycles, complex interactions, and episymbiosis, which may not be apparent when using single approaches in isolation, but are nonetheless critical to advancing our understanding of this deep biosphere.

While recent efforts to catalogue Earth’s microbial diversity have focused upon surface and marine habitats, 12–20 % of Earth’s biomass is suggested to exist in the terrestrial deep subsurface, compared to ~1.8 % in the deep subseafloor. Metagenomic studies of the terrestrial deep subsurface have yielded a trove of divergent and functionally important microbiomes from a range of localities. However, a wider perspective of microbial diversity and its relationship to environmental conditions within the terrestrial deep subsurface is still required. Our meta-analysis reveals that terrestrial deep subsurface microbiota are dominated by Betaproteobacteria, Gammaproteobacteria and Firmicutes, probably as a function of the diverse metabolic strategies of these taxa. Evidence was also found for a common small consortium of prevalent Betaproteobacteria and Gammaproteobacteria operational taxonomic units across the localities. This implies a core terrestrial deep subsurface community, irrespective of aquifer lithology, depth and other variables, that may play an important role in colonizing and sustaining microbial habitats in the deep terrestrial subsurface. An in silico contamination-aware approach to analysing this dataset underscores the importance of downstream methods for assuring that robust conclusions can be reached from deep subsurface-derived sequencing data. Understanding the global panorama of microbial diversity and ecological dynamics in the deep terrestrial subsurface provides a first step towards understanding the role of microbes in global subsurface element and nutrient cycling.

A novel, obligately anaerobic bacterium (strain SURF-ANA1T) was isolated from deep continental subsurface fluids at a depth of 1500 m below surface in the former Homestake Gold Mine (now Sanford Underground Research Facility, in Lead, South Dakota, USA). Cells of strain SURF-ANA1T were Gram-negative, helical, non-spore-forming and were 0.25-0.55×5.0-75.0 µm with a wavelength of 0.5-0.62 µm. Strain SURF-ANA1T grew at 15-50 °C (optimally at 40 °C), at pH 4.8-9.0 (pH 7.2) and in 1.0-40.0 g l-1 NaCl (10 g l-1 NaCl). The strain grew chemoheterotrophically with hydrogen or mono-, di- and polysaccharides as electron donors. The major cellular fatty acids in order of decreasing abundance (comprising >5% of total) were 10-methyl C16:0, iso-C15:0, C18:2 and C18:0 dimethyl acetal (DMA) and C20:0 methylene-nonadecanoic acid. Phylogenetic analysis based on the 16S rRNA gene sequence of strain SURF-ANA1T indicated a closest relationship with the recently characterized Rectinema cohabitans (99%). Despite high sequence identity, because of its distinct physiology, morphology and fatty acid profile, strain SURF-ANA1T is considered to represent a novel species within the genus Rectinema, for which the name Rectinema subterraneum sp. nov. is proposed. To our knowledge, this is the first report of an isolate within the phylum Spirochaetes from the deep (>100 m) terrestrial subsurface. The GenBank/EMBL/DDBJ accession numbers for the 16S rRNA gene and genomic sequences of strain SURF-ANA1T are KU359248 and GCF 009768935.1, respectively. The type strain of Rectinema subterraneum is SURF-ANA1T (=ATCC TSD-67=JCM 32656).

Earth's deep subsurface biosphere (DSB) is home to a vast number and wide variety of microorganisms. Although difficult to access and sample, deep subsurface environments have been probed through drilling programs, exploration of mines and sampling of deeply sourced vents and springs. In an effort to understand the ecology of deep terrestrial habitats, we examined bacterial diversity in the Sanford Underground Research Facility (SURF), the former Homestake gold mine, in South Dakota, USA. Whole genomic DNA was extracted from deeply circulating groundwater and corresponding host rock (at a depth of 1.45 km below ground surface). Pyrotag DNA sequencing of the 16S rRNA gene revealed diverse communities of putative chemolithoautotrophs, aerobic and anaerobic heterotrophs, numerous candidate phyla and unique rock-associated microbial assemblage. There was a clear and near-total separation of communities between SURF deeply circulating fracture fluids and SURF host-rocks. Sequencing data from SURF compared against five similarly sequenced terrestrial subsurface sites in Europe and North America revealed classes Clostridia and Betaproteobacteria were dominant in terrestrial fluids. This study presents a unique analysis showing differences in terrestrial subsurface microbial communities between fracture fluids and host rock through which those fluids permeate.

