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An astrophysical view of Earth-based metabolic biosignature gases
Sara Seager1, Matthew Schrenk, William Bains
1Department of Earth, Atmospheric, and Planetary Sciences, MIT, Cambridge, Massachusetts, USA. seager@mit.edu
Abstract:
Microbial life on Earth uses a wide range of chemical and energetic resources from diverse habitats. An outcome of this microbial diversity is an extensive and varied list of metabolic byproducts. We review key points of Earth-based microbial metabolism that are useful to the astrophysical search for biosignature gases on exoplanets, including a list of primary and secondary metabolism gas byproducts. Beyond the canonical, unique-to-life biosignature gases on Earth (O(2), O(3), and N(2)O), the list of metabolic byproducts includes gases that might be associated with biosignature gases in appropriate exoplanetary environments. This review aims to serve as a starting point for future astrophysical biosignature gas research.
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