Microbial colonization in impact-generated hydrothermal sulphate deposits, Haughton impact structure, and implications for sulphates on Mars

被引:73
作者
Parnell, J. [1 ]
Lee, P. [2 ,3 ]
Cockell, C. S. [4 ]
Osinski, G. R. [5 ]
机构
[1] Univ Aberdeen, Dept Geol, Aberdeen AB24 3UE, Scotland
[2] SETI Inst, Mars Inst, Moffett Field, CA 94035 USA
[3] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA
[4] British Antarctic Survey, Cambridge CB3 0ET, England
[5] Univ Arizona, Dept Planetary Sci, Tucson, AZ 85721 USA
基金
加拿大自然科学与工程研究理事会;
关键词
cyanobacteria; endoliths; gypsum; Haughton impact structure; impact craters; life on Mars; sulphates;
D O I
10.1017/S1473550404001995
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Hydrothermal gypsum deposits in the Haughton impact structure, Devon Island, Canada, contain microbial communities in an endolithic habitat within individual gypsum crystals. Cyanobacterial colonies occur as masses along cleavage planes, up to 5 cm from crystal margins. The crystals are transparent, so allow transmission of light for photosynthesis, while affording protection from dehydration and wind. The colonies appear to have modified their mineral host to provide additional space as they expanded. The colonies are black due to UV-screening pigments. The relative ease with which microbial colonization may be detected and identified in impact-generated sulphate deposits at Haughton suggests that analogous settings on other planets might merit future searches for biosignatures. The proven occurrence of sulphates on the Martian surface suggests that sulphate minerals should be a priority target in the search for life on Mars. Received 12 May 2004, accepted 7 July 2004
引用
收藏
页码:247 / 256
页数:10
相关论文
共 53 条
[1]  
Banin A., 1992, Mars, P594
[2]   Electrospray ionization nigh-resolution ion mobility spectrometry for the detection of organic compounds, 1. Amino acids [J].
Beegle, LW ;
Kanik, I ;
Matz, L ;
Hill, HH .
ANALYTICAL CHEMISTRY, 2001, 73 (13) :3028-3034
[3]   CRYPTOENDOLITHIC ALGAE OF HOT SEMIARID LANDS AND DESERTS [J].
BELL, RA .
JOURNAL OF PHYCOLOGY, 1993, 29 (02) :133-139
[4]   Evaporite mineral assemblages in the nakhlite (martian) meteorites [J].
Bridges, JC ;
Grady, MM .
EARTH AND PLANETARY SCIENCE LETTERS, 2000, 176 (3-4) :267-279
[5]   Alteration assemblages in martian meteorites: Implications for near-surface processes [J].
Bridges, JC ;
Catling, DC ;
Saxton, JM ;
Swindle, TD ;
Lyon, IC ;
Grady, MM .
SPACE SCIENCE REVIEWS, 2001, 96 (1-4) :365-392
[6]   Electrically conducting, Ca-rich brines, rather than water, expected in the Martian subsurface [J].
Burt, DM ;
Knauth, LP .
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 2003, 108 (E4)
[7]   Hydrogeologic evolution of Gale crater and its relevance to the exobiological exploration of Mars [J].
Cabrol, NA ;
Grin, EA ;
Newsom, HE ;
Landheim, R ;
McKay, CP .
ICARUS, 1999, 139 (02) :235-245
[8]   Sulfuric acid production on Europa: The Radiolysis of sulfur in water ice [J].
Carlson, RW ;
Anderson, MS ;
Johnson, RE ;
Schulman, MB ;
Yavrouian, AH .
ICARUS, 2002, 157 (02) :456-463
[9]  
Cid A, 2001, ESA SP PUBL, V496, P201
[10]   The impact crater as a habitat: Effects of impact processing of target materials [J].
Cockell, CS ;
Osinski, GR ;
Lee, P .
ASTROBIOLOGY, 2003, 3 (01) :181-191