A Microbial Oasis in the Hypersaline Atacama Subsurface Discovered by a Life Detector Chip: Implications for the Search for Life on Mars

作者：Parro Victor^*; de Diego Castilla Graciela; Moreno Paz Mercedes; Blanco Yolanda; Cruz Gil Patricia; Rodriguez Manfredi Jose A; Fernandez Remolar David; Gomez Felipe; Gomez Manuel J; Rivas Luis A; Demergasso Cecilia; Echeverria Alex; Urtuvia Viviana N; Ruiz Bermejo Marta; Garcia Villadangos Miriam; Postigo Marina; Sanchez Roman Monica; Chong Diaz Guillermo; Gomez Elvira Javier

来源：Astrobiology, 2011, 11(10): 969-996.

DOI：10.1089/ast.2011.0654

• Atacama Desert
• Life detection
• Biosensor
• Biopolymers
• In situ measurement

The Atacama Desert has long been considered a good Mars analogue for testing instrumentation for planetary exploration, but very few data (if any) have been reported about the geomicrobiology of its salt-rich subsurface. We performed a Mars analogue drilling campaign next to the Salar Grande (Atacama, Chile) in July 2009, and several cores and powder samples from up to 5 m deep were analyzed in situ with LDChip300 (a Life Detector Chip containing 300 antibodies). Here, we show the discovery of a hypersaline subsurface microbial habitat associated with halite-, nitrate-, and perchlorate-containing salts at 2 m deep. LDChip300 detected bacteria, archaea, and other biological material (DNA, exopolysaccharides, some peptides) from the analysis of less than 0.5 g of ground core sample. The results were supported by oligonucleotide microarray hybridization in the field and finally confirmed by molecular phylogenetic analysis and direct visualization of microbial cells bound to halite crystals in the laboratory. Geochemical analyses revealed a habitat with abundant hygroscopic salts like halite (up to 260 g kg(-1)) and perchlorate (41.13 mu g g(-1) maximum), which allow deliquescence events at low relative humidity. Thin liquid water films would permit microbes to proliferate by using detected organic acids like acetate (19.14 mu g g(-1)) or formate (76.06 mu g g(-1)) as electron donors, and sulfate (15875 mu g g(-1)), nitrate (13490 mu g g(-1)), or perchlorate as acceptors. Our results correlate with the discovery of similar hygroscopic salts and possible deliquescence processes on Mars, and open new search strategies for subsurface martian biota. The performance demonstrated by our LDChip300 validates this technology for planetary exploration, particularly for the search for life on Mars.

• 出版日期2011-12