Arid
DOI10.1089/ast.2011.0654
A Microbial Oasis in the Hypersaline Atacama Subsurface Discovered by a Life Detector Chip: Implications for the Search for Life on Mars
Parro, Victor1; de Diego-Castilla, Graciela1; Moreno-Paz, Mercedes1; Blanco, Yolanda1; Cruz-Gil, Patricia1; Rodriguez-Manfredi, Jose A.2; Fernandez-Remolar, David3; Gomez, Felipe3; Gomez, Manuel J.1; Rivas, Luis A.1; Demergasso, Cecilia4,5; Echeverria, Alex4; Urtuvia, Viviana N.4; Ruiz-Bermejo, Marta1; Garcia-Villadangos, Miriam1; Postigo, Marina1; Sanchez-Roman, Monica3; Chong-Diaz, Guillermo5,6; Gomez-Elvira, Javier2
通讯作者Parro, Victor
来源期刊ASTROBIOLOGY
ISSN1531-1074
出版年2011
卷号11期号:10页码:969-996
英文摘要

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.


英文关键词Atacama Desert Life detection Biosensor Biopolymers In situ measurement
类型Article
语种英语
国家Spain ; Chile
收录类别SCI-E
WOS记录号WOS:000298345600004
WOS关键词RHODOSPIRILLUM-CENTENUM ; NORTHERN CHILE ; DESERT ; INSTRUMENT ; MICROARRAY ; SOIL ; RNA ; ENVIRONMENTS ; ASTROBIOLOGY ; ACIDOPHILE
WOS类目Astronomy & Astrophysics ; Biology ; Geosciences, Multidisciplinary
WOS研究方向Astronomy & Astrophysics ; Life Sciences & Biomedicine - Other Topics ; Geology
资源类型期刊论文
条目标识符http://119.78.100.177/qdio/handle/2XILL650/167194
作者单位1.Ctr Astrobiol INTA CSIC, Dept Mol Evolut, Madrid 28850, Spain;
2.Ctr Astrobiol INTA CSIC, Dept Instrumentat, Madrid 28850, Spain;
3.Ctr Astrobiol INTA CSIC, Dept Planetol & Habitabil, Madrid 28850, Spain;
4.Univ Catolica Norte, Ctr Biotecnol, Antofagasta, Chile;
5.Univ Catolica Norte, Ctr Invest Cient & Tecnol Mineria, Antofagasta, Chile;
6.Univ Catolica Norte, Dept Geol Sci, Antofagasta, Chile
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Parro, Victor,de Diego-Castilla, Graciela,Moreno-Paz, Mercedes,et al. A Microbial Oasis in the Hypersaline Atacama Subsurface Discovered by a Life Detector Chip: Implications for the Search for Life on Mars[J],2011,11(10):969-996.
APA Parro, Victor.,de Diego-Castilla, Graciela.,Moreno-Paz, Mercedes.,Blanco, Yolanda.,Cruz-Gil, Patricia.,...&Gomez-Elvira, Javier.(2011).A Microbial Oasis in the Hypersaline Atacama Subsurface Discovered by a Life Detector Chip: Implications for the Search for Life on Mars.ASTROBIOLOGY,11(10),969-996.
MLA Parro, Victor,et al."A Microbial Oasis in the Hypersaline Atacama Subsurface Discovered by a Life Detector Chip: Implications for the Search for Life on Mars".ASTROBIOLOGY 11.10(2011):969-996.
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