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Kaur J, Kaur J, Nigam A. Extremophiles in Space Exploration. Indian J Microbiol 2024; 64:418-428. [PMID: 39010991 PMCID: PMC11246395 DOI: 10.1007/s12088-024-01297-4] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/14/2024] [Accepted: 04/28/2024] [Indexed: 07/17/2024] Open
Abstract
In the era of deep space exploration, extremophile research represents a key area of research w.r.t space survival. This review thus delves into the intriguing realm of 'Space and Astro Microbiology', providing insights into microbial survival, resilience, and behavioral adaptations in space-like environments. This discussion encompasses the modified behavior of extremophilic microorganisms, influencing virulence, stress resistance, and gene expression. It then shifts to recent studies on the International Space Station and simulated microgravity, revealing microbial responses that impact drug susceptibility, antibiotic resistance, and its commercial implications. The review then transitions into Astro microbiology, exploring the possibilities of interplanetary transit, lithopanspermia, and terraforming. Debates on life's origin and recent Martian meteorite discoveries are noted. We also discuss Proactive Inoculation Protocols for selecting adaptable microorganisms as terraforming pioneers. The discussion concludes with a note on microbes' role as bioengineers in bioregenerative life support systems, in recycling organic waste for sustainable space travel; and in promoting optimal plant growth to prepare Martian and lunar basalt. This piece emphasizes the transformative impact of microbes on the future of space exploration.
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Affiliation(s)
- Jasvinder Kaur
- Gargi College, University of Delhi, Siri Fort Road, New Delhi, 110 049 India
| | - Jaspreet Kaur
- Maitreyi College, University of Delhi, New Delhi, 110 021 India
| | - Aeshna Nigam
- Shivaji College, University of Delhi, New Delhi, 110 027 India
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2
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Sephton MA, Freeman K, Hays L, Thiessen F, Benison K, Carrier B, Dworkin JP, Glamoclija M, Gough R, Onofri S, Peterson R, Quinn R, Russell S, Stüeken EE, Velbel M, Zolotov M. Thresholds of Temperature and Time for Mars Sample Return: Final Report of the Mars Sample Return Temperature-Time Tiger Team. ASTROBIOLOGY 2024; 24:443-488. [PMID: 38768433 DOI: 10.1089/ast.2023.0098] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/22/2024]
Affiliation(s)
- Mark A Sephton
- Imperial College London, Earth Science and Engineering, South Kensington Campus, London, UK
| | - Kate Freeman
- The Pennsylvania State University, Geosciences, University Park, Pennsylvania, USA
| | - Lindsay Hays
- NASA Headquarters, Mars Sample Return Program, Washington, DC, USA
| | - Fiona Thiessen
- European Space Research and Technology Centre, Noordwijk, South Holland, Netherlands
| | - Kathleen Benison
- West Virginia University, Department of Geology and Geography, Morgantown, West Virginia, USA
| | - Brandi Carrier
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA
| | - Jason P Dworkin
- NASA Goddard Space Flight Center, Astrochemistry, Greenbelt, Maryland, USA
| | - Mihaela Glamoclija
- Rutgers University Newark College of Arts and Sciences, Earth and Environmental Sciences, Newark, New Jersey, USA
| | - Raina Gough
- University of Colorado, Department of Chemistry and Biochemistry, Boulder, Colorado, USA
| | - Silvano Onofri
- University of Tuscia, Department of Ecological and Biological Sciences, Largo dell'Università snc Viterbo, Italy
| | | | - Richard Quinn
- NASA Ames Research Center, Moffett Field, California, USA
| | - Sara Russell
- Natural History Museum, Department of Earth Sciences, London, UK
| | - Eva E Stüeken
- University of St Andrews, School of Earth and Environmental Sciences, St Andrews, Fife, UK
| | - Michael Velbel
- Michigan State University, Earth and Environmental Sciences, East Lansing, Michigan, USA
- Smithsonian Institution, Department of Mineral Sciences, National Museum of Natural History, Washington, DC, USA
| | - Mikhail Zolotov
- Arizona State University, School of Earth and Space Exploration, Tempe, Arizona, USA
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3
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Deshevaya EA, Fialkina SV, Shubralova EV, Tsygankov OS, Khamidullina NM, Vasilyak LM, Pecherkin VY, Shcherbakova VA, Nosovsky AM, Orlov ОI. Survival of microorganisms during two-year exposure in outer space near the ISS. Sci Rep 2024; 14:334. [PMID: 38172103 PMCID: PMC10764764 DOI: 10.1038/s41598-023-49525-z] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 05/01/2023] [Accepted: 12/08/2023] [Indexed: 01/05/2024] Open
Abstract
Results of an experiment named "Test" on survival and variability of microorganisms in open space near the International Space Station are presented. It was found after two-years exposure, spore-forming bacteria of the species Bacillus subtilis, fungi of the species Aureobasidium pullulans and archaea of the species Methanosarcina mazei S-6T, deposited on cotton wool, are able to survive, and their numbers decreased equally, regardless of whether the microorganisms belong to different taxonomic groups. The main factors for the long-term survival could be the result of their dehydration and partial lyophilization in the vacuum of near-Earth space. For the first time, after being in outer space, cyst-like cells of the archaea strain M. mazei S-6T and a 14-day delay in their growth were detected when cultured on a nutrient medium compared to the ground-based control strain. In 30% of fungi species strains A. pullulans, isolated after a two-year stay in outer space, the resistance to γ-radiation increased compared to the control strain. It was found that the reaction to the action of various concentrations of hydrogen peroxide and 1% chlorine in the surviving strains of the fungus A. pullulans on the ISS is less pronounced than in the control strain.
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Affiliation(s)
- Elena A Deshevaya
- State Scientific Center of the Russian Federation - Institute of Biomedical Problems of the Russian Academy of Sciences, Moscow, Russia
| | - Svetlana V Fialkina
- State Scientific Center of the Russian Federation - Institute of Biomedical Problems of the Russian Academy of Sciences, Moscow, Russia
| | - Elena V Shubralova
- Joint Stock Company «Central Research Institute for Machine Building», Moscow Region, Russia
| | - Oleg S Tsygankov
- Rocket and Space Public Corporation Energia, Moscow Region, Russia
| | | | - Leonid M Vasilyak
- Joint Institute for High Temperatures of the Russian Academy of Sciences, Moscow, Russia
| | - Vladimir Ya Pecherkin
- Joint Institute for High Temperatures of the Russian Academy of Sciences, Moscow, Russia.
