Real-Time Monitoring for Aseptic Drilling: Lessons Learned from the Atacama Rover Astrobiology Drilling Studies Contamination Control Strategy and Implementation and Application to the Icebreaker Mars Life Detection Mission.

Journal: Astrobiology
PMID:

Abstract

In 2019, the Atacama Rover Astrobiology Drilling Studies (ARADS) project field-tested an autonomous rover-mounted robotic drill prototype for a 6-Sol life detection mission to Mars (Icebreaker). ARADS drilled Mars-like materials in the Atacama Desert (Chile), one of the most life-diminished regions on Earth, where mitigating contamination transfer into life-detection instruments becomes critical. Our Contamination Control Strategy and Implementation (CCSI) for the Sample Handling and Transfer System (SHTS) hardware (drill, scoop and funnels) included out-of-simulation protocol testing (out-of-sim) for hardware decontamination and verification during the 6-Sol simulation (in-sim). The most effective five-step decontamination combined safer-to-use sterilants (3%_hydrogen-peroxide-activated 5%_sodium-hypochlorite), and real-time verification by adenosine triphosphate (ATP) and Signs of Life Detector (SOLID) Fluorescence Immunoassay for characterization hardware bioburden and airborne contaminants. The 20- to 40-min protocol enabled a 4-log bioburden reduction down to <0.1 fmoles ATP detection limit (funnels and drill) to 0.2-0.7 fmoles (scoop) of total ATP. The (post-cleaning) hardware background was 0.3 to 1-2 attomoles ATP/cm (cleanliness benchmark background values) equivalent to ca. 1-10 colony forming unit (CFU)/cm. Further, 60-100% of the in-sim hardware background was ≤3-4 bacterial cells/cm, the threshold limit for Class <7 aseptic operations. Across the six Sols, the flux of airborne contaminants to the drill sites was ∼5 and ∼22 amoles ATP/(cm·day), accounting for an unexpectedly high Fluorescence Intensity (FI) signal (FI: ∼6000) against aquatic cyanobacteria, but negligible anthropogenic contribution. The SOLID immunoassay also detected microorganisms from multiple habitats across the Atacama Desert (anoxic, alkaline/acidic microenvironments in halite fields, playas, and alluvial fans) in both airborne and post-cleaning hardware background. Finally, the hardware ATP background was 40-250 times lower than the ATP in cores. Similarly, the FI peaks (FI) against the microbial taxa and molecular biomarkers detected in the post-cleaned hardware (FI: ∼1500-1600) were 5-10 times lower than biomarkers in drilled sediments, excluding significant interference with putative biomarker found in cores. Similar protocols enable the acquisition of contamination-free materials for ultra-sensitive instruments analysis and the integrity of scientific results. Their application can augment our scientific knowledge of the distribution of cryptic life on Mars-like grounds and support life-detection robotic and human-operated missions to Mars.

Authors

  • Rosalba Bonaccorsi
    SETI Institute, Mountain View, California, USA.
  • Brian Glass
    NASA Ames Research Center, Moffett Field, California, USA.
  • Mercedes Moreno-Paz
    Centro de Astrobiología (CAB), CSIC-INTA, Madrid, Spain.
  • Miriam García-Villadangos
    Department of Molecular Evolution, Centro de Astrobiología (INTA-CSIC), Madrid, Spain.
  • Kimberley Warren-Rhodes
    SETI Institute, Mountain View, California, USA.
  • Víctor Parro
    Centro de Astrobiología (CAB), CSIC-INTA, Madrid, Spain.
  • Juan Manuel Manchado
    Department of Molecular Evolution, Centro de Astrobiología (INTA-CSIC), Madrid, Spain.
  • Mary Beth Wilhelm
    NASA Ames Research Center, Moffett Field, California, USA.
  • Christopher P McKay
    NASA Ames Research Center, Moffett Field, California, USA.