The Rio Tinto Mars analogue site: An extremophilic Raman spectroscopic study

被引:48
作者
Edwards, Howell G. M. [1 ]
Vandenabeele, Peter [2 ]
Jorge-Villar, Susana E. [3 ]
Carter, Elizabeth A. [4 ]
Perez, Fernando Rull [5 ]
Hargreaves, Michael D. [1 ]
机构
[1] Univ Bradford, Sch Life Sci, Ctr Astrobiol & extremophile Res, Bradford BD7 1DP, W Yorkshire, England
[2] Univ Ghent, Dept Analyt Chem, B-9000 Ghent, Belgium
[3] Univ Burgos, Fac Humanidades & Educ, Area Geodinam Interna, Burgos 09001, Spain
[4] Univ Sydney, Sch Chem, Sydney, NSW 2006, Australia
[5] Univ Valladolid, Fac Ciencias, Ctr Astrobiol, E-47011 Valladolid, Spain
基金
英国工程与自然科学研究理事会;
关键词
Raman spectroscopy; Mars analogue; Rio Tinto; acidotrophic; astrobiology; spectral biomarkers;
D O I
10.1016/j.saa.2006.12.080
中图分类号
O433 [光谱学];
学科分类号
0703 ; 070302 ;
摘要
The Rio Tinto site is recognised as a terrestrial Mars analogue because of the presence of jarosite and related sulfates which have recently been identified by the NASA Mars Exploration Rover "Opportunity" in the El Capitan region of Meridiani Planum on Mars. It has long been known that acidophilic microbial action is responsible for the deep blood-red colour of the water in Rio Tinto, where the pH varies from about 1.5 to 3.0 and the water is rich in iron and sulfur. Following recent Raman spectroscopic characterisation of the mineral phases of the Rio Tinto system, we report here a study of the biological components found in several specimens of deposited minerals and near the waterside that were collected during a GeoRaman VI Conference organized field trip in 2006. Key biosignatures were found for carotenoids, scytonemin and mycosporine-like amino acids, which are indicative of the biological colonisation of exposed mineral substrates; information from this study will be useful for targeting Martian sites using a miniaturized Raman instrument where the biosignatures of relict or extant life could remain in the geological record. (c) 2006 Elsevier B.V. All rights reserved.
引用
收藏
页码:1133 / 1137
页数:5
相关论文
共 25 条
[1]  
AMILS R, 2006, COMMUNICATION
[2]  
CHEVRIER V, PLANET SPACE SCI
[3]   Mineralogy at Meridiani Planum from the Mini-TES experiment on the Opportunity Rover [J].
Christensen, PR ;
Wyatt, MB ;
Glotch, TD ;
Rogers, AD ;
Anwar, S ;
Arvidson, RE ;
Bandfield, JL ;
Blaney, DL ;
Budney, C ;
Calvin, WM ;
Faracaro, A ;
Fergason, RL ;
Gorelick, N ;
Graff, TG ;
Hamilton, VE ;
Hayes, AG ;
Johnson, JR ;
Knudson, AT ;
McSween, HY ;
Mehall, GL ;
Mehall, LK ;
Moersch, JE ;
Morris, RV ;
Smith, MD ;
Squyres, SW ;
Ruff, SW ;
Wolff, MJ .
SCIENCE, 2004, 306 (5702) :1733-1739
[4]   Surviving the limits to life at the surface of Mars [J].
Clark, BC .
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 1998, 103 (E12) :28545-28555
[5]   Ultraviolet radiation screening compounds [J].
Cockell, CS ;
Knowland, J .
BIOLOGICAL REVIEWS, 1999, 74 (03) :311-345
[6]   Antarctic paleolake sediments and the search for extinct life on Mars [J].
Doran, PT ;
Wharton, RA ;
Des Marais, DJ ;
McKay, CP .
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 1998, 103 (E12) :28481-28493
[7]  
Edwards H. G. M., 1999, SEARCH LIFE MARS, P83
[8]   Thermophiles, early biosphere evolution, and the origin of life on Earth: Implications for the exobiological exploration of Mars [J].
Farmer, J .
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 1998, 103 (E12) :28457-28461
[9]  
Frost R. L., 2005, SPECTROCHIM ACTA A, V62, P166
[10]  
GRYMES R, 2005, EGU GEOPH RES ABSTR, V7