The metal resistance of 350 subsurface bacterial strains from two U.S. Department of Energy facilities, the Savannah River Site (SRS), South Carolina, and the Hanford site, Washington, was determined to assess the effect of metal toxicity on microorganisms in the deep terrestrial subsurface. Resistance was measured by growth inhibition around discs containing optimized amounts of Hg(II), Pb(II), and Cr(VI). A broad range of resistance levels was observed, with some strains of Arthrobacter spp. demonstrating exceptional tolerance. A higher level of resistance to Hg(II) and Pb(II) (P < 0.05) and a higher occurrence of multiple resistances suggested that metals more effectively influenced microbial evolution in subsurface sediments of the SRS than in those of the Hanford site. Common resistance to heavy metals suggests that toxic metals are unlikely to inhibit bioremediation in deep subsurface environments that are contaminated with mixed wastes.

Hydraulic fracturing is the industry standard for extracting hydrocarbons from shale formations. Attention has been paid to the economic benefits and environmental impacts of this process, yet the biogeochemical changes induced in the deep subsurface are poorly understood. Recent single-gene investigations revealed that halotolerant microbial communities were enriched after hydraulic fracturing. Here, the reconstruction of 31 unique genomes coupled to metabolite data from the Marcellus and Utica shales revealed that many of the persisting organisms play roles in methylamine cycling, ultimately supporting methanogenesis in the deep biosphere. Fermentation of injected chemical additives also sustains long-term microbial persistence, while thiosulfate reduction could produce sulfide, contributing to reservoir souring and infrastructure corrosion. Extensive links between viruses and microbial hosts demonstrate active viral predation, which may contribute to the release of labile cellular constituents into the extracellular environment. Our analyses show that hydraulic fracturing provides the organismal and chemical inputs for colonization and persistence in the deep terrestrial subsurface.

A freshly intersected water-bearing fracture zone from the Mponeng Au mine located in the Witwatersrand Basin, Republic of South Africa was sampled, providing an opportunity to examine the natural, deep subsurface biosphere. The fracture, intersected by an advancing tunnel 2.8 kilometers below land surface, possessed a millimeter thick layer of chlorite group minerals, i.e., chamosite, at the water-mineral interface. Water flowing out from the fracture zone had a temperature of 52°C, pH of 9.16 and Eh of −263 mV. Using scanning electron microscopy, the water-mineral interface was generally found to be clean, i.e., it did not possess any secondary mineral or dominant organic coatings. Irregular patches (10's of μm 2 ) of organic material, however, resembling bacterial exopolysaccharides, occurred in the presence or absence of bacteria. The surface was colonized by highly dispersed individual bacteria or by microcolonies containing up to 5 cells, with an overall cell density of 5 × 104 bacteria cm −2 . This biofilm population, although low, was 2 orders of magnitude greater than the bacteria present within the aqueous phase and provides the first direct observation of the sessile population from the terrestrial deep subsurface. Time of Flight-Secondary Ion Mass spectrometry revealed that the fracture surface was actually coated with a thin, i.e., molecular, organic conditioning film over much of its surface that was separate from the exopolysaccharide layers associated with the mineral water interface and with some of the attached cells.

The deep subsurface biosphere has been regarded as an emerging topic in geo-bioscience and industry for the past few decades, and has been approached by terrestrial and seafloor drillings. Terrestrial sites have better proximity and greater relevance to the anthroposphere and technosphere, i.e., human habitats and societies, than do seafloor sites. Therefore, understanding the subterranean biosphere has more direct importance to issues related to a sustainable civilization, and issues such as formation/maturation of hydrocarbon reservoirs and ore deposits, disposal of radioactive wastes and carbon dioxide, and postulated association between seismogenic and microbial activities. Microbiological studies in the terrestrial deep subsurface have been prompted to respond to such human-related issues, and microbial life in sedimentary and crystalline rocks as well as pore-filling fluids has been studied to evaluate rock stability and (im) mobilization of redox-sensitive elements/nuclides, for instance. This is in contrast to subseafloor microbiology, which focuses more on microbial interactions with hydrothermal circulation, relevant biogeochemical processes including gas hydrate formation, associated diversity of life, and modern analogs of origin-of-life. Avoiding man-induced contamination of cored samples and pumped fluids has been a microbiological issue. Technical (both instrumental and operational) measures to minimize contamination were first developed in subterranean microbiology, because of easier accesses to test sites for repetition, evaluation, improvement, etc. of attempted measures on land. Then, anti-contamination expertise was introduced into subseafloor practices, and anti-contamination protocols and facilities are now better developed by the Integrated Ocean Drilling Program (IODP) than the International Continental Scientific Drilling Program (ICDP). Newly developed techniques are also applied to measure/monitor geological and geochemical parameters that are used to characterize microbial habitats and processes occurring there. Lessons from subterranean microbiology are directly applicable to subglacial microbiology that may retrieve microbial life from sub-million-year-old ice cores, although additional measures are needed for glacier drilling. Because land and icy surfaces are common in Earth-like planets or potentially life-bearing satellites, lessons (experiences and expertise) from subterranean microbiology should be applicable to astrobiological searches for extraterrestrial life.

