On-site mineralogical and microbiological analyses of rock samples were performed by human operators during simulated surface extra-vehicular activity (EVA) at lunar and Mars analogue field sites. Operations were facilitated during AMASE by JPL’s Cliffbot Rover, which obtained rock samples from inaccessible sites e.g. 80-90 degree slopes. These tests provide an example of what humans could do on the Moon to address challenges facing future crews on Mars e.g. planetary protection, life detection and performing science on the surface as ‘scientists’, with greater flexibility and less direct guidance from mission control. Mineralogical analysis of rocks was performed (within seconds) with a hand-held Raman spectrometer to verify geological field observations; microbiological analysis (within minutes) with the Lab-On-a-Chip Application Development Portable Test System (LOCAD-PTS), a handheld device for biochemical analysis – now aboard the International Space Station (ISS). Figure 1. A. Lunar analogue site (Cinder Lakes, Arizona). B. Mars analogue site (Bockfjorden, Arctic). Introduction: The Vision for Space Exploration, announced by the President of the United States in January 2004, stated that NASA would work towards a “human return to the Moon before 2020, in preparation for human exploration of Mars” [1]. Mendell has summarized various ideas concerning exactly what humans should do on the Moon [2]. The remoteness of Mars from Earth – in terms of distance and communications delays – necessitates greater crew autonomy, in science as much as mission operations. Science instruments that are small, easy to use and provide rapid results (in space) encourage iterative scientific thought processes in the field. We have used this approach to perform microbiological and mineralogical research at remote field sites on Earth [3-6] and suggest that it could be extended to human exploration of the Moon and Mars. While the potential for life on the Moon is negligible [7], it’s absence (apart from those organisms introduced by spacecraft) makes it an ideal place to understand how humans and their microbe-laden spacecraft [9,10] bio-contaminate a planetary surface [8]. Studies on the Moon will help us limit biocontamination of the Martian surface which threatens to interfere with life detection experiments and endanger planetary protection [11-14]. Methods: Analogue Field Sites. Lunar analogue site: cinder field ‘Cinder Lakes’ (elevation 2031 meters), near San Francisco Peaks, Flagstaff, Arizona. Site has little/no vegetation, artificially cratered in the 1960s to re-create lunar landing site terrain to train the Apollo 15-17 crews now used as test site for NASA Desert Research and Technology Study (D-RATS). Mars analogue site located at Bockfjorden, Spitsbergen (79.5°N, 13.5°E), visited during 2006 Arctic Mars Analogue Svalbard Expedition (AMASE), August 2006. Spacesuits. Simulated surface EVA performed with Zero Prebreathe System Mark III spacesuit, a prototype for future lunar exploration. Swab Microbial Analysis. Swab analysis performed by brushing sterile swab over surface for 10 seconds, swab tip then immersed in 1ml LAL reagent water (LRW, Charles River Labs, Wilmington, MA), mixed 30 seconds, followed by LOCAD-PTS analysis. Mineralogical analysis. Raman spectrometry performed by suited subject during EVA with Raman Systems RSL Plus using a 785 nm wavelength laser. Size of Raman spectrometer: 10” x 5” x 3”, with small screen (4” x 2.5”) to display spectra. Rover Interaction. JPL Cliffbot deployed to obtain samples from site inaccessible to the human operator: steep cliff with 80-90 degree slope. Rover and EVA operations coordinated to enable hand-off of rock samples to human operator. Results: At Mars analogue site, suited subject identified rock of interest, approximately 10” in diameter, reddish color with a white vein (figure 2). Geologists field observations suggested this vein consisted of feldspar (a dark layer of unknown composition was located within the vein). Raman analysis actually showed the vein to be carbonate and dark layer to be macromolecular carbon.
[1]
W W Mendell,et al.
Meditations on the new space vision: the Moon as a stepping stone to Mars.
,
2005,
Acta astronautica.
[2]
V K Ilyin,et al.
Microbiological status of cosmonauts during orbital spaceflights on Salyut and Mir orbital stations.
,
2005,
Acta astronautica.
[3]
D. Pierson,et al.
Microbial contamination of spacecraft.
,
2001,
Gravitational and space biology bulletin : publication of the American Society for Gravitational and Space Biology.
[4]
John D. Rummel,et al.
Biological contamination studies of lunar landing sites: implications for future planetary protection and life detection on the Moon and Mars
,
2004,
International Journal of Astrobiology.
[5]
Joseph N. Tatarewicz,et al.
The “Vision for Space Exploration” of President George W. Bush, space science, and U.S. space policy
,
2009
.