| | - Viktoria A Shcherbakova
- Pushchino Scientific Center for Biological Research of the Russian Academy of Sciences, Skryabin Institute of Biochemistry and Physiology of Microorganisms, Moscow Region, Russia
| | - Andrey M Nosovsky
- State Scientific Center of the Russian Federation - Institute of Biomedical Problems of the Russian Academy of Sciences, Moscow, Russia
| | - Оleg I Orlov
- State Scientific Center of the Russian Federation - Institute of Biomedical Problems of the Russian Academy of Sciences, Moscow, Russia
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Perera LJ, Cockell CS. Dispersion of Bacteria by Low-Pressure Boiling: Life Detection in Enceladus' Plume Material. ASTROBIOLOGY 2023; 23:269-279. [PMID: 36689196 DOI: 10.1089/ast.2022.0009] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/17/2023]
Abstract
The plume of Enceladus is thought to originate from the dispersion of a liquid source beneath the icy crust. Cryovolcanic activity on Enceladus may present a direct way of accessing material originating from the potentially habitable subsurface ocean. One way to test the hypothesis of whether life is present within the ocean of Enceladus would be to investigate the plume material for the presence of microbial life. In this study, we investigated the entrainment of Bacillus subtilis within Enceladus-like fluids under boiling conditions caused by exposure of the fluids to low pressure. We show that boiling, associated with exposure of a fluid to low pressure, works as a mechanism for dispersing bacteria in Enceladus plume-like environments. Exposure of Enceladus-type fluids (0.01-0.1 molal Na2CO3 and 0.05-0.2 molal NaCl) to low pressure (5 mbar) results in the dispersion of bacteria in droplets that evaporate to produce particles of salt. We find that, for particles with radius (r) ≤ 10 μm, the number of dispersed particles containing cells was between 7.7% and 10.9%. However, for larger particles 10 < r ≤ 50 μm, 64.4% and 56.4% contained cells for lower and upper end-member solutions, respectively. Our results suggest that the gravity-induced size sorting of plume particles will result in plume deposits closer to the vent source containing a larger volume of biological material than within the plume. If life is present in the ocean of Enceladus, we would expect that it would be effectively entrained and deposited on the surface; therefore, it would be accessible with a surface-lander-based instrument.
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Affiliation(s)
- L J Perera
- UK Centre for Astrobiology, University of Edinburgh, Edinburgh, UK
| | - C S Cockell
- UK Centre for Astrobiology, University of Edinburgh, Edinburgh, UK
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Olsson-Francis K, Doran PT, Ilyin V, Raulin F, Rettberg P, Kminek G, Mier MPZ, Coustenis A, Hedman N, Shehhi OA, Ammannito E, Bernardini J, Fujimoto M, Grasset O, Groen F, Hayes A, Gallagher S, Kumar K P, Mustin C, Nakamura A, Seasly E, Suzuki Y, Peng J, Prieto-Ballesteros O, Sinibaldi S, Xu K, Zaitsev M. The COSPAR Planetary Protection Policy for robotic missions to Mars: A review of current scientific knowledge and future perspectives. LIFE SCIENCES IN SPACE RESEARCH 2023; 36:27-35. [PMID: 36682826 DOI: 10.1016/j.lssr.2022.12.001] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/03/2022] [Revised: 12/07/2022] [Accepted: 12/09/2022] [Indexed: 06/17/2023]
Abstract
Planetary protection guidance for martian exploration has become a notable point of discussion over the last decade. This is due to increased scientific interest in the habitability of the red planet with updated techniques, missions becoming more attainable by smaller space agencies, and both the private sector and governments engaging in activities to facilitate commercial opportunities and human-crewed missions. The international standards for planetary protection have been developed through consultation with the scientific community and the space agencies by the Committee on Space Research's (COSPAR) Panel on Planetary Protection, which provides guidance for compliance with the Outer Space Treaty of 1967. In 2021, the Panel evaluated recent scientific data and literature regarding the planetary protection requirements for Mars and the implications of this on the guidelines. In this paper, we discuss the COSPAR Planetary Protection Policy for Mars, review the new scientific findings and discuss the next steps required to enable the next generation of robotic missions to Mars.
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Affiliation(s)
- Karen Olsson-Francis
- AstrobiologyOU, Faculty of Science, Technology, Engineering and Mathematics, The Open University, Milton Keynes, UK.
| | - Peter T Doran
- Department of Geology and Geophysics, Louisiana State, Baton Rouge, Louisiana, USA
| | - Vyacheslav Ilyin
- Institute for Biomedical Problems, Russian Academy of Sciences, Moscow, Russia
| | - Francois Raulin
- Univ Paris Est Cr Univ Paris Est Créteil and Université Paris Cité, CNRS, LISA, F-94010 Créteil, France
| | - Petra Rettberg
- German Aerospace Center (DLR), Institute of Aerospace Medicine, Radiation Biology Department, Research Group Astrobiology, 51147 Cologne, Germany
| | | | - María-Paz Zorzano Mier
- Centro deAstrobiología (CAB), CSIC-INTA, Carretera de Ajalvir km 4, 28850 Torrejón de Ardoz, Madrid, Spain
| | - Athena Coustenis
- LESIA, Paris Observatory, PSL University, CNRS, Paris University, 92195 Meudon Cedex, France
| | - Niklas Hedman
- Committee, Policy and Legal Affairs Section, Office for Outer Space Affairs, United Nations Office at Vienna, Austria
| | | | | | - James Bernardini
- Office of Safety and Mission Assurance, NASA Headquarters, Washington, DC 20546, USA
| | - Masaki Fujimoto
- Japan Aerospace Exploration Agency (JAXA), Institute of Space and Astronautical Science (ISAS), Kanagawa, Japan
| | | | - Frank Groen
- Office of Safety and Mission Assurance, NASA Headquarters, Washington, DC 20546, USA
| | - Alex Hayes
- Cornell University, Ithaca, NY 14853-6801, USA
| | - Sarah Gallagher
- Institute of Earth and Space Exploration, Western University, London, Ontario, Canada
| | | | | | - Akiko Nakamura
- Department of Earth and Planetary Science, The University of Tokyo,7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan
| | - Elaine Seasly
- Office of Safety and Mission Assurance, NASA Headquarters, Washington, DC 20546, USA
| | - Yohey Suzuki
- Department of Earth and Planetary Science, The University of Tokyo,7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan
| | - Jing Peng
- China National Space Administration, Beijing, China
| | - Olga Prieto-Ballesteros
- Centro deAstrobiología (CAB), CSIC-INTA, Carretera de Ajalvir km 4, 28850 Torrejón de Ardoz, Madrid, Spain
| | | | - Kanyan Xu
- Laboratory of Space Microbiology, Shenzhou Space Biotechnology Group, Chinese Academy of Space Technology, Beijing, China
| | - Maxim Zaitsev
- Planetary Physics Dept., Space Research Inst. of Russian Acad. of Sciences, Moscow, Russia
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Schuerger AC. Microbial Protocols for Spacecraft: 1. Effects of Surface Texture, Low Pressure, and UV Irradiation on Recovery of Microorganisms from Surfaces. ASTROBIOLOGY 2022; 22:1061-1071. [PMID: 35675686 DOI: 10.1089/ast.2021.0141] [Citation(s) in RCA: 3] [Impact Index Per Article: 1.5] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/15/2023]
Abstract
Modeling risks for the forward contamination of planetary surfaces from endemic bioburdens on landed spacecraft requires precise data on the biocidal effects of space factors on microbial survival. Numerous studies have been published over the preceding 60 years on the survival of diverse microorganisms exposed to solar heating, solar ultraviolet (UV) irradiation, vacuum, ionizing radiation, desiccation, and many other planetary surface conditions. These data were generated with diverse protocols that can impair the interpretations of the results due to dynamic experimental errors inherent in all lab protocols. The current study (1) presents data on how metal surfaces can affect spore adhesion, (2) proposes doping and extraction protocols that can achieve very high recovery rates (close to 100%) from aluminum coupons with four Bacillus spp., (3) establishes a timeline in which dried spores on aluminum coupons should be used to minimize aging effects of spore monolayers, (4) confirms that vacuum alone does not dislodge spores dried on aluminum coupons, and (5) establishes that multiple UV irradiation sources yield similar results if properly cross-calibrated. The protocols are given to advance discussions in the planetary protection community on how to standardize lab protocols to align results from diverse labs into a coherent interpretation of how space conditions will degrade microbial survival over time.
