TY - GEN A1 - de Vera, Jean-Pierre Paul A1 - Alawi, Mashal A1 - Backhaus, Theresa A1 - Baque, Mickael A1 - Billi, Daniela A1 - Boettger, Ute A1 - Berger, Thomas A1 - Bohmeier, Maria A1 - Cockell, Charles A1 - Demets, Rene A1 - de la Torre Noetzel, Rosa A1 - Edwards, Howell A1 - Elsaesser, Andreas A1 - Fagliarone, Claudia A1 - Fiedler, Annelie A1 - Foing, Bernard A1 - Foucher, Frederic A1 - Fritz, Jörg A1 - Hanke, Franziska A1 - Herzog, Thomas A1 - Horneck, Gerda A1 - Hübers, Heinz-Wilhelm A1 - Huwe, Björn A1 - Joshi, Jasmin Radha A1 - Kozyrovska, Natalia A1 - Kruchten, Martha A1 - Lasch, Peter A1 - Lee, Natuschka A1 - Leuko, Stefan A1 - Leya, Thomas A1 - Lorek, Andreas A1 - Martinez-Frias, Jesus A1 - Meessen, Joachim A1 - Moritz, Sophie A1 - Moeller, Ralf A1 - Olsson-Francis, Karen A1 - Onofri, Silvano A1 - Ott, Sieglinde A1 - Pacelli, Claudia A1 - Podolich, Olga A1 - Rabbow, Elke A1 - Reitz, Günther A1 - Rettberg, Petra A1 - Reva, Oleg A1 - Rothschild, Lynn A1 - Garcia Sancho, Leo A1 - Schulze-Makuch, Dirk A1 - Selbmann, Laura A1 - Serrano, Paloma A1 - Szewzyk, Ulrich A1 - Verseux, Cyprien A1 - Wadsworth, Jennifer A1 - Wagner, Dirk A1 - Westall, Frances A1 - Wolter, David A1 - Zucconi, Laura T1 - Limits of life and the habitability of Mars BT - the ESA space experiment BIOMEX on the ISS T2 - Astrobiology N2 - BIOMEX (BIOlogy and Mars EXperiment) is an ESA/Roscosmos space exposure experiment housed within the exposure facility EXPOSE-R2 outside the Zvezda module on the International Space Station (ISS). The design of the multiuser facility supports-among others-the BIOMEX investigations into the stability and level of degradation of space-exposed biosignatures such as pigments, secondary metabolites, and cell surfaces in contact with a terrestrial and Mars analog mineral environment. In parallel, analysis on the viability of the investigated organisms has provided relevant data for evaluation of the habitability of Mars, for the limits of life, and for the likelihood of an interplanetary transfer of life (theory of lithopanspermia). In this project, lichens, archaea, bacteria, cyanobacteria, snow/permafrost algae, meristematic black fungi, and bryophytes from alpine and polar habitats were embedded, grown, and cultured on a mixture of martian and lunar regolith analogs or other terrestrial minerals. The organisms and regolith analogs and terrestrial mineral mixtures were then exposed to space and to simulated Mars-like conditions by way of the EXPOSE-R2 facility. In this special issue, we present the first set of data obtained in reference to our investigation into the habitability of Mars and limits of life. This project was initiated and implemented by the BIOMEX group, an international and interdisciplinary consortium of 30 institutes in 12 countries on 3 continents. Preflight tests for sample selection, results from ground-based simulation experiments, and the space experiments themselves are presented and include a complete overview of the scientific processes required for this space experiment and postflight analysis. The presented BIOMEX concept could be scaled up to future exposure experiments on the Moon and will serve as a pretest in low Earth orbit. KW - EXPOSE-R2 KW - BIOMEX KW - Habitability KW - Limits of life KW - Extremophiles KW - Mars Y1 - 2019 U6 - https://doi.org/10.1089/ast.2018.1897 SN - 1531-1074 SN - 1557-8070 VL - 19 IS - 2 SP - 145 EP - 157 PB - Liebert CY - New Rochelle ER - TY - THES A1 - Serrano, Paloma T1 - Methanogens from Siberian permafrost as models for life on Mars : response to simulated martian conditions and biosignature characterization T1 - Methanogene Archaeen aus sibirischen Permafrost als Modelle für Leben auf dem Mars N2 - Mars is one of the best candidates among planetary bodies for supporting life. The presence of water in the form of ice and atmospheric vapour together with the availability of biogenic elements and energy are indicators of the possibility of hosting life as we know it. The occurrence of permanently frozen ground – permafrost, is a common phenomenon on Mars and it shows multiple morphological analogies with terrestrial permafrost. Despite the extreme inhospitable conditions, highly diverse microbial communities inhabit terrestrial permafrost in large numbers. Among these are methanogenic archaea, which are anaerobic chemotrophic microorganisms that meet many of the metabolic and physiological requirements for survival on the martian subsurface. Moreover, methanogens from Siberian permafrost are extremely resistant against