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Life Detection on Icy Moons Using Flow Cytometry and Exogenous Fluorescent Stains
Matthew L Wallace1, Nicholas Tallarida1, Wayne W Schubert1
1Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA.
Flow cytometry can detect life on icy moons and Mars using fluorescent stains to identify biomarkers like nucleic acids and proteins. This method successfully distinguishes between living organisms and non-living material in simulated space samples.
Area of Science:
- Astrobiology
- Planetary Science
- Analytical Chemistry
Background:
- Flow cytometry is a promising technology for *in situ* life detection on extraterrestrial bodies like icy moons and Mars.
- Identifying key biomarkers is crucial for distinguishing life from abiotic materials in extreme environments.
Purpose of the Study:
- To develop and validate a flow cytometry method for identifying four classes of biomarkers (nucleic acids, proteins, carbohydrates, lipids) using exogenous fluorescent stains.
- To assess the effectiveness of this method in distinguishing between biotic and abiotic materials in simulated extraterrestrial samples.
Main Methods:
- Utilized flow cytometry with exogenous fluorescent stains targeting nucleic acids, proteins, carbohydrates, and lipids.
- Tested the method with six known organisms and abiotic materials.
- Analyzed six natural samples with unknown biotic/abiotic content to simulate a lander experiment.
Main Results:
- Successfully identified the four target biomarker classes using exogenous stains.
- Demonstrated the ability to clearly distinguish between known organisms and abiotic materials.
- Showcased the separation of biotic from abiotic material in natural samples using scatter plots.
Conclusions:
- Exogenous staining with flow cytometry is effective for *in situ* biomarker detection and life identification on icy moons and Mars.
- This technique, combined with intrinsic fluorescence and data analysis, enhances life detection capabilities for space missions.
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