Examinando por Autor "Selbmann, Laura"

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Acceso Abierto
Astrobiology of life on Earth
(Society for Applied Microbiology, 2021-04-05) Hallsworth, J. E.; Mancinelli, R. L.; Conley, C. A.; Dallas, T. D.; Rinaldi, T.; Davila, A. F.; Benison, K. C.; Rapoport, A.; Cavalazzi, B.; Selbmann, Laura; Changela, H.; Westall, Frances; Yakimov, M. M.; Amils Pibernat, R.; Madigan, M. T.; Biotechnology and Biological Sciences Research Council (BBSRC); Hallsworth, J. E. [0000-0001-6797-9362]; Mancinelli, R. L. [0000-0002-8200-4878]; Dallas, T. D. [0000-0002-5310-9857]; Rinaldi, T. [0000-0001-6291-245X]; Benison, K. C. [0000-0001-6104-2333]; Rapoport, A. [0000-0002-6185-0039]; Selbmann, L. [0000-0002-8967-3329]; Amils, R. [0000-0002-7560-1033]
Astrobiology is mistakenly regarded by some as a field confined to studies of life beyond Earth. Here, we consider life on Earth through an astrobiological lens. Whereas classical studies of microbiology historically focused on various anthropocentric sub-fields (such as fermented foods or commensals and pathogens of crop plants, livestock and humans), addressing key biological questions via astrobiological approaches can further our understanding of all life on Earth. We highlight potential implications of this approach through the articles in this Environmental Microbiology special issue ‘Ecophysiology of Extremophiles’. They report on the microbiology of places/processes including low-temperature environments and chemically diverse saline- and hypersaline habitats; aspects of sulphur metabolism in hypersaline lakes, dysoxic marine waters, and thermal acidic springs; biology of extremophile viruses; the survival of terrestrial extremophiles on the surface of Mars; biological soils crusts and rock-associated microbes of deserts; subsurface and deep biosphere, including a salticle formed within Triassic halite; and interactions of microbes with igneous and sedimentary rocks. These studies, some of which we highlight here, contribute to our understanding of the spatiotemporal reach of Earth'sfunctional biosphere, and the tenacity of terrestrial life. Their findings will help set the stage for future work focused on the constraints for life, and how organisms adapt and evolve to circumvent these constraints.
Acceso Abierto
Biosignature stability in space enables their use for life detection on Mars
(Science Advances, 2022-09-07) Baqué, Mickael; Backhaus, Theresa; Meeßen, Joachim; Hanke, Franziska; Böttger, Ute; Ramkissoon, Nisha; Olsson-Francis, Karen; Baumgärtner, Michael; Billi, Daniela; Cassaro, Alessia; de la Torre Noetzel, Maria Rosa; Demets, René; Edwards, Howell; Ehrenfreund, P.; Elsaesser, Andreas; Foing, Bernard; Foucher, Frédéric; Huwe, Björn; Joshi, Jasmin; Kozyrovska, Natalia; Lasch, Peter; Lee, Natuschka; Leuko, Stefan; Onofri, Silvano; Ott, Sieglinde; Pacelli, Claudia; Rabbow, Elke; Rothschild, Lynn; Schulze Makuch, D.; Selbmann, Laura; Serrano, Paloma; Szewzyk, Ulrich; Verseux, Cyprien; Wagner, Dirk; Westall, Frances; Zucconi, Laura; De Vera, Jean Pierre; Agenzia Spaziale Italiana (ASI); Bundesministerium für Wirtschaft und Energie (BMWi); Deutsches Zentrum für Luft- und Raumfahrt (DLR); Volkswagen Foundation; "Deutsche Forschungsgemeinschaft (DFG)
Two rover missions to Mars aim to detect biomolecules as a sign of extinct or extant life with, among other instruments, Raman spectrometers. However, there are many unknowns about the stability of Raman-detectable biomolecules in the martian environment, clouding the interpretation of the results. To quantify Raman-detectable biomolecule stability, we exposed seven biomolecules for 469 days to a simulated martian environment outside the International Space Station. Ultraviolet radiation (UVR) strongly changed the Raman spectra signals, but only minor change was observed when samples were shielded from UVR. These findings provide support for Mars mission operations searching for biosignatures in the subsurface. This experiment demonstrates the detectability of biomolecules by Raman spectroscopy in Mars regolith analogs after space exposure and lays the groundwork for a consolidated space-proven database of spectroscopy biosignatures in targeted environments.
Acceso Abierto
Limits of Life and the Habitability of Mars: The ESA Space Experiment BIOMEX on the ISS
(Mary Ann Liebert, 2019-02-11) De Vera, Jean Pierre; Alawi, Mashal; Backhaus, Theresa; Baqué, Mickael; Billi, Daniela; Böttger, Ute; Berger, T.; Bohmeier, M.; Cockell, Charles S.; Demets, René; de la Torre Noetzel, Maria Rosa; Edwards, Howell; Elsaesser, Andreas; Fagliarone, Claudia; Fiedler, Annelie; Foing, Bernard; Foucher, Frédéric; Fritz, Jörg; Hanke, Franziska; Herzog, Thomas; Horneck, Gerda; Hübers, Heinz-Wilhelm; Huwe, Björn; Joshi, Jasmin; Kozyrovska, Natalia; Kruchten, Martha; Lasch, Peter; Lee, Natuschka; Leuko, Stefan; Leya, Thomas; Lorek, Andreas; Martínez Frías, Jesús; Meessen, Joachim; Moritz, Sophie; Moeller, Ralf; Olsson-Francis, Karen; Onofri, Silvano; Ott, Sieglinde; Pacelli, Claudia; Podolich, Olga; Rabbow, Elke; Reitz, Günther; Rettberg, Petra; Reva, Oleg; Rothschild, Lynn; García Sancho, Leo; Schulze Makuch, D.; Selbmann, Laura; Serrano, Paloma; Szewzyk, Ulrich; Verseux, Cyprien; Wadsworth, Jennifer; Wagner, Dirk; Westall, Frances; Wolter, David; Zucconi, Laura; Ministerio de Economía y Competitividad (MINECO); Agencia Estatal de Investigación (AEI); Agenzia Spaziale Italiana (ASI); National Academy of Sciences of Ukraine (NASU); German Centre for Air and Space Travel; Helmholtz Association
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.