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Affiliation(s)
- Andrew C Schuerger
- Department of Plant Pathology, University of Florida, Space Life Sciences Lab, Exploration Park, Merritt Island, Florida, USA
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Weingarten EA, Zee PC, Jackson CR. Microbial Communities in Saltpan Sediments Show Tolerance to Mars Analog Conditions, but Susceptibility to Chloride and Perchlorate Toxicity. ASTROBIOLOGY 2022; 22:838-850. [PMID: 35731161 PMCID: PMC9464085 DOI: 10.1089/ast.2021.0132] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 08/12/2021] [Accepted: 02/28/2022] [Indexed: 06/15/2023]
Abstract
Brines at or near the surface of present-day Mars are a potential explanation for seasonally recurring dark streaks on the walls of craters, termed recurring slope lineae (RSL). Deliquescence and freezing point depression are possible drivers of brine stability, attributable to the high salinity observed in martian regolith including chlorides and perchlorates. Investigation of life, which may inhabit RSL, and the cellular mechanisms necessary for survival, must consider the tolerance of highly variable hydration, freeze-thaw cycles, and high osmolarity in addition to the anaerobic, oligotrophic, and irradiated environment. We propose the saltpan, an ephemeral, hypersaline wetland as an analogue for putative RSL hydrology. Saltpan sediment archaeal and bacterial communities showed tolerance of the Mars-analogous atmosphere, hydration, minerology, salinity, and temperature. Although active growth and a shift to well-adapted taxa were observed, susceptibility to low-concentration chloride and perchlorate addition suggested that such a composition was insufficient for beneficial water retention relative to added salt stress.
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Affiliation(s)
- Eric A. Weingarten
- Department of Biology, University of Mississippi, University, Mississippi, USA
- U.S. Army Engineer Research and Development Center, Vicksburg, Mississippi, USA
| | - Peter C. Zee
- Department of Biology, University of Mississippi, University, Mississippi, USA
| | - Colin R. Jackson
- Department of Biology, University of Mississippi, University, Mississippi, USA
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Proteomic Response of Deinococcus radiodurans to Short-Term Real Microgravity during Parabolic Flight Reveals Altered Abundance of Proteins Involved in Stress Response and Cell Envelope Functions. Life (Basel) 2021; 12:life12010023. [PMID: 35054415 PMCID: PMC8779699 DOI: 10.3390/life12010023] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 11/25/2021] [Revised: 12/17/2021] [Accepted: 12/20/2021] [Indexed: 12/22/2022] Open
Abstract
Rapidly evolving space exploration makes understanding the short- and long- term effects of microgravity on humans, plants, and microorganisms an important task. The ubiquitous presence of the gravitational force has had an influence on the development of all living entities on Earth, and short- and long-term changes in perceived gravitational force can induce notable changes within cells. Deinococcus radiodurans is the Gram-positive bacterium that is best known for its extreme resistance to UV-C and gamma radiation, oxidation stress, and desiccation. Thus increased interest has been placed on this species in the context of space research. The present study aims to elucidate the short-term proteomic response of this species to real microgravity during parabolic flight. Overnight cultures of D. radiodurans were subjected to microgravity during a single parabola, and metabolic activity was quenched using methanol. Proteins were extracted and subsequently measured using HPLC nESI MS/MS. The results, such as the enrichment of the peptidoglycan biosynthesis pathway with differentially abundant proteins and altered S-layer protein abundance, suggested molecular rearrangements in the cell envelope of D. radiodurans. Altered abundance of proteins involved in energy metabolism and DNA repair could be linked with increased endogenous ROS production that contributes to the stress response. Moreover, changes in protein abundance in response to microgravity show similarities with previously reported stress responses. Thus, the present results could be used to further investigate the complex regulation of the remarkable stress management of this bacterium.
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Fan W, Cui J, Li Q, Huo Y, Xiao D, Yang X, Yu H, Wang C, Jarvis P, Lyu T, Huo M. Bactericidal efficiency and photochemical mechanisms of micro/nano bubble-enhanced visible light photocatalytic water disinfection. WATER RESEARCH 2021; 203:117531. [PMID: 34388494 DOI: 10.1016/j.watres.2021.117531] [Citation(s) in RCA: 20] [Impact Index Per Article: 6.7] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 06/22/2021] [Revised: 07/28/2021] [Accepted: 08/03/2021] [Indexed: 06/13/2023]
Abstract
Microbial contamination of water in the form of highly-resistant bacterial spores can cause a long-term risk of waterborne disease. Advanced photocatalysis has become an effective approach to inactivate bacterial spores due to its potential for efficient solar energy conversion alongside reduced formation of disinfection by-products. However, the overall efficiency of the process still requires significant improvements. Here, we proposed and evaluated a novel visible light photocatalytic water disinfection technology by its close coupling with micro/nano bubbles (MNBs). The inactivation rate constant of Bacillus subtilis spores reached 1.28 h-1, which was 5.6 times higher than that observed for treatment without MNBs. The superior performance for the progressive destruction of spores' cells during the treatment was confirmed by transmission electron microscopy (TEM) and excitation-emission matrix (EEM) spectra determination. Experiments using scavengers of reactive oxygen species (ROSs) revealed that H2O2 and •OH were the primary active species responsible for the inactivation of spores. The effective supply of oxygen from air MNBs helped accelerate the hole oxidation of H2O2 on the photocatalyst (i.e. Ag/TiO2). In addition, the interfacial photoelectric effect from the MNBs was also confirmed to contribute to the spore inactivation. Specifically, MNBs induced strong light scattering, consequently increasing the optical path length in the photocatalysis medium by 54.8% at 700nm and enhancing light adsorption of the photocatalyst. The non-uniformities in dielectricity led to a high-degree of heterogeneity of the electric field, which triggered the formation of a region of enhanced light intensity which ultimately promoted the photocatalytic reaction. Overall, this study provided new insights on the mechanisms of photocatalysis coupled with MNB technology for advanced water treatment.