different types of physiological stresses as well as simulated martian thermo-physical and subsurface conditions, making them promising model organisms for potential life on Mars. The main aims of this investigation are to assess the survival of methanogenic archaea under Mars conditions, focusing on methanogens from Siberian permafrost, and to characterize their biosignatures by means of Raman spectroscopy, a powerful technology for microbial identification that will be used in the ExoMars mission. For this purpose, methanogens from Siberian permafrost and non-permafrost habitats were subjected to simulated martian desiccation by exposure to an ultra-low subfreezing temperature (-80ºC) and to Mars regolith (S-MRS and P-MRS) and atmospheric analogues. They were also exposed to different concentrations of perchlorate, a strong oxidant found in martian soils. Moreover, the biosignatures of methanogens were characterized at the single-cell level using confocal Raman microspectroscopy (CRM). The results showed survival and methane production in all methanogenic strains under simulated martian desiccation. After exposure to subfreezing temperatures, Siberian permafrost strains had a faster metabolic recovery, whereas the membranes of non-permafrost methanogens remained intact to a greater extent. The strain Methanosarcina soligelidi SMA-21 from Siberian permafrost showed significantly higher methane production rates than all other strains after the exposure to martian soil and atmospheric analogues, and all strains survived the presence of perchlorate at the concentration on Mars. Furthermore, CRM analyses revealed remarkable differences in the overall chemical composition of permafrost and non-permafrost strains of methanogens, regardless of their phylogenetic relationship. The convergence of the chemical composition in non-sister permafrost strains may be the consequence of adaptations to the environment, and could explain their greater resistance compared to the non-permafrost strains. As part of this study, Raman spectroscopy was evaluated as an analytical technique for remote detection of methanogens embedded in a mineral matrix. This thesis contributes to the understanding of the survival limits of methanogenic archaea under simulated martian conditions to further assess the hypothetical existence of life similar to methanogens on the martian subsurface. In addition, the overall chemical composition of methanogens was characterized for the first time by means of confocal Raman microspectroscopy, with potential implications for astrobiological research. N2 - Der Mars ist unter allen Planeten derjenige, der aufgrund verschiedener Faktoren am wahrscheinlichsten Leben ermöglichen kann. Das Vorhandensein von Wasser in Form von Eis und atmosphärischem Dampf zusammen mit der Verfügbarkeit biogener Elemente sowie Energie sind Indikatoren für die Möglichkeit, Leben, wie wir es kennen, zu beherbergen. Das Auftreten von dauerhaft gefrorenen Böden, oder auch Permafrost, ist ein verbreitetes Phänomen auf dem Mars. Dabei zeigen sich vielfältige morphologische Analogien zum terrestrischen Permafrost. Permafrostgebiete auf der Erde, welche trotz extremer, Bedingungen durch eine große Zahl und Vielfalt mikrobieller Gemeinschaften besiedelt sind, sind hinsichtlich möglicher Habitate auf dem Mars die vielversprechendste Analogie. Die meisten methanogenen Archaeen sind anaerobe, chemolithotrophe Mikroorganismen, die auf der Marsoberfläche viele der metabolischen und physiologischen Erfordernisse zum Überleben vorfinden. Methanogene Archaeen aus dem sibirischen Permafrost sind zudem extrem resistent gegenüber unterschiedlichen Formen von physiologischem Stress sowie simulierten thermo-physikalischen Marsbedingungen. Die Hauptziele dieser Untersuchung bestehen darin, das Überleben der methanogenen Archaeen unter Marsbedingungen zu beurteilen, wobei der Fokus auf methanogenen Archaeen aus dem sibirischen Permafrost liegt, sowie deren Biosignaturen mit Hilfe der Raman-Spektroskopie zu charakterisieren, einer starken Technologie zur mikrobiellen Identifikation, welche bei der ExoMars-Mission zum Einsatz kommen wird. Zu diesem Zweck wurden methanogene Archaeen aus dem sibirischen Permafrost sowie aus Nicht-Permafrost-Habitaten in Simulationen Marsbedingungen ausgesetzt, wie Austrocknung durch Langzeitversuche bei ultraniedrigen Temperaturen unter dem Gefrierpunkt (-80ºC), Mars-analogen Mineralien (S-MRS und P-MRS) sowie einer Marsatmosphäre. Weiterhin wurden die Kulturen verschiedenen Konzentrationen von