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      Limits of Life and the Habitability of Mars: The ESA Space Experiment BIOMEX on the ISS

      research-article
      1 , 2 , 3 , 1 , 4 , 5 , 6 , 6 , 7 , 8 , 9 , 10 , 11 , 4 , 12 , 8 , 13 , 14 , 5 , 15 , 6 , 5 , 12 , 12, , 16 , 17 , 3 , 18 , 19 , 6 , 20 , 1 , 21 , 3 , 12 , 6 , 22 , 23 , 3 , 23 , 17 , 6 , 6 , 6 , 24 , 25 , 26 , 27 , 23, , 28 , 2, , 29 , 30 , 4 , 7 , 2, , 31 , 13 , 1 , 23
      Astrobiology
      Mary Ann Liebert, Inc., publishers
      EXPOSE-R2, BIOMEX, Habitability, Limits of life, Extremophiles, Mars

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          Abstract

          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.

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          Most cited references79

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          Phyllosilicates on Mars and implications for early martian climate.

          The recent identification of large deposits of sulphates by remote sensing and in situ observations has been considered evidence of the past presence of liquid water on Mars. Here we report the unambiguous detection of diverse phyllosilicates, a family of aqueous alteration products, on the basis of observations by the OMEGA imaging spectrometer on board the Mars Express spacecraft. These minerals are mainly associated with Noachian outcrops, which is consistent with an early active hydrological system, sustaining the long-term contact of igneous minerals with liquid water. We infer that the two main families of hydrated alteration products detected-phyllosilicates and sulphates--result from different formation processes. These occurred during two distinct climatic episodes: an early Noachian Mars, resulting in the formation of hydrated silicates, followed by a more acidic environment, in which sulphates formed.
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            Mars surface diversity as revealed by the OMEGA/Mars Express observations.

            The Observatoire pour la Minéralogie, l'Eau, les Glaces, et l'Activité (OMEGA) investigation, on board the European Space Agency Mars Express mission, is mapping the surface composition of Mars at a 0.3- to 5-kilometer resolution by means of visible-near-infrared hyperspectral reflectance imagery. The data acquired during the first 9 months of the mission already reveal a diverse and complex surface mineralogy, offering key insights into the evolution of Mars. OMEGA has identified and mapped mafic iron-bearing silicates of both the northern and southern crust, localized concentrations of hydrated phyllosilicates and sulfates but no carbonates, and ices and frosts with a water-ice composition of the north polar perennial cap, as for the south cap, covered by a thin carbon dioxide-ice veneer.
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              Detection of methane in the atmosphere of Mars.

              We report a detection of methane in the martian atmosphere by the Planetary Fourier Spectrometer onboard the Mars Express spacecraft. The global average methane mixing ratio is found to be 10 +/- 5 parts per billion by volume (ppbv). However, the mixing ratio varies between 0 and 30 ppbv over the planet. The source of methane could be either biogenic or nonbiogenic, including past or present subsurface microorganisms, hydrothermal activity, or cometary impacts.
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                Author and article information

