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Cleanroom Microbes Survive Drying, Vacuum, and Proton IrradiationIntroduction: The goal of planetary protection at NASA is to mitigate the risk of contaminating sensitive target bodies with biological life. While many cleaning procedures have been put in place to reduce bioburden on spacecraft, microbes are experts at evolving to survive harsh conditions. Specifically, the dry, low-nutrient environment of a cleanroom (commonly used for assembly of spacecraft) can represent an environment where extremophiles can survive.

Methods: Scientists at NASA MSFC wished to gather a snapshot of the microbial population within a variety of cleanrooms on site. A study was undertaken to collect air, surface, and floor samples from clean-rooms and isolate unique morphologies. From this study, 95 isolates were collected and saved in a microbial library. About 86% of these were identified at least to a genus level.

Following identification, 24 microbes were selected, based on a literature review, as potential extremophiles. These were grown in liquid cultures, diluted to a set optical density, washed with water, and then applied to a sterilized Kapton coupon. Droplets were allowed to dry overnight in a biosafety cabinet. Coupons were then installed in a pelletron and pumped down to high vacuum (~1E-6 Torr). Samples were then subjected 100 keV protons at a fluence of 2x1015 p+/cm2 up to 4x1015 p+/cm2. Following exposure, samples were returned to the microbiology lab where they were pro-cessed by submerging in water, vortexing, and then plating either droplets or spread plates. Recovery data collected was qualitative with a ranking or +, minor, or – for growth. Some selected radiotolerant strains were sequenced using the Illumina sequencing platform. The resulting genomes were annotated with the Rapid Annotations using Subsystems Technology (RAST) server and analyzed for conserved and unique stress response relevant genomic signatures to identify clues related to specific tolerances.

Results and Discussion: After five rounds of proton radiation, we narrowed our isolates to five, non-spore forming bacteria that demonstrated survival: Arthrobacter koreensis, Paenarthrobacter nitroguajacolicus, Mycetocola manganoxydans, and an Erwinia sp. Furthermore, we exposed these four microbes to 254 nm wavelength light at an intensity of 80 W/m2 at a distance of ~18 cm for 10 minutes. Only A. koreensis demonstrated survival following UV exposure.

Finally, we performed whole genome sequencing on the four strains to look for genetic markers of stress resistance. When we compared the genomes of the four strains, we found that genes coding for GGDEF and EAL domains with PAS/PAC sensors were only found in A. koreensis. These domains, modulated by PAS/PAC sensors, are hypothesized to facilitate survival under drying, desiccation, and proton irradiation.

Drying and Desiccation: PAS domains sense hydration changes and modulate GGDEF and EAL domain activity to adjust c-di-GMP levels, enhancing resistance to desiccation. For instance, in Pseudomonas aeruginosa, the PAS domain of RbdA modulates activity under varying hydration conditions, affecting stress responses [1].

Proton Irradiation: Proton irradiation causes oxidative stress, leading to ROS generation. PAS domains detect this stress and modulate GGDEF and EAL domains to manage oxidative stress responses. In Shewanella, EAL domain proteins modulated by PAS sensors help bacteria adapt to extreme conditions [2]. These genes upregulate other stress response genes, protecting membrane function, protein stability, DNA repair, and antioxidant defenses. The modulation of c-di-GMP by PAS domains is crucial for bacterial
adaptation to stress conditions, enabling dynamic physio-logical adjustments [3]. Understanding these mechanisms provides insights into bacterial stress responses and strategies for controlling bacterial growth [4].

Conclusions: These findings indicate that clean-rooms harbor extremophile microbes that may be able to survive conditions in deep space. Furthermore, while we identified certain stress-response genes that may be at least partly responsible for the phenotypes observed in this study, there are likely unidentified genes or characteristics about A. koreensis, and other bacteria, that may allow them to survive in harsh environments. Future studies will focus on identifying these unknown genes and characteristics, further elucidating the mechanisms of extremophile survival and potentially informing the development of new biotechnologies for space exploration and other extreme environments.
Document ID
20240012269
Acquisition Source
Marshall Space Flight Center
Document Type
Presentation
Authors
Chelsi Cassilly
(Marshall Space Flight Center Redstone Arsenal, United States)
Atul Chander
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
Curtis Bahr
(Jacobs (United States) Dallas, Texas, United States)
Jason Vaughn
(Marshall Space Flight Center Redstone Arsenal, United States)
Peter Bertone
(Marshall Space Flight Center Redstone Arsenal, United States)
Stefan Green
(Rush University Medical Center Chicago, Illinois, United States)
Kevin Kunstman
(Rush University Medical Center Chicago, Illinois, United States)
Kasthuri Venkateswaran
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
Samantha Marcella
(Jacobs (United States) Dallas, Texas, United States)
Heather Morris
(Jacobs (United States) Dallas, Texas, United States)
Date Acquired
September 24, 2024
Meeting Information
Meeting: Astrobiology and the Future of Life Meeting
Location: Houston, TX
Country: US
Start Date: October 16, 2024
End Date: October 18, 2024
Sponsors: Lunar and Planetary Institute
Funding Number(s)
WBS: 829688.13.05.02.10.04
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
NASA Peer Committee
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