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Affiliation(s)
- Wei Fan
- School of Environment, Northeast Normal University, 2555 Jingyue Street, Changchun 130117, China
| | - Jingyu Cui
- School of Environment, Northeast Normal University, 2555 Jingyue Street, Changchun 130117, China
| | - Qi Li
- School of Environment, Northeast Normal University, 2555 Jingyue Street, Changchun 130117, China
| | - Yang Huo
- National Demonstration Center for Experimental Physics Education, Northeast Normal University, Changchun 130024, China
| | - Dan Xiao
- Jilin Academy of Agricultural Science, 1363 Shengtai Street, Changchun 130033, China
| | - Xia Yang
- School of Environment, Northeast Normal University, 2555 Jingyue Street, Changchun 130117, China
| | - Hongbin Yu
- School of Environment, Northeast Normal University, 2555 Jingyue Street, Changchun 130117, China
| | - Chunliang Wang
- National Demonstration Center for Experimental Physics Education, Northeast Normal University, Changchun 130024, China.
| | - Peter Jarvis
- Cranfield Water Science Institute, Cranfield University, College Road, Cranfield, Bedfordshire MK43 0AL, United Kingdom
| | - Tao Lyu
- Cranfield Water Science Institute, Cranfield University, College Road, Cranfield, Bedfordshire MK43 0AL, United Kingdom.
| | - Mingxin Huo
- School of Environment, Northeast Normal University, 2555 Jingyue Street, Changchun 130117, China
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10
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Ott E, Kawaguchi Y, Kölbl D, Rabbow E, Rettberg P, Mora M, Moissl-Eichinger C, Weckwerth W, Yamagishi A, Milojevic T. Molecular repertoire of Deinococcus radiodurans after 1 year of exposure outside the International Space Station within the Tanpopo mission. MICROBIOME 2020; 8:150. [PMID: 33121542 PMCID: PMC7597052 DOI: 10.1186/s40168-020-00927-5] [Citation(s) in RCA: 11] [Impact Index Per Article: 2.8] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/01/2020] [Accepted: 09/24/2020] [Indexed: 05/10/2023]
Abstract
BACKGROUND The extraordinarily resistant bacterium Deinococcus radiodurans withstands harsh environmental conditions present in outer space. Deinococcus radiodurans was exposed for 1 year outside the International Space Station within Tanpopo orbital mission to investigate microbial survival and space travel. In addition, a ground-based simulation experiment with conditions, mirroring those from low Earth orbit, was performed. METHODS We monitored Deinococcus radiodurans cells during early stage of recovery after low Earth orbit exposure using electron microscopy tools. Furthermore, proteomic, transcriptomic and metabolomic analyses were performed to identify molecular mechanisms responsible for the survival of Deinococcus radiodurans in low Earth orbit. RESULTS D. radiodurans cells exposed to low Earth orbit conditions do not exhibit any morphological damage. However, an accumulation of numerous outer-membrane-associated vesicles was observed. On levels of proteins and transcripts, a multi-faceted response was detected to alleviate cell stress. The UvrABC endonuclease excision repair mechanism was triggered to cope with DNA damage. Defense against reactive oxygen species is mirrored by the increased abundance of catalases and is accompanied by the increased abundance of putrescine, which works as reactive oxygen species scavenging molecule. In addition, several proteins and mRNAs, responsible for regulatory and transporting functions showed increased abundances. The decrease in primary metabolites indicates alternations in the energy status, which is needed to repair damaged molecules. CONCLUSION Low Earth orbit induced molecular rearrangements trigger multiple components of metabolic stress response and regulatory networks in exposed microbial cells. Presented results show that the non-sporulating bacterium Deinococcus radiodurans survived long-term low Earth orbit exposure if wavelength below 200 nm are not present, which mirrors the UV spectrum of Mars, where CO2 effectively provides a shield below 190 nm. These results should be considered in the context of planetary protection concerns and the development of new sterilization techniques for future space missions. Video Abstract.
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Affiliation(s)
- Emanuel Ott
- Space Biochemistry Group, Department of Biophysical Chemistry, University of Vienna, Vienna, Austria
| | - Yuko Kawaguchi
- Planetary Exploration Research Center (PERC), Chiba Institute of Technology (CIT), Chiba, Japan
| | - Denise Kölbl
- Space Biochemistry Group, Department of Biophysical Chemistry, University of Vienna, Vienna, Austria
| | - Elke Rabbow
- Institute of Aerospace Medicine, Radiation Biology Department, German Aerospace Center, Cologne, Germany
| | - Petra Rettberg
- Institute of Aerospace Medicine, Radiation Biology Department, German Aerospace Center, Cologne, Germany
| | - Maximilian Mora
- Department of Internal Medicine, Section of Infectious Diseases and Tropical Medicine, Medical University Graz, Graz, Austria
| | - Christine Moissl-Eichinger
- Department of Internal Medicine, Section of Infectious Diseases and Tropical Medicine, Medical University Graz, Graz, Austria
| | - Wolfram Weckwerth
- Department of Ecogenomics and Systems Biology, University of Vienna, Vienna, Austria
- Vienna Metabolomics Center (VIME), University of Vienna, Vienna, Austria
| | - Akihiko Yamagishi
- Department of Life Science, Tokyo Institute of Technology, Nagatsuta, Yokohama, Japan
| | - Tetyana Milojevic
- Space Biochemistry Group, Department of Biophysical Chemistry, University of Vienna, Vienna, Austria.
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11
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Kawaguchi Y, Shibuya M, Kinoshita I, Yatabe J, Narumi I, Shibata H, Hayashi R, Fujiwara D, Murano Y, Hashimoto H, Imai E, Kodaira S, Uchihori Y, Nakagawa K, Mita H, Yokobori SI, Yamagishi A. DNA Damage and Survival Time Course of Deinococcal Cell Pellets During 3 Years of Exposure to Outer Space. Front Microbiol 2020; 11:2050. [PMID: 32983036 PMCID: PMC7479814 DOI: 10.3389/fmicb.2020.02050] [Citation(s) in RCA: 35] [Impact Index Per Article: 8.8] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 06/01/2020] [Accepted: 08/05/2020] [Indexed: 11/13/2022] Open
Abstract
The hypothesis called “panspermia” proposes an interplanetary transfer of life. Experiments have exposed extremophilic organisms to outer space to test microbe survivability and the panspermia hypothesis. Microbes inside shielding material with sufficient thickness to protect them from UV-irradiation can survive in space. This process has been called “lithopanspermia,” meaning rocky panspermia. We previously proposed sub-millimeter cell pellets (aggregates) could survive in the harsh space environment based on an on-ground laboratory experiment. To test our hypothesis, we placed dried cell pellets of the radioresistant bacteria Deinococcus spp. in aluminum plate wells in exposure panels attached to the outside of the International Space Station (ISS). We exposed microbial cell pellets with different thickness to space environments. The results indicated the importance of the aggregated form of cells for surviving in harsh space environment. We also analyzed the samples exposed to space from 1 to 3 years. The experimental design enabled us to get and extrapolate the survival time course to predict the survival time of Deinococcus radiodurans. Dried deinococcal cell pellets of 500 μm thickness were alive after 3 years of space exposure and repaired DNA damage at cultivation. Thus, cell pellets 1 mm in diameter have sufficient protection from UV and are estimated to endure the space environment for 2–8 years, extrapolating the survival curve and considering the illumination efficiency of the space experiment. Comparison of the survival of different DNA repair-deficient mutants suggested that cell aggregates exposed in space for 3 years suffered DNA damage, which is most efficiently repaired by the uvrA gene and uvdE gene products, which are responsible for nucleotide excision repair and UV-damage excision repair. Collectively, these results support the possibility of microbial cell aggregates (pellets) as an ark for interplanetary transfer of microbes within several years.
