The Effects of Freeze-Thaw and UVC Radiation on Microbial Survivability in a Selected Mars-like Environment
Daniel Keaney1, Brigid Lucey1, Noreen Quinn2
1Department of Biological Sciences, Munster Technological University, Bishopstown, T12 P928 Cork, Ireland.
Abstract:
The purpose of this study was to determine survivability of Escherichia coli, Deinococcus radiodurans and Paraburkholderia fungorum under Mars-simulated conditions for freeze-thawing (-80 °C to +30 °C) and UV exposure alone and in combination. E. coli ATCC 25922, D. radiodurans and P. fungorum remained viable following 20 successive freeze-thaw cycles, exhibiting viabilities of 2.3%, 96% and 72.6%, respectively. E. coli ATCC 9079 was non-recoverable by cycle 9. When exposed to UV irradiation, cells withstood doses of 870 J/m2 (E. coli ATCC 25922), 200 J/m2 (E. coli ATCC 9079), 50,760 J/m2 (D. radiodurans) and 44,415 J/m2 (P. fungorum). Data suggests P. fungorum is highly UV-resistant. Combined freeze-thawing with UV irradiation showed freezing increased UV resistance in E. coli ATCC 25922, E. coli DSM 9079 and D. radiodurans by 6-fold, 30-fold and 1.2-fold, respectively. Conversely, freezing caused P. fungorum to exhibit a 1.75-fold increase in UV susceptibility. Strain-dependent experimentation demonstrated that freezing increases UV resistance and prolongs survival. These findings suggest that exposure to short wavelength UV rays (254 nm) and temperature cycles resembling the daily fluctuating conditions on Mars do not significantly affect survival of D. radiodurans, P. fungorum and E. coli ATCC 25922 following 20 days of exposure.
Insights
Certain microbes like Deinococcus radiodurans and Paraburkholderia fungorum show high survival rates under Mars-simulated freeze-thaw and UV conditions. Escherichia coli survival varies by strain, with some showing increased UV resistance after freezing.
Area of Science:
- Astrobiology
- Microbial Ecology
- Planetary Science
Background:
- Understanding microbial survival is crucial for assessing the potential for life on Mars and for planetary protection protocols.
- Mars experiences extreme temperature fluctuations and significant UV radiation, posing challenges for extant or introduced life.
Purpose of the Study:
- To evaluate the survivability of key bacterial species (Escherichia coli, Deinococcus radiodurans, Paraburkholderia fungorum) under simulated Martian environmental conditions.
- To investigate the combined effects of freeze-thawing cycles and UV exposure on microbial viability.
Main Methods:
- Microbial strains were subjected to repeated freeze-thaw cycles (-80 °C to +30 °C) and UV irradiation (254 nm) independently and in combination.
- Viability assessments were performed after 20 freeze-thaw cycles and at various UV doses.
- Comparative analysis of survival rates across different strains and conditions was conducted.
Main Results:
- Deinococcus radiodurans (96% viability) and Paraburkholderia fungorum (72.6% viability) showed high survival after 20 freeze-thaw cycles.
- Escherichia coli ATCC 25922 withstood high UV doses (870 J/m²), while Paraburkholderia fungorum and Deinococcus radiodurans exhibited remarkable UV resistance.
- Freezing enhanced UV resistance in E. coli strains and D. radiodurans but increased UV susceptibility in P. fungorum.
Conclusions:
- Deinococcus radiodurans and Paraburkholderia fungorum demonstrate significant resilience to Martian freeze-thaw and UV conditions.
- Escherichia coli ATCC 25922 also shows potential for survival, with freezing paradoxically increasing its UV resistance.
- These findings have implications for the search for life on Mars and the design of future astrobiological missions.
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