Searching for life on mars: Selection of molecular targets for ESA's aurora ExoMars mission

被引:132
作者
Parnell, John [1 ]
Cullen, David
Sims, Mark R.
Bowden, Stephen
Cockell, Charles S.
Court, Richard
Ehrenfreund, Pascale
Gaubert, Francois
Grant, William
Parro, Victor
Rohmer, Michel
Sephton, Mark
Stan-Lotter, Helga
Steele, Andrew
Toporski, Jan
Vago, Jorge
机构
[1] Univ Aberdeen, Dept Geol & Petr Geol, Aberdeen AB24 FX, Scotland
[2] Cranfield Univ, Silsoe, Beds, England
[3] Univ Leicester, Leicester LE1 7RH, Leics, England
[4] Open Univ, Milton Keynes MK7 6AA, Bucks, England
[5] Leiden Univ, NL-2300 RA Leiden, Netherlands
[6] European Space Agcy, NL-2200 AG Noordwijk, Netherlands
[7] Ctr Astrobiol, Madrid, Spain
[8] Univ Strasbourg, Strasbourg, France
[9] Imperial Coll London, London, England
[10] Salzburg Univ, A-5020 Salzburg, Austria
[11] Carnegie Inst Sci, Washington, DC 20005 USA
[12] Univ Kiel, Kiel, Germany
基金
英国科学技术设施理事会;
关键词
D O I
10.1089/ast.2006.0110
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The European Space Agency's ExoMars mission will seek evidence of organic compounds of biological and non-biological origin at the martian surface. One of the instruments in the Pasteur payload may be a Life Marker Chip that utilizes an immunoassay approach to detect specific organic molecules or classes of molecules. Therefore, it is necessary to define and prioritize specific molecular targets for antibody development. Target compounds have been selected to represent meteoritic input, fossil organic matter, extant ( living, recently dead) organic matter, and contamination. Once organic molecules are detected on Mars, further information is likely to derive from the detailed distribution of compounds rather than from single molecular identification. This will include concentration gradients beneath the surface and gradients from generic to specific compounds. The choice of biomarkers is informed by terrestrial biology but is wide ranging, and nonterrestrial biology may be evident from unexpected molecular distributions. One of the most important requirements is to sample where irradiation and oxidation are minimized, either by drilling or by using naturally excavated exposures. Analyzing regolith samples will allow for the search of both extant and fossil biomarkers, but sequential extraction would be required to optimize the analysis of each of these in turn.
引用
收藏
页码:578 / 604
页数:27
相关论文
共 170 条
[91]   Deep drill (DeeDri) for Mars application [J].
Magnani, PG ;
Re, E ;
Ylikorpi, T ;
Cherubini, G ;
Olivieri, A .
PLANETARY AND SPACE SCIENCE, 2004, 52 (1-3) :79-82
[92]  
MAHAFFY P, 2004, SCI PRIORITIES RELAT
[93]   Brines and evaporites: analogs for Martian life [J].
Mancinelli, RL ;
Fahlen, TF ;
Landheim, R ;
Klovstad, MR .
SPACE LIFE SCIENCES: SEARCH FOR SIGNATURES OF LIFE, AND SPACE FLIGHT ENVIRONMENTAL EFFECTS ON THE NERVOUS SYSTEM, 2004, 33 (08) :1244-1246
[94]   Martian soil and UV radiation: microbial viability assessment on spacecraft surfaces [J].
Mancinelli, RL ;
Klovstad, M .
PLANETARY AND SPACE SCIENCE, 2000, 48 (11) :1093-1097
[95]   Purification, analysis, and preservation of reduced nicotinamide adenine dinucleotide 2′-phosphate [J].
Markham, KA ;
Sikorski, RS ;
Kohen, A .
ANALYTICAL BIOCHEMISTRY, 2003, 322 (01) :26-32
[96]  
MEPAG M.E.P.A.G., 2006, MARS SCI GOALS OBJ I
[97]   Natural transfer of viable microbes in space - 1. From Mars to Earth and Earth to Mars [J].
Mileikowsky, C ;
Cucinotta, FA ;
Wilson, JW ;
Gladman, B ;
Horneck, G ;
Lindegren, L ;
Melosh, J ;
Rickman, H ;
Valtonen, M ;
Zheng, JQ .
ICARUS, 2000, 145 (02) :391-427
[98]   VIKING LANDING SITES, REMOTE-SENSING OBSERVATIONS, AND PHYSICAL-PROPERTIES OF MARTIAN SURFACE MATERIALS [J].
MOORE, HJ ;
JAKOSKY, BM .
ICARUS, 1989, 81 (01) :164-184
[99]   Focused proteomics: Monoclonal antibody-based isolation of the oxidative phosphorylation machinery and detection of phosphoproteins using a fluorescent phosphoprotein gel stain [J].
Murray, J ;
Marusich, MF ;
Capaldi, RA ;
Aggeler, R .
ELECTROPHORESIS, 2004, 25 (15) :2520-2525