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Affiliation(s)
- Yuko Kawaguchi
- School of Life Sciences, Tokyo University of Pharmacy and Life Sciences, Hachioji, Japan
| | - Mio Shibuya
- School of Life Sciences, Tokyo University of Pharmacy and Life Sciences, Hachioji, Japan
| | - Iori Kinoshita
- School of Life Sciences, Tokyo University of Pharmacy and Life Sciences, Hachioji, Japan
| | - Jun Yatabe
- School of Life Sciences, Tokyo University of Pharmacy and Life Sciences, Hachioji, Japan
| | - Issay Narumi
- Faculty of Life Sciences, Toyo University, Oura-gun, Japan
| | - Hiromi Shibata
- The Institute of Scientific and Industrial Research, Osaka University, Ibaraki, Japan
| | - Risako Hayashi
- School of Life Sciences, Tokyo University of Pharmacy and Life Sciences, Hachioji, Japan
| | - Daisuke Fujiwara
- School of Life Sciences, Tokyo University of Pharmacy and Life Sciences, Hachioji, Japan
| | - Yuka Murano
- School of Life Sciences, Tokyo University of Pharmacy and Life Sciences, Hachioji, Japan
| | - Hirofumi Hashimoto
- Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan
| | - Eiichi Imai
- Department of Bioengineering, Nagaoka University of Technology, Nagaoka, Japan
| | - Satoshi Kodaira
- National Institute of Radiological Sciences, National Institutes for Quantum and Radiological Science and Technology, Chiba, Japan
| | - Yukio Uchihori
- National Institute of Radiological Sciences, National Institutes for Quantum and Radiological Science and Technology, Chiba, Japan
| | - Kazumichi Nakagawa
- The Institute of Scientific and Industrial Research, Osaka University, Ibaraki, Japan
| | - Hajime Mita
- Department of Life, Environment and Applied Chemistry, Faculty of Engineering, Fukuoka Institute of Technology, Fukuoka, Japan
| | - Shin-Ichi Yokobori
- School of Life Sciences, Tokyo University of Pharmacy and Life Sciences, Hachioji, Japan
| | - Akihiko Yamagishi
- School of Life Sciences, Tokyo University of Pharmacy and Life Sciences, Hachioji, Japan.,Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA), Sagamihara, Japan
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Milojevic T, Weckwerth W. Molecular Mechanisms of Microbial Survivability in Outer Space: A Systems Biology Approach. Front Microbiol 2020; 11:923. [PMID: 32499769 PMCID: PMC7242639 DOI: 10.3389/fmicb.2020.00923] [Citation(s) in RCA: 23] [Impact Index Per Article: 5.8] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 12/03/2019] [Accepted: 04/20/2020] [Indexed: 01/08/2023] Open
Abstract
Since the dawn of space exploration, the survivability of terrestrial life in outer space conditions has attracted enormous attention. Space technology has enabled the development of advanced space exposure facilities to investigate in situ responses of microbial life to the stress conditions of space during interplanetary transfer. Significant progress has been made toward the understanding of the effects of space environmental factors, e.g., microgravity, vacuum and radiation, on microorganisms exposed to real and simulated space conditions. Of extreme importance is not only knowledge of survival potential of space-exposed microorganisms, but also the determination of mechanisms of survival and adaptation of predominant species to the extreme space environment, i.e., revealing the molecular machinery, which elicit microbial survivability and adaptation. Advanced technologies in -omics research have permitted genome-scale studies of molecular alterations of space-exposed microorganisms. A variety of reports show that microorganisms grown in the space environment exhibited global alterations in metabolic functions and gene expression at the transcriptional and translational levels. Proteomic, metabolomic and especially metabolic modeling approaches as essential instruments of space microbiology, synthetic biology and metabolic engineering are rather underrepresented. Here we summarized the molecular space-induced alterations of exposed microorganisms in terms of understanding the molecular mechanisms of microbial survival and adaptation to drastic outer space environment.
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Affiliation(s)
- Tetyana Milojevic
- Extremophiles/Space Biochemistry Group, Department of Biophysical Chemistry, University of Vienna, Vienna, Austria
| | - Wolfram Weckwerth
- Department of Ecogenomics and Systems Biology, University of Vienna, Vienna, Austria
- Vienna Metabolomics Center, University of Vienna, Vienna, Austria
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de la Torre Noetzel R, Ortega García MV, Miller AZ, Bassy O, Granja C, Cubero B, Jordão L, Martínez Frías J, Rabbow E, Backhaus T, Ott S, García Sancho L, de Vera JPP. Lichen Vitality After a Space Flight on Board the EXPOSE-R2 Facility Outside the International Space Station: Results of the Biology and Mars Experiment. ASTROBIOLOGY 2020; 20:583-600. [PMID: 32364796 DOI: 10.1089/ast.2018.1959] [Citation(s) in RCA: 7] [Impact Index Per Article: 1.8] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/11/2023]
Abstract
As part of the Biology and Mars Experiment (BIOMEX; ILSRA 2009-0834), samples of the lichen Circinaria gyrosa were placed on the exposure platform EXPOSE-R2, on the International Space Station (ISS) and exposed to space and to a Mars-simulated environment for 18 months (2014-2016) to study: (1) resistance to space and Mars-like conditions and (2) biomarkers for use in future space missions (Exo-Mars). When the experiment returned (June 2016), initial analysis showed rapid recovery of photosystem II activity in the samples exposed exclusively to space vacuum and a Mars-like atmosphere. Significantly reduced recovery levels were observed in Sun-exposed samples, and electron and fluorescence microscopy (transmission electron microscope and field emission scanning electron microscope) data indicated that this was attributable to the combined effects of space radiation and space vacuum, as unirradiated samples exhibited less marked morphological changes compared with Sun-exposed samples. Polymerase chain reaction analyses confirmed that there was DNA damage in lichen exposed to harsh space and Mars-like environmental conditions, with ultraviolet radiation combined with space vacuum causing the most damage. These findings contribute to the characterization of space- and Mars-resistant organisms that are relevant to Mars habitability.
