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Microbial active motion and other traits serve as biosignatures, detectable via in situ microscopy in extreme environments. Stimulating cells and optimizing data processing are key for future space missions.

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Area of Science:

  • Astrobiology
  • Microbiology
  • Geochemistry

Background:

  • Microbial life detection in extreme environments is crucial for astrobiology.
  • In situ characterization of microbial biosignatures is challenging.
  • Previous imaging efforts have not explored diverse extreme field sites.

Purpose of the Study:

  • Investigate microbial active motion, morphology, and optical properties as biosignatures.
  • Assess the utility of in situ video microscopy for life detection in extreme environments.
  • Evaluate methods for stimulating microbial activity and processing data for space missions.

Main Methods:

  • In situ video microscopy was employed across diverse extreme field sites.
  • Samples included seawater, sea ice brines, cryopeg brines, hypersaline pools, hyperalkaline springs, and cave ice.
  • An autonomous, open-source software package was used for data classification.

Main Results:

  • Active microbial motion was observed in most samples without treatment, and in cryopeg brines with a temperature gradient.
  • Motility increased significantly with stimuli like warming and L-serine addition; chemotaxis and thermotaxis were observed.
  • Non-motile cells were distinguishable from minerals by passive motion, optical properties, and morphology.

Conclusions:

  • Volumetric light microscopy is a valuable tool for in situ life detection.
  • Stimulating cells in situ and developing space-mission-compatible data processing are important.
  • Future missions require instruments for capturing cell-like objects for chemical analysis.