Magnesiumperchlorat, einem starken Oxidant, der im Marsboden nachgewiesenen wurde, ausgesetzt. Ferner wurden die Biosignaturen einzelner Zellen der methanogenen Archaeen mit Hilfe der konfokalen Raman-Mikrospektroskopie (CRM) charakterisiert. Die Ergebnisse zeigten für alle untersuchten methanogenen Stämme Überleben und Methanbildung, nachdem diese simulierten Austrocknungsbedingungen ausgesetzt worden waren. Nach Versuchen mit Temperaturen unter dem Gefrierpunkt zeigten die Stämme aus dem sibirischen Permafrost eine schnellere Wiederaufnahme der Stoffwechseltätigkeit, wohingegen bei den Referenzorganismen aus Nicht-Permafrost-Habitaten die Zell¬membranen im größeren Ausmaß intakt blieben. Der Stamm Methanosarcina soligelidi SMA-21 aus dem sibirischen Permafrost zeigte nach dem Belastungstest mit Marsboden und Mars-analoger Atmosphäre signifikant höhere Methanbildungsraten. Zudem überlebten alle untersuchten Stämme die Zugabe von Magnesiumperchlorat in der entsprechenden Konzentration, die auf dem Mars vorkommt. Weiterhin konnten durch die Raman-Spektroskopie beachtliche Unterschiede in der chemischen Zusammensetzung zwischen methanogenen Archaeen aus Permafrost- und Nicht-Permafrost-Habitaten, trotz ihrer phylogenetischen Verwandtschaft, ermittelt werden. Die Konvergenz der chemischen Zusammensetzung der Permafrost-Stämme könnte das Resultat ihrer Anpassung an die Umgebung sein, was auch die Unterschiede hinsichtlich ihrer Resistenz verglichen mit Nicht-Permafrost-Stämmen erklären könnte. Als Teil dieser Studie wurde die Raman-Spektroskopie als Analyse-Technik zur Ferndetektion von methanogenen Archaeen, welche in eine Mineral-Matrix eingebettet sind, evaluiert. Diese Dissertation trägt zu einem besseren Verständnis hinsichtlich der Grenzen für ein Überleben von methanogenen Archaeen unter simulierten Marsbedingungen bei und damit zu einer Beurteilung der Hypothese, ob es ähnliches Leben unter der Marsoberfläche geben könnte. Darüber hinaus wurde erstmalig die chemische Zusammensetzung von methanogenen Archaeen mit Hilfe der Raman-Mikrospektroskopie charakterisiert. Dieser Technologie kommt eine wesentliche Bedeutung für weitere Forschungstätigkeit in der Astrobiologie zu. KW - Methanogene Archaeen KW - sibirischen Permafrost KW - Mars KW - Raman Spektroskopie KW - Biosignaturen KW - methanogenic archaea KW - Siberian permafrost KW - Mars KW - Raman spectroscopy KW - biosignatures Y1 - 2014 U6 - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus-72299 ER - TY - JOUR A1 - de Vera, Jean-Pierre Paul A1 - Böttger, Ute A1 - de la Torre Nötzel, Rosa A1 - Sanchez, Francisco J. A1 - Grunow, Dana A1 - Schmitz, Nicole A1 - Lange, Caroline A1 - Hübers, Heinz-Wilhelm A1 - Billi, Daniela A1 - Baque, Mickael A1 - Rettberg, Petra A1 - Rabbow, Elke A1 - Reitz, Günther A1 - Berger, Thomas A1 - Möller, Ralf A1 - Bohmeier, Maria A1 - Horneck, Gerda A1 - Westall, Frances A1 - Jänchen, Jochen A1 - Fritz, Jörg A1 - Meyer, Cornelia A1 - Onofri, Silvano A1 - Selbmann, Laura A1 - Zucconi, Laura A1 - Kozyrovska, Natalia A1 - Leya, Thomas A1 - Foing, Bernard A1 - Demets, Rene A1 - Cockell, Charles S. A1 - Bryce, Casey A1 - Wagner, Dirk A1 - Serrano, Paloma A1 - Edwards, Howell G. M. A1 - Joshi, Jasmin Radha A1 - Huwe, Björn A1 - Ehrenfreund, Pascale A1 - Elsaesser, Andreas A1 - Ott, Sieglinde A1 - Meessen, Joachim A1 - Feyh, Nina A1 - Szewzyk, Ulrich A1 - Jaumann, Ralf A1 - Spohn, Tilman T1 - Supporting Mars exploration BIOMEX in Low Earth Orbit and further astrobiological studies on the Moon using Raman and PanCam technology JF - Planetary and space science N2 - The Low Earth Orbit (LEO) experiment Biology and Mars Experiment (BIOMEX) is an interdisciplinary and international space research project selected by ESA. The experiment will be accommodated on the space exposure facility EXPOSE-R2 on the International Space Station (ISS) and is foreseen to be launched in 2013. The prime objective of BIOMEX is to measure to what extent biomolecules, such as pigments and cellular components, are resistant to and able to maintain their stability under space and Mars-like conditions. The results of BIOMEX will be relevant for space proven biosignature definition and for building a biosignature data base (e.g. the proposed creation of an international Raman library). The library will be highly relevant for future space missions such as the search for life on Mars. The secondary scientific objective is to analyze to what extent terrestrial extremophiles are able to survive in space and to determine which interactions between