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Affiliation(s)
- Rosa de la Torre Noetzel
- Departamentos de Observación de la Tierra, Instituto Nacional de Técnica Aeroespacial (INTA), Madrid, Spain
| | - Maria Victoria Ortega García
- Departamentos de Sistemas de Defensa NBQ y Materiales Energéticos, Instituto Nacional de Técnica Aeroespacial (INTA), Madrid, Spain
| | - Ana Zélia Miller
- Instituto de Recursos Naturales y Agrobiología de Sevilla (IRNAS-CSIC), Sevilla, Spain
- HERCULES Laboratory, University of Évora, Évora, Portugal
| | - Olga Bassy
- ISDEFE (ISDEFE as External Consultant for INTA), Madrid, Spain
| | - Carmen Granja
- Departamentos de Sistemas de Defensa NBQ y Materiales Energéticos, Instituto Nacional de Técnica Aeroespacial (INTA), Madrid, Spain
| | - Beatriz Cubero
- Instituto de Recursos Naturales y Agrobiología de Sevilla (IRNAS-CSIC), Sevilla, Spain
| | - Luisa Jordão
- INSA-Instituto Nacional Saúde Doutor Ricardo Jorge, Lisboa, Portugal
| | | | - Elke Rabbow
- DLR-German Aerospace Center, Institute of Aerospace Medicine, Cologne, Germany
| | - Theresa Backhaus
- Institute of Botany, Heinrich-Heine-University Duesseldorf (HHU), Duesseldorf, Germany
| | - Sieglinde Ott
- Institute of Botany, Heinrich-Heine-University Duesseldorf (HHU), Duesseldorf, Germany
| | | | - Jean-Pierre Paul de Vera
- DLR-German Aerospace Center, Management and Infrastructure, Astrobiology Laboratories, Berlin, Germany
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Begyn K, Kim TD, Heyndrickx M, Michiels C, Aertsen A, Rajkovic A, Devlieghere F. Directed evolution by UV-C treatment of Bacillus cereus spores. Int J Food Microbiol 2019; 317:108424. [PMID: 31790956 DOI: 10.1016/j.ijfoodmicro.2019.108424] [Citation(s) in RCA: 8] [Impact Index Per Article: 1.6] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 05/13/2019] [Revised: 09/02/2019] [Accepted: 11/03/2019] [Indexed: 12/23/2022]
Abstract
Bacterial endospores are exposed to a broad variety of sublethal and lethal stresses in the food production chain. Generally, these stresses will not completely eliminate the existing spore populations, and thus constitute a selection pressure on the spores. One stress that is frequently used in the food production chains to disinfect (food) contact surfaces is UV-C. At a wavelength of 254 nm, UV-C has germicidal properties. The aim of this research is to investigate the impact of UV-C stress on the evolution of endospore recalcitrance and germination in B. cereus. A directed evolution experiment was set up in which B. cereus was repeatedly subjected to a cycle of sporulation, sporicidal UV-C treatment, germination and outgrowth. We show here that three independent lineages of UV-C cycled B. cereus spores reproducibly acquired a 30-fold or higher increase in UV-C resistance at 164 mJ/cm2. Surprisingly, the UV-C resistant spores of the clones isolated from each of the lineages also became significantly more sensitive to wet heat as a normally non-lethal heat treatment at 70 °C for 15 min resulted in an average 1.8 log cfu/mL reduction. From time-lapse phase contrast microscopy analysis, UV-C resistant mutant spores also showed a distinctive heterogeneity in refractility and a severe germination defect compared to the wild type. However, UV-C resistance of the corresponding vegetative cells was not altered. In conclusion, this work shows that UV-C resistance of endospores is an adaptive trait that can readily be improved, although at an apparent cost for heat resistance and germination efficiency. As such, these results provide novel insights in the evolvability of, and correlation between, some endospore properties.
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Affiliation(s)
- Katrien Begyn
- Research Unit Food Microbiology and Food Preservation (FMFP-UGent), Department of Food Technology, Safety and Health, Part of Food2Know, Faculty Bioscience Engineering, Ghent University, Ghent, Belgium
| | - Tom Dongmin Kim
- Laboratory of Food Microbiology, Department of Microbial and Molecular systems (M(2)S), Faculty of Bioscience Engineering, KU Leuven, Leuven, Belgium
| | - Marc Heyndrickx
- ILVO - Flanders Research Institute for Agriculture, Fisheries and Food, Technology and Food Science, Unit - Food Safety, Melle, Belgium; Department of Pathology, Bacteriology and Avian Diseases, Faculty of Veterinary Medicine, Ghent University, Merelbeke, Belgium
| | - Chris Michiels
- Laboratory of Food Microbiology, Department of Microbial and Molecular systems (M(2)S), Faculty of Bioscience Engineering, KU Leuven, Leuven, Belgium; Leuven Food Science and Nutrition Research Centre (LFoRCe), KU Leuven, Leuven, Belgium
| | - Abram Aertsen
- Laboratory of Food Microbiology, Department of Microbial and Molecular systems (M(2)S), Faculty of Bioscience Engineering, KU Leuven, Leuven, Belgium.
| | - Andreja Rajkovic
- Research Unit Food Microbiology and Food Preservation (FMFP-UGent), Department of Food Technology, Safety and Health, Part of Food2Know, Faculty Bioscience Engineering, Ghent University, Ghent, Belgium
| | - Frank Devlieghere
- Research Unit Food Microbiology and Food Preservation (FMFP-UGent), Department of Food Technology, Safety and Health, Part of Food2Know, Faculty Bioscience Engineering, Ghent University, Ghent, Belgium.
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Panitz C, Frösler J, Wingender J, Flemming HC, Rettberg P. Tolerances of Deinococcus geothermalis Biofilms and Planktonic Cells Exposed to Space and Simulated Martian Conditions in Low Earth Orbit for Almost Two Years. ASTROBIOLOGY 2019; 19:979-994. [PMID: 30925079 DOI: 10.1089/ast.2018.1913] [Citation(s) in RCA: 13] [Impact Index Per Article: 2.6] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/25/2023]
Abstract
Fossilized biofilms represent one of the oldest known confirmations of life on the Earth. The success of microbes in biofilms results from properties that are inherent in the biofilm, including enhanced interaction, protection, and biodiversity. Given the diversity of microbes that live in biofilms in harsh environments on the Earth, it is logical to hypothesize that, if microbes inhabit other bodies in the Universe, there are also biofilms on those bodies. The Biofilm Organisms Surfing Space experiment was conducted as part of the EXPOSE-R2 mission on the International Space Station. The experiment was an international collaboration designed to perform a comparative study regarding the survival of biofilms versus planktonic cells of various microorganisms, exposed to space and Mars-like conditions. The objective was to determine whether there are lifestyle-dependent differences to cope with the unique mixture of stress factors, including desiccation, temperature oscillations, vacuum, or a Mars-like gas atmosphere and pressure in combination with extraterrestrial or Mars-like ultraviolet (UV) radiation residing during the long-term space mission. In this study, the outcome of the flight and mission ground reference analysis of Deinococcus geothermalis is presented. Cultural tests demonstrated that D. geothermalis remained viable in the desiccated state, being able to survive space and Mars-like conditions and tolerating high extraterrestrial UV radiation for more than 2 years. Culturability decreased, but was better preserved, in the biofilm consortium than in planktonic cells. These results are correlated to differences in genomic integrity after exposure, as visualized by random amplified polymorphic DNA-polymerase chain reaction. Interestingly, cultivation-independent viability markers such as membrane integrity, ATP content, and intracellular esterase activity remained nearly unaffected, indicating that subpopulations of the cells had survived in a viable but nonculturable state. These findings support the hypothesis of long-term survival of microorganisms under the harsh environmental conditions in space and on Mars to a higher degree if exposed as biofilm.
