Community Characterization of Microbial Populations Found at a Cold Water Sulfidic Spring in the Canadian High Arctic

Abstract:

The unique environment on Europa makes it an ideal target for astrobiological investigation. One such earth-based analogue to aid in this investigation is the sulfur-dominated glacial spring system found at Borup Fiord Pass (BFP), Ellesmere Island, Nunavut, Canada. In this system, subsurface microbial sulfate reduction produces hydrogen sulfide, which is transported through the glacier along spring channels [1]. As the surface oxidation of H₂S occurs, resultant deposition of elemental sulfur (S⁰) and other minerals becomes visible (attached image). The energy released from these reactions can support potential microbial metabolisms and may be a valuable representation of microbial processes occurring on Europa. The resulting sulfur minerals provide sensitive records of dynamic atmospheric, geological, hydrological, chemical, and biological processes on planetary surfaces. Moreover, we expect that the S⁰-rich deposits of this glacial spring system will serve as a mineralogical record for biological activity and will provide a valuable tool for recognizing potential sulfur-based life on Europa.

During a recent collaborative expedition (2014) to BFP, samples were taken from the toe of the glacier in an area called the ‘Blister Crust’ (attached image). At this location, glacial channels reach the surface, representing an active interface between subsurface and surface processes. Initial geochemical characterization at the site revealed high amounts of aqueous sulfide (1.8 mM) and hydrogen (29 nM), which likely serve as the electron donation potential in the system. Furthermore, preliminary 16S rRNA gene sequencing has shown a high abundance of the genus Sulfurimonas, which is a known sulfur metabolizer. Our research seeks to further characterize microbial communities found at this interface in order to elucidate information regarding in situ sulfur cycling and the potential to tie this into subsurface/surface processes on Europa. Continued work will provide guidance into potential astrobiological targets on the surface of Europa, predominantly in regions where subsurface fluids interact with surface icings.

References: [1] Grasby S. E. et al. (2003) Astrobiology, 3(3), 583-596.