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    Life Underground: Investigating Microbial Communities and Their Biomarkers in Mars-Analog Lava Tubes at Craters of the Moon National Monument and Preserve

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    JGRPlanets_2022_Weng.pdf
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    Final Published Version
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    Author
    Weng, M.M.
    Zaikova, E.
    Millan, M.
    Williams, A.J.
    McAdam, A.C.
    Knudson, C.A.
    Fuqua, S.R.
    Wagner, N.Y.
    Craft, K.
    Kobs Nawotniak, S.
    Shields, A.
    Bevilacqua, J.
    Bai, Y.
    Hughes, S.S.
    Garry, W.B.
    Heldmann, J.L.
    Lim, D.S.S.
    Buckner, D.
    Gant, P.
    Johnson, S.S.
    Show allShow less
    Affiliation
    Department of Ecology and Evolutionary Biology, University of Arizona
    Issue Date
    2022
    Keywords
    analog
    genomics
    habitability
    lava tube
    life detection
    Mars
    
    Metadata
    Show full item record
    Publisher
    John Wiley and Sons Inc
    Citation
    Weng, M. M., Zaikova, E., Millan, M., Williams, A. J., McAdam, A. C., Knudson, C. A., Fuqua, S. R., Wagner, N. Y., Craft, K., Kobs Nawotniak, S., Shields, A., Bevilacqua, J., Bai, Y., Hughes, S. S., Garry, W. B., Heldmann, J. L., Lim, D. S. S., Buckner, D., Gant, P., & Johnson, S. S. (2022). Life Underground: Investigating Microbial Communities and Their Biomarkers in Mars-Analog Lava Tubes at Craters of the Moon National Monument and Preserve. Journal of Geophysical Research: Planets, 127(11).
    Journal
    Journal of Geophysical Research: Planets
    Rights
    Copyright © 2022. American Geophysical Union. All Rights Reserved.
    Collection Information
    This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.
    Abstract
    Craters of the Moon National Monument and Preserve (CotM) is a strong terrestrial analog for lava tube formations on Mars. The commonality of its basalt composition to Martian lava tubes makes it especially useful for probing how interactions between water, rock, and life have developed over time, and what traces of these microbial communities may be detectable by current flight-capable instrumentation. Our investigations found that secondary mineral deposits within these caves contain a range of underlying compositions that support diverse and active microbial communities. Examining the taxonomy, activity, and metabolic potential of these communities revealed largely heterotrophic life strategies supported by contributions from chemolithoautotrophs that facilitate key elemental cycles. Finally, traces of these microbial communities were detectable by flight-capable pyrolysis and wet chemistry gas chromatography-mass spectrometry methods comparable to those employed by the Sample Analysis at Mars (SAM) instrument aboard the Curiosity rover and the Mars Organic Molecule Analyzer (MOMA) on the upcoming Rosalind Franklin rover. Using a suite of methods for chemical derivatization of organic compounds is beneficial for resolving the greatest variety of biosignatures. Tetramethylammonium hydroxide (TMAH), for example, allowed for optimal resolution of long chain fatty acids. Taken together, these results have implications for the direction of mass spectrometry as a tool for biosignature detection on Mars, as well as informing the selection of sampling sites that could potentially host biosignatures. © 2022. American Geophysical Union. All Rights Reserved.
    Note
    6 month embargo; first published: 03 November 2022
    ISSN
    2169-9097
    DOI
    10.1029/2022JE007268
    Version
    Final published version
    ae974a485f413a2113503eed53cd6c53
    10.1029/2022JE007268
    Scopus Count
    Collections
    UA Faculty Publications

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