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Affiliation(s)
- Corinna Panitz
- 1Institute of Pharmacology and Toxicology, University Hospital/RWTH Aachen, Aachen, Germany
| | - Jan Frösler
- 2Biofilm Centre, University of Duisburg-Essen, Essen, Germany
| | - Jost Wingender
- 2Biofilm Centre, University of Duisburg-Essen, Essen, Germany
| | | | - Petra Rettberg
- 3Research Group Astrobiology, Radiation Biology Department, Institute of Aerospace Medicine, Deutsches Zentrum für Luft- und Raumfahrt e.V. (DLR), Cologne, Germany
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Peyvan K, Karouia F, Cooper JJ, Chamberlain J, Suciu D, Slota M, Pohorille A. Gene Expression Measurement Module (GEMM) for space application: Design and validation. LIFE SCIENCES IN SPACE RESEARCH 2019; 22:55-67. [PMID: 31421849 DOI: 10.1016/j.lssr.2019.07.004] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/07/2019] [Revised: 07/05/2019] [Accepted: 07/07/2019] [Indexed: 06/10/2023]
Abstract
In order to facilitate studies on the impact of the space environment on biological systems, we have developed a prototype of GEMM (Gene Expression Measurement Module) - an automated, miniaturized, integrated fluidic system for in-situ measurements of gene expression in microbial samples. The GEMM instrument is capable of (1) lysing bacterial cell walls, (2) extracting and purifying RNA released from cells, (3) hybridizing the RNA to probes attached to a microarray and (4) providing electrochemical readout, all in a microfluidics cartridge. To function on small, uncrewed spacecraft, the conventional, laboratory protocols for both sample preparation and hybridization required significant modifications. Biological validation of the instrument was carried out on Synechococcus elongatus, a photosynthetic cyanobacterium known for its metabolic diversity and resilience to adverse conditions. It was demonstrated that GEMM yielded reliable, reproducible gene expression profiles. GEMM is the only high throughput instrument that can be deployed in near future on space platforms other than the ISS to advance biological research in space. It can also prove useful for numerous terrestrial applications in the field.
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Affiliation(s)
| | - Fathi Karouia
- University of California San Francisco, Department of Pharmaceutical Chemistry, San Francisco, CA 94158, USA; NASA Ames Research Center, Space Biosciences Research Branch, Moffett Field, CA 94035, USA; NASA Ames Research Center, Exobiology Branch, MS 239-4, Moffett Field, CA 94035, USA.
| | | | | | | | | | - Andrew Pohorille
- University of California San Francisco, Department of Pharmaceutical Chemistry, San Francisco, CA 94158, USA; NASA Ames Research Center, Exobiology Branch, MS 239-4, Moffett Field, CA 94035, USA.
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17
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de Vera JP, Alawi M, Backhaus T, Baqué M, Billi D, Böttger U, Berger T, Bohmeier M, Cockell C, Demets R, de la Torre Noetzel R, Edwards H, Elsaesser A, Fagliarone C, Fiedler A, Foing B, Foucher F, Fritz J, Hanke F, Herzog T, Horneck G, Hübers HW, Huwe B, Joshi J, Kozyrovska N, Kruchten M, Lasch P, Lee N, Leuko S, Leya T, Lorek A, Martínez-Frías J, Meessen J, Moritz S, Moeller R, Olsson-Francis K, Onofri S, Ott S, Pacelli C, Podolich O, Rabbow E, Reitz G, Rettberg P, Reva O, Rothschild L, Sancho LG, Schulze-Makuch D, Selbmann L, Serrano P, Szewzyk U, Verseux C, Wadsworth J, Wagner D, Westall F, Wolter D, Zucconi L. Limits of Life and the Habitability of Mars: The ESA Space Experiment BIOMEX on the ISS. ASTROBIOLOGY 2019; 19:145-157. [PMID: 30742496 PMCID: PMC6383581 DOI: 10.1089/ast.2018.1897] [Citation(s) in RCA: 55] [Impact Index Per Article: 11.0] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 04/29/2018] [Accepted: 01/07/2019] [Indexed: 06/01/2023]
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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Affiliation(s)
- Jean-Pierre de Vera
- German Aerospace Center (DLR), Institute of Planetary Research, Management and Infrastructure, Research Group Astrobiological Laboratories, Berlin, Germany
| | - Mashal Alawi
- GFZ, German Research Centre for Geosciences, Helmholtz Centre Potsdam, Section 5.3 Geomicrobiology, Telegrafenberg, Potsdam, Germany
| | - Theresa Backhaus
- Institut für Botanik, Heinrich-Heine-Universität (HHU), Düsseldorf, Germany
| | - Mickael Baqué
- German Aerospace Center (DLR), Institute of Planetary Research, Management and Infrastructure, Research Group Astrobiological Laboratories, Berlin, Germany
| | - Daniela Billi
- University of Rome Tor Vergata, Department of Biology, Rome, Italy
| | - Ute Böttger
- German Aerospace Center (DLR), Institute for Optical Sensor Systems, Berlin, Germany
| | - Thomas Berger
- German Aerospace Center (DLR), Institute of Aerospace Medicine, Radiation Biology Department, Köln, Germany
| | - Maria Bohmeier
- German Aerospace Center (DLR), Institute of Aerospace Medicine, Radiation Biology Department, Köln, Germany
| | - Charles Cockell
- School of Physics and Astronomy, University of Edinburgh, Edinburgh, UK
| | - René Demets
- European Space Research and Technology Centre (ESTEC), European Space Agency (ESA), Noordwijk, the Netherlands
| | - Rosa de la Torre Noetzel
- Departamento de Observación de la Tierra, Instituto Nacional de Técnica Aeroespacial (INTA), Madrid, Spain
| | - Howell Edwards
- Raman Spectroscopy Group, University Analytical Centre, Division of Chemical and Forensic Sciences, University of Bradford, West Yorkshire, UK
| | - Andreas Elsaesser
- Institut für experimentelle Physik, Experimentelle Molekulare Biophysik, Frei Universität Berlin, Berlin, Germany
| | | | - Annelie Fiedler
- University of Potsdam, Biodiversity Research/Systematic Botany, Potsdam, Germany
| | - Bernard Foing
- European Space Research and Technology Centre (ESTEC), European Space Agency (ESA), Noordwijk, the Netherlands
| | - Frédéric Foucher
- CNRS, Centre de Biophysique Moléculaire, UPR 4301, Orléans, France
| | - Jörg Fritz
- Museum für Naturkunde - Leibniz Institute for Evolution and Biodiversity Science, Berlin, Germany
| | - Franziska Hanke
