Observations from a 4-Year Contamination Study of a Sample Depth Profile Through Martian Meteorite Nakhla

Details Observations from a 4-Year Contamination Study of a Sample Depth Profile Through Martian Meteorite Nakhla Observations from a 4-Year Contamination Study of a Sample Depth Profile Through Martian Meteorite Nakhla

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007asbio...7..389t&link_type=abstract

Astrobiology, Volume 7, Issue 2, pp. 389-401.

Biology

3

Martian Meteorites, Nakhla, Microbial Contamination, Life Detection

Scientific paper

Morphological, compositional, and biological evidence indicates the presence of numerous well-developed microbial hyphae structures distributed within four different sample splits of the Nakhla meteorite obtained from the British Museum (allocation BM1913,25). By examining depth profiles of the sample splits over time, morphological changes displayed by the structures were documented, as well as changes in their distribution on the samples, observations that indicate growth, decay, and reproduction of individual microorganisms. Biological staining with DNA-specific molecular dyes followed by epifluorescence microscopy showed that the hyphae structures contain DNA. Our observations demonstrate the potential of microbial interaction with extraterrestrial materials, emphasize the need for rapid investigation of Mars return samples as well as any other returned or impactor-delivered extraterrestrial materials, and suggest the identification of appropriate storage conditions that should be followed immediately after samples retrieved from the field are received by a handling/curation facility. The observations are further relevant in planetary protection considerations as they demonstrate that microorganisms may endure and reproduce in extraterrestrial materials over long (at least 4 years) time spans. The combination of microscopy images coupled with compositional and molecular staining techniques is proposed as a valid method for detection of life forms in martian materials as a first-order assessment. Time-resolved in situ observations further allow observation of possible (bio)dynamics within the system.

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