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ORIGINAL RESEARCH article

Front. Microbiol.
Sec. Extreme Microbiology
Volume 15 - 2024 | doi: 10.3389/fmicb.2024.1455594
This article is part of the Research Topic Deep Subsurface Microbiology and Energetics View all 7 articles

Calorimetric measurement of energy and nutrient stimulation of microorganisms from the continental deep subsurface

Provisionally accepted
  • 1 Department of Earth Sciences, University of Southern California, Los Angeles, United States
  • 2 School of Life Sciences, Eastern Institute of Technology, Ningbo, China
  • 3 GeoZentrum Nordbayern, Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen, Germany
  • 4 Department of Biological Sciences, University of Southern California, Los Angeles, United States
  • 5 Division of Hydrologic Sciences, Desert Research Institute, Las Vegas, Nevada, United States
  • 6 Department of Earth and Planetary Sciences, Northwestern University, Evanston, Illinois, United States
  • 7 Department of Biological Sciences, Dornsife College of Letters, Arts and Sciences, University of Southern California, Los Angeles, California, United States

The final, formatted version of the article will be published soon.

    Microbial activity in the deep continental subsurface is difficult to measure due to low cell densities, low energy fluxes, cryptic elemental cycles and enigmatic metabolisms. Nonetheless, direct access to rare sample sites and sensitive laboratory measurements can be used to better understand the variables that govern microbial life underground. In this study, we sampled fluids from six boreholes at depths ranging from 244 m to 1478 m below ground at the Sanford Underground Research Facility (SURF), a former goldmine in South Dakota, USA. The heat produced by microorganisms in these samples was measured in a nanocalorimeter as a proxy for activity. Heat flow measurements on unamended groundwater samples from five of the six boreholes comprising the Deep Underground Microbial Observatory (DeMMO) fell below the limit of detection, suggesting very low metabolic rates. Fluid samples from the borehole that registered a heat signal (DeMMO 6) from 1478 m deep, were amended with a series of electron donors, electron acceptors, and amino acids before being introduced into the calorimeter. The addition of formate resulted in more than a ~500 nW increase in heat flow relative to the signal for unamended fluids during the first 100 hours of incubation while the next highest heat flow arose from nitrate and acetate co-addition, at ~125 nW. Notably, both amendment conditions led to a ~1.5 orders of magnitude increase in cell density without causing major changes to community composition, suggesting that these electron donors and acceptors may be exploited by these communities in-situ. The addition of ~0.4 mM casamino acids resulted in a total heat flow of 2.25 uW within 35 hours and a more than three orders of magnitude increase in cell density. In these experiments, Hydrogenophaga grew to dominate the amino acid amended borehole fluids. The strong microbial response to amino acid addition indicates a deep continental surface community that is limited by the availability of amino acids. A high potential for amino acid metabolism was proposed in genomic studies from this and similar sites but has not been shown in actively growing communities.

    Keywords: calorimetry1, deep biosphere2, Sanford Underground Research Facility3, nutrient limitation4, microbial activity5. (Min.5-Max. 8

    Received: 27 Jun 2024; Accepted: 04 Dec 2024.

    Copyright: © 2024 Feyhl-Buska, Wu, Smith, LaRowe, Robador, Kruger, Osburn and Amend. 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) or licensor 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.

    * Correspondence: Jayme Feyhl-Buska, Department of Earth Sciences, University of Southern California, Los Angeles, United States

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