                Journal
                Astrobiology
                Astrobiology
                ast
                Astrobiology
                Mary Ann Liebert, Inc., publishers (140 Huguenot Street, 3rd FloorNew Rochelle, NY 10801USA )
                1531-1074
                1557-8070
                01 February 2019
                12 February 2019
                12 February 2019
                : 19
                : 2
                : 145-157
                Affiliations
                [ 1 ]German Aerospace Center (DLR), Institute of Planetary Research, Management and Infrastructure, Research Group Astrobiological Laboratories, Berlin, Germany.
                [ 2 ]GFZ, German Research Centre for Geosciences, Helmholtz Centre Potsdam, Section 5.3 Geomicrobiology, Telegrafenberg, Potsdam, Germany.
                [ 3 ]Institut für Botanik, Heinrich-Heine-Universität (HHU), Düsseldorf, Germany.
                [ 4 ]University of Rome Tor Vergata, Department of Biology, Rome, Italy.
                [ 5 ]German Aerospace Center (DLR), Institute for Optical Sensor Systems, Berlin, Germany.
                [ 6 ]German Aerospace Center (DLR), Institute of Aerospace Medicine, Radiation Biology Department, Köln, Germany.
                [ 7 ]School of Physics and Astronomy, University of Edinburgh, Edinburgh, UK.
                [ 8 ]European Space Research and Technology Centre (ESTEC), European Space Agency (ESA), Noordwijk, the Netherlands.
                [ 9 ]Departamento de Observación de la Tierra, Instituto Nacional de Técnica Aeroespacial (INTA), Madrid, Spain.
                [ 10 ]Raman Spectroscopy Group, University Analytical Centre, Division of Chemical and Forensic Sciences, University of Bradford, West Yorkshire, UK.
                [ 11 ]Institut für experimentelle Physik, Experimentelle Molekulare Biophysik, Frei Universität Berlin, Berlin, Germany.
                [ 12 ]University of Potsdam, Biodiversity Research/Systematic Botany, Potsdam, Germany.
                [ 13 ]CNRS, Centre de Biophysique Moléculaire, UPR 4301, Orléans, France.
                [ 14 ]Museum für Naturkunde - Leibniz Institute for Evolution and Biodiversity Science, Berlin, Germany.
                [ 15 ]TH Wildau (Technical University of Applied Sciences), Wildau, Germany.
                [ 16 ]Hochschule für Technik HSR Rapperswil, Institute for Landscape and Open Space, Rapperswil, Switzerland.
                [ 17 ]Institute of Molecular Biology & Genetics of NASU, Kyiv, Ukraine.
                [ 18 ]Robert Koch Institute, Centre for Biological Threats and Special Pathogens, Berlin, Germany.
                [ 19 ]Department of Ecology and Environmental Sciences, Umeå University, Umeå, Sweden.
                [ 20 ]Extremophile Research & Biobank CCCryo, Fraunhofer Institute for Cell Therapy and Immunology, Branch Bioanalytics and Bioprocesses (IZI-BB), Potsdam, Germany.
                [ 21 ]Instituto de Geociencias, CSIC-Universidad Complutense de Madrid, Madrid, Spain.
                [ 22 ]School of Environment, Earth and Ecosystem Sciences, The Open University, Milton Keynes, UK.
                [ 23 ]Department of Ecological and Biological Sciences, University of Tuscia, Viterbo, Italy.
                [ 24 ]Centre for Bioinformatics and Computational Biology, Department of Biochemistry, Genetics and Microbiology, University of Pretoria, Pretoria, South Africa.
                [ 25 ]NASA Ames Research Center, Moffett Field, California, USA.
                [ 26 ]UCM, Universidad Complutense Madrid, Madrid, Spain.
                [ 27 ]Technical University Berlin, ZAA, Berlin, Germany.
                [ 28 ]Italian National Antarctic Museum (MNA), Mycological Section, Genoa, Italy.
                [ 29 ]AWI, Alfred Wegener Institute, Helmholtz Centre for Polar and Marine Research, Potsdam, Germany.
                [ 30 ]TU Berlin, Institute of Environmental Technology, Environmental Microbiology, Berlin, Germany.
                [ 31 ]University of Potsdam, Institute of Earth and Environmental Sciences, Potsdam, Germany.
                Author notes
                [*]Address correspondence to: Jean-Pierre de Vera, German Aerospace Center (DLR), Institute of Planetary Research, Management and Infrastructure, Research Group Astrobiological Laboratories, Rutherfordstr. 2, 12489 Berlin, Germany jean-pierre.devera@ 123456dlr.de
                Article
                10.1089/ast.2018.1897
                10.1089/ast.2018.1897
                6383581
                30742496
                c443af5f-ed8e-4379-a41e-4cbb66026cc1
                © Jean-Pierre de Vera et al., 2019; Published by Mary Ann Liebert, Inc.

                This Open Access article is distributed under the terms of the Creative Commons Attribution Noncommercial License ( http://creativecommons.org/licenses/by-nc/4.0/) which permits any noncommercial use, distribution, and reproduction in any medium, provided the original author(s) and the source are credited.

                History
                : 29 April 2018
                : 07 January 2019
                Page count
                Figures: 6, Tables: 6, References: 71, Pages: 13
                Categories
                Introduction

                expose-r2,biomex,habitability,limits of life,extremophiles,mars
                expose-r2, biomex, habitability, limits of life, extremophiles, mars

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