Geomicrobiological properties of Tertiary sedimentary rocks from the deep terrestrial subsurface

The deep terrestrial subsurface is the largest reservoir of Earth’s freshwater resources as well as the largest habitat for prokaryotic life. However, the deep-subsurface microbiome, especially its spatial distribution across countries/continents, is still poorly understood. In this study, we compiled and compared 30 16S rRNA gene amplicon libraries from three deep fractured aquifers in different parts of the world (depth range of tens of meters to 2.4 km below surface) to understand the spatial distribution and functions of deep-subsurface microbial community, and to test for the presence of core taxa. The results revealed spatially heterogenous microbial community composition at both the local and the global scales, even at the phylum level. Environmental filtering was identified as an important driver of the microbial community structure of deep groundwaters. Despite the spatial heterogeneity, the three aquifers share a core microbiome at the genus level. Only one family, Comamonadaceae, was present in all the 30 samples analyzed. Several other families were also prevalent, including Hydrogenophilaceae, Omnitrophaceae, BSV26 (Candidatus Kryptonia), and an unclassified Thermodesulfovibrionia. FAPROTAX functional prediction indicated that chemoheterotrophic functions predominate, and the core microbial genera, together with the dominant genera, collectively govern the functional characteristics. Taken together, our findings provide new insights into the spatial heterogeneity and functional potential of deep-subsurface ecosystems across the globe.

Decomposition of humic substances (HSs) is a slow and cryptic but non-negligible component of carbon cycling in sediments. Aerobic decomposition of HSs by microorganisms in the surface environment has been well documented; however, the mechanism of anaerobic microbial decomposition of HSs is not completely understood. Moreover, no microorganisms capable of anaerobic decomposition of HSs have been isolated. Here, we report the anaerobic decomposition of humic acids (HAs) by the anaerobic bacterium Clostridium sp. HSAI-1 isolated from the deep terrestrial subsurface. The use of 14C-labelled polycatechol as an HA analogue demonstrated that the bacterium decomposed this substance up to 7.4% over 14 days. The decomposition of commercial and natural HAs by the bacterium yielded lower molecular mass fractions, as determined using high-performance size-exclusion chromatography. Fourier transform infrared spectroscopy revealed the removal of carboxyl groups and polysaccharide-related substances, as well as the generation of aliphatic components, amide and aromatic groups. Therefore, our results suggest that Clostridium sp. HSAI-1 anaerobically decomposes and transforms HSs. This study improves our understanding of the anaerobic decomposition of HSs in the hidden carbon cycling in the Earth’s subsurface.

The deep terrestrial subsurface remains an environment where there is limited understanding of the extant microbial metabolisms. At Olkiluoto, Finland, a deep geological repository is under construction for the final storage of spent nuclear fuel. It is therefore critical to evaluate the potential impact microbial metabolism, including sulfide generation, could have upon the safety of the repository. We investigated a deep groundwater where sulfate is present, but groundwater geochemistry suggests limited microbial sulfate-reducing activity. Examination of the microbial community at the genome-level revealed microorganisms with the metabolic capacity for both oxidative and reductive sulfur transformations. Deltaproteobacteria are shown to have the genetic capacity for sulfate reduction and possibly sulfur disproportionation, while Rhizobiaceae, Rhodocyclaceae, Sideroxydans, and Sulfurimonas oxidize reduced sulfur compounds. Further examination of the proteome confirmed an active sulfur cycle, serving for microbial energy generation and growth. Our results reveal that this sulfide-poor groundwater harbors an active microbial community of sulfate-reducing and sulfide-oxidizing bacteria, together mediating a sulfur cycle that remained undetected by geochemical monitoring alone. The ability of sulfide-oxidizing bacteria to limit the accumulation of sulfide was further demonstrated in groundwater incubations and highlights a potential sink for sulfide that could be beneficial for geological repository safety.

