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GEOLOGY AND ASTROBIOLOGY FIELD RESEARCH IN MARS ANALOGUE EXTREME ENVIRONMENTS (ILEWG EUROMOONMARS)

机译:火星模拟极端环境(ILEWG EUROMOONMARS)的地质和天文生物学研究

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We give an update on the data analysis from a series of field research campaigns (ILEWG EuroMoon-Mars campaigns 2009 to 2013)in the extreme environment of the Utah desert relevant to habitability and astrobiology in Mars environments, and in order to help in the interpretation of Mars missions measurements from orbit (MEX, MRO) or from the surface (MER, MSL). We discuss results relevant to the preparation of future lander and sample return missions. We deployed at Mars Desert Research station, Utah, a suite of instruments and techniques including sample collection, context imaging from remote to local and microscale, drilling, spectrometers and life sensors. We analyzed how geological and geochem-ical evolution affected local parameters (mineralogy, organics content, environment variations) and the habitability and signature of organics and biota. We find high diversity in the composition of soil samples even when collected in close proximity, the low abundances of detectable PAHs and amino acids and the presence of biota of all three domains of life with significant heterogeneity. An extraordinary variety of putative cxtrcmophilcs was observed. A dominant factor seems to be soil porosity and lower clay-sized particle content. A protocol was developed for sterile sampling, contamination issues, and the diagnostics of biodiversity via PCR and DGGE analysis in soils and rocks samples. We compare 2009 campaign results to new measurements from 2010-2013 campaigns: comparison between remote sensing and in-situ measurements; the study of minerals: the detection of organics and signs of life. References [1-11] in Foing, Stoker Ehrcnfreund (Editors, 2011) l;Astrobiology field Research in Moon/Mars Analogue Environments", Special Issue of International Journal of Astrobiology , IJA 2011, 10, vol. 3. 137-305 ILEWG EuroMoonMars Team: B.H. Foing (1, 2, 6), C. Stoker (3), P. Ehrcnfreund (4, 5), I. Rammos (2), L. Rodrigucs (2), A. Svendscn (2), D. Olthctcn (2), K. Nebergall (6), M. Battler (6, 7), H. v't Houd (8), A. Bruneau (6,9), M. Cross (6,7), V. Maivald (10), C. Orgel (6), A. Elsacsser (4), S.O.L. Direito (2,4), W.F.M. Roling (2), G.R. Davies (2); (1) ESA/ ESTEC, Postbus 299, 2200 AG Noordwik, NL; (2) Vrijc Univcrsitcit, Amsterdam, Faculty of Earth Life Sciences, De Boelclaan 1085, 1081 HV Amsterdam, NL: (3) NASA Ames Research Centre: US: (4) Leiden Institute of Chemistry, NL; (5) Space Policy Institute, GWU, Washington D.C., USA; (6) ILEWG; (7) CPSX; (8) Cerberus Blackshorc, ESIC Noordwijk, NL; (9) ENSC Bordeaux; (10) DLR, Bremen.
机译:我们提供了在犹他州沙漠的极端环境中与火星环境中的可居住性和天体生物学相关的一系列现场研究活动(ILEWG EuroMoon-Mars运动2009至2013年)的数据分析的最新信息,以帮助解释从轨道(MEX,MRO)或从地面(MER,MSL)进行火星任务测量。我们讨论与准备未来的着陆器和样品返回任务有关的结果。我们在犹他州的火星沙漠研究站部署了一套仪器和技术,包括样品采集,从远程到本地和微观范围的环境成像,钻井,光谱仪和生命传感器。我们分析了地质和地球化学演化如何影响局部参数(矿物学,有机物含量,环境变化)以及有机物和生物群的可居住性和特征。我们发现土壤样品的成分具有很高的多样性,即使在非常接近的位置采集,可检测的PAHs和氨基酸含量低,以及生活中所有三个领域的生物群均具有显着的异质性。观察到非常多种推定的嗜xctrcmophilcs。一个主要因素似乎是土壤孔隙率和较低的粘土颗粒含量。制定了一项协议,用于通过土壤和岩石样品中的PCR和DGGE分析进行无菌采样,污染问题和生物多样性诊断。我们将2009年活动的结果与2010-2013年活动的新测量结果进行了比较:遥感与实地测量之间的比较;矿物质研究:检测有机物和生命迹象。参考文献[1-11],Foing,Stoker Ehrcnfreund(编辑,2011年);《月/火星模拟环境中的天体生物学领域研究》,《国际天体生物学杂志》特刊,IJA 2011,第10卷,第3卷。137-305 ILEWG EuroMoonMars团队:BH Foing(1、2、6),C。Stoker(3),P。Ehrcnfreund(4、5),I。Rammos(2),L。Rodrigucs(2),A。Svendscn(2), D.Olthctcn(2),K.Nebergall(6),M.Battler(6、7),H.v't Houd(8),A.Bruneau(6,9),M.Cross(6,7) ,V. Maivald(10),C.Orgel(6),A.Elsacsser(4),SOL Direito(2,4),WFM Roling(2),GR Davies(2);(1)ESA / ESTEC,Postbus 299,2200 AG Noordwik,NL;(2)Vrijc Univcrsitcit,阿姆斯特丹,地球生命科学学院,De Boelclaan 1085,1081 HV Amsterdam,NL:(3)NASA Ames研究中心:美国:(4)莱顿化学研究所, NL;(5)美国华盛顿特区GWU空间政策研究所;(6)ILEWG;(7)CPSX;(8)NL ESIC Noordwijk的Cerberus Blackshorc;(9)波尔多ENSC;(10)不来梅DLR。

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