biological samples and selected minerals (including terrestrial, Moon- and Mars analogs) can be observed under space and Mars-like conditions. In this context, the Moon will be an additional platform for performing similar experiments with negligible magnetic shielding and higher solar and galactic irradiation compared to LEO. Using the Moon as an additional astrobiological exposure platform to complement ongoing astrobiological LEO investigations could thus enhance the chances of detecting organic traces of life on Mars. We present a lunar lander mission with two related objectives: a lunar lander equipped with Raman and PanCam instruments which can analyze the lunar surface and survey an astrobiological exposure platform. This dual use of testing mission technology together with geo- and astrobiological analyses will significantly increase the science return, and support the human preparation objectives. It will provide knowledge about the Moon's surface itself and, in addition, monitor the stability of life-markers, such as cells, cell components and pigments, in an extraterrestrial environment with much closer radiation properties to the surface of Mars. The combination of a Raman data base of these data together with data from LEO and space simulation experiments, will lead to further progress on the analysis and interpretation of data that we will obtain from future Moon and Mars exploration missions. KW - Moon KW - Mars KW - Low Earth Orbit KW - Astrobiology KW - Instrumentation KW - Spectroscopy KW - Biosignature Y1 - 2012 U6 - https://doi.org/10.1016/j.pss.2012.06.010 SN - 0032-0633 VL - 74 IS - 1 SP - 103 EP - 110 PB - Elsevier CY - Oxford ER - TY - JOUR A1 - Serrano, Paloma A1 - Alawi, Mashal A1 - de Vera, Jean-Pierre Paul A1 - Wagner, Dirk T1 - Response of Methanogenic Archaea from Siberian Permafrost and Non-permafrost Environments to Simulated Mars-like Desiccation and the Presence of Perchlorate JF - Astrobiology N2 - Numerous preflight investigations were necessary prior to the exposure experiment BIOMEX on the International Space Station to test the basic potential of selected microorganisms to resist or even to be active under Mars-like conditions. In this study, methanogenic archaea, which are anaerobic chemolithotrophic microorganisms whose lifestyle would allow metabolism under the conditions on early and recent Mars, were analyzed. Some strains from Siberian permafrost environments have shown a particular resistance. In this investigation, we analyzed the response of three permafrost strains (Methanosarcina soligelidi SMA-21, Candidatus Methanosarcina SMA-17, Candidatus Methanobacterium SMA-27) and two related strains from non-permafrost environments (Methanosarcina mazei, Methanosarcina barkeri) to desiccation conditions (-80 degrees C for 315 days, martian regolith analog simulants S-MRS and P-MRS, a 128-day period of simulated Mars-like atmosphere). Exposure of the different methanogenic strains to increasing concentrations of magnesium perchlorate allowed for the study of their metabolic shutdown in a Mars-relevant perchlorate environment. Survival and metabolic recovery were analyzed by quantitative PCR, gas chromatography, and a new DNA-extraction method from viable cells embedded in S-MRS and P-MRS. All strains survived the two Mars-like desiccating scenarios and recovered to different extents. The permafrost strain SMA-27 showed an increased methanogenic activity by at least 10-fold after deep-freezing conditions. The methanogenic rates of all strains did not decrease significantly after 128 days S-MRS exposure, except for SMA-27, which decreased 10-fold. The activity of strains SMA-17 and SMA-27 decreased after 16 and 60 days P-MRS exposure. Non-permafrost strains showed constant survival and methane production when exposed to both desiccating scenarios. All strains showed unaltered methane production when exposed to the perchlorate concentration reported at the Phoenix landing site (2.4 mM) or even higher concentrations. We conclude that methanogens from (non-)permafrost environments are suitable candidates for potential life in the martian subsurface and therefore are worthy of study after space exposure experiments that approach Mars-like surface conditions. KW - Methanogenic archaea KW - Simulated Mars-like conditions KW - Subfreezing temperatures KW - Martian regolith analogs KW - Perchlorate KW - Permafrost Y1 - 2019 U6 - https://doi.org/10.1089/ast.2018.1877 SN - 1531-1074 SN - 1557-8070 VL - 19 IS - 2 SP - 197 EP - 208 PB - Liebert CY - New Rochelle ER -