Marine sponges are increasingly being recognised for their nutrient cycling ecosystem services, linking pelagic nutrients with the benthic ecosystem. Furthermore, sponges are the most prolific producers of bioactive secondary metabolites in the marine environment. Despite their ecological and commercial value, little is know about the metabolic processes that are responsible. The inability to produce sufficient sponge biomass, and thus specific bioactive compounds, has been repeatedly identified as a major bottleneck towards commercialising sponge holobiont derived drugs. Likewise, nutrient cycling by sponges has been a relatively recent advancement in marine ecology and the scale of this process is unknown. This thesis takes a systems approach to understanding sponge-symbiont metabolic processes by utilising the genomic resources available for the demosponge Amphimedon queenslandica and its bacterial symbiont AqS1. Specifically, I undertake genome-scale modelling and metabolic flux analyses to investigate the metabolic networks present in this sponge as well as its associated vertically-transmitted microbial symbiont. The goal of this thesis is to generate the data required for, and subsequently develop, a dual-species genome-scale metabolic model for A. queenslandica and AqS1. This will provide a framework to further our understanding of how sponges produce their biomass while living in an oligotrophic, tropical reef environment. To develop a genome-scale metabolic model, the biochemical composition of the organism must first be determined. Knowledge of the relative quantities of macromolecules and their respective building blocks (e.g. protein and amino acids) is vital, as each requires different substrates, enzymes and cofactors for their synthesis. I adapted and developed methods to characterise the composition and abundance of DNA, RNA, protein, lipids and carbohydrates in a marine sponge. These methods are described in detail that allows them to be easily transferred to other, non-model, large marine organisms. This is followed by a detailed analysis of A. queenslandica’s macromolecular, amino acid, fatty acid and sterol composition. The biochemical data from this chapter was used to generate a biomass equation that represent the average composition of adult A. queenslandica in the metabolic model. To understand how the metabolic network may work towards producing more biomass, it must be considered in the context of the environmental conditions that naturally constrain growth. The dominant environmental constraint on growth on an oligotrophic reef system is nutrient availability. The abundance of key elements, such as carbon and nitrogen, were quantified throughout the course of a year. To investigate effects on the sponge of any changes in nutrient availability, I concurrently sampled sponges and analysed their biochemical composition to the macromolecular level. Chapter 4 presents these data and discusses a number of trends and correlations in the biochemical composition of the sponges with changing nutrient availability through four seasons of the year. For instance, there was a significant increase in particulate to dissolved organic carbon at the end of summer with a corresponding rise in carbohydrates in A. queenslandica. Of particular importance for the subsequent metabolic modelling, was the separation of carbon into the dissolved and particulate fractions. Chapter 5 presents the metabolic models and their analysis. Initially, I manually constructed a genome-scale metabolic model for the sponge A. queenslandica. The model construction identified 10 amino acids, 4 vitamins and a plant-derived phytosterol for which A. queenslandica is auxotrophic. These represent nutrients that are essential for sponge growth and may in future form the basis of a defined cell culture medium. The microbial community within A. queenslandica is relatively simple and dominated by a species of sulfur oxidising bacteria, called Aqs1. I generated a genome-scale model for Aqs1, which is able to synthesise all 20 proteinogenic amino acids, in addition to having a diverse range of carbohydrate-specific transporters and enzymes. To investigate the interactions between the host sponge and Aqs1, the two models were joined using a shared compartment. This was called the extracellular matrix, and represents the area of interaction within the sponge body where metabolite transfers can occur. I measured the pumping rate of A. queenslandica and calculated the average volume of water pumped per hour, standardised to gram dry weight. This was used to constrain the nutrient uptake rate of the model. To investigate how the metabolic network may respond to different nutrient conditions, low and high nutrient conditions were defined using the ratios of particulate and dissolved carbon from the seasonal environmental profiling. This work represents the first genome-scale model for a sponge-symbiont system, and marine invertebrates in general. The genome-scale metabolic models resulting from this work are an important resource that will guide future work into the metabolic processes of both A. queenslandica and its symbiont, Aqs1.

Complete Genome Sequences of Five Gram-Negative Bacterial Strains Comprising Synthetic Bacterial Consortium "The Great Five" with Antagonistic Activity Against Plant-Pathogenic Pectobacterium spp. and Dickeya spp.