- German Aerospace Center (DLR), Institute for Optical Sensor Systems, Berlin, Germany
| | - Thomas Herzog
- TH Wildau (Technical University of Applied Sciences), Wildau, Germany
| | - Gerda Horneck
- German Aerospace Center (DLR), Institute of Aerospace Medicine, Radiation Biology Department, Köln, Germany
| | - Heinz-Wilhelm Hübers
- German Aerospace Center (DLR), Institute for Optical Sensor Systems, Berlin, Germany
| | - Björn Huwe
- University of Potsdam, Biodiversity Research/Systematic Botany, Potsdam, Germany
| | - Jasmin Joshi
- University of Potsdam, Biodiversity Research/Systematic Botany, Potsdam, Germany
- Hochschule für Technik HSR Rapperswil, Institute for Landscape and Open Space, Rapperswil, Switzerland
| | | | - Martha Kruchten
- Institut für Botanik, Heinrich-Heine-Universität (HHU), Düsseldorf, Germany
| | - Peter Lasch
- Robert Koch Institute, Centre for Biological Threats and Special Pathogens, Berlin, Germany
| | - Natuschka Lee
- Department of Ecology and Environmental Sciences, Umeå University, Umeå, Sweden
| | - Stefan Leuko
- German Aerospace Center (DLR), Institute of Aerospace Medicine, Radiation Biology Department, Köln, Germany
| | - Thomas Leya
- Extremophile Research & Biobank CCCryo, Fraunhofer Institute for Cell Therapy and Immunology, Branch Bioanalytics and Bioprocesses (IZI-BB), Potsdam, Germany
| | - Andreas Lorek
- German Aerospace Center (DLR), Institute of Planetary Research, Management and Infrastructure, Research Group Astrobiological Laboratories, Berlin, Germany
| | | | - Joachim Meessen
- Institut für Botanik, Heinrich-Heine-Universität (HHU), Düsseldorf, Germany
| | - Sophie Moritz
- University of Potsdam, Biodiversity Research/Systematic Botany, Potsdam, Germany
| | - Ralf Moeller
- German Aerospace Center (DLR), Institute of Aerospace Medicine, Radiation Biology Department, Köln, Germany
| | - Karen Olsson-Francis
- School of Environment, Earth and Ecosystem Sciences, The Open University, Milton Keynes, UK
| | - Silvano Onofri
- Department of Ecological and Biological Sciences, University of Tuscia, Viterbo, Italy
| | - Sieglinde Ott
- Institut für Botanik, Heinrich-Heine-Universität (HHU), Düsseldorf, Germany
| | - Claudia Pacelli
- Department of Ecological and Biological Sciences, University of Tuscia, Viterbo, Italy
| | - Olga Podolich
- Institute of Molecular Biology & Genetics of NASU, Kyiv, Ukraine
| | - Elke Rabbow
- German Aerospace Center (DLR), Institute of Aerospace Medicine, Radiation Biology Department, Köln, Germany
| | - Günther Reitz
- German Aerospace Center (DLR), Institute of Aerospace Medicine, Radiation Biology Department, Köln, Germany
| | - Petra Rettberg
- German Aerospace Center (DLR), Institute of Aerospace Medicine, Radiation Biology Department, Köln, Germany
| | - Oleg Reva
- Centre for Bioinformatics and Computational Biology, Department of Biochemistry, Genetics and Microbiology, University of Pretoria, Pretoria, South Africa
| | | | | | | | - Laura Selbmann
- Department of Ecological and Biological Sciences, University of Tuscia, Viterbo, Italy
- Italian National Antarctic Museum (MNA), Mycological Section, Genoa, Italy
| | - Paloma Serrano
- GFZ, German Research Centre for Geosciences, Helmholtz Centre Potsdam, Section 5.3 Geomicrobiology, Telegrafenberg, Potsdam, Germany
- AWI, Alfred Wegener Institute, Helmholtz Centre for Polar and Marine Research, Potsdam, Germany
| | - Ulrich Szewzyk
- TU Berlin, Institute of Environmental Technology, Environmental Microbiology, Berlin, Germany
| | - Cyprien Verseux
- University of Rome Tor Vergata, Department of Biology, Rome, Italy
| | | | - Dirk Wagner
- GFZ, German Research Centre for Geosciences, Helmholtz Centre Potsdam, Section 5.3 Geomicrobiology, Telegrafenberg, Potsdam, Germany
- University of Potsdam, Institute of Earth and Environmental Sciences, Potsdam, Germany
| | - Frances Westall
- CNRS, Centre de Biophysique Moléculaire, UPR 4301, Orléans, France
| | - David Wolter
- German Aerospace Center (DLR), Institute of Planetary Research, Management and Infrastructure, Research Group Astrobiological Laboratories, Berlin, Germany
| | - Laura Zucconi
- Department of Ecological and Biological Sciences, University of Tuscia, Viterbo, Italy
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Experimental studies addressing the longevity of Bacillus subtilis spores - The first data from a 500-year experiment. PLoS One 2018; 13:e0208425. [PMID: 30513104 PMCID: PMC6279046 DOI: 10.1371/journal.pone.0208425] [Citation(s) in RCA: 40] [Impact Index Per Article: 6.7] [Reference Citation Analysis] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/27/2018] [Accepted: 11/17/2018] [Indexed: 11/23/2022] Open
Abstract
The ability to form endospores allows certain Gram-positive bacteria (e.g. Bacillus subtilis) to challenge the limits of microbial resistance and survival. Thus, B. subtilis is able to tolerate many environmental extremes by transitioning into a dormant state as spores, allowing survival under otherwise unfavorable conditions. Despite thorough study of spore resistance to external stresses, precisely how long B. subtilis spores can lie dormant while remaining viable, a period that potentially far exceeds the human lifespan; is not known although convincing examples of long term spore survival have been recorded. In this study, we report the first data from a 500-year microbial experiment, which started in 2014 and will finish in 2514. A set of vials containing a defined concentration of desiccated B. subtilis spores is opened and tested for viability every two years for the first 24 years and then every 25 years until experiment completion. Desiccated baseline spore samples were also exposed to environmental stresses, including X-rays, 254 nm UV-C, 10% H2O2, dry heat (120°C) and wet heat (100°C) to investigate how desiccated spores respond to harsh environmental conditions after long periods of storage. Data from the first 2 years of storage show no significant decrease in spore viability. Additionally, spores of B. subtilis were subjected to various short-term storage experiments, revealing that space-like vacuum and high NaCl concentration negatively affected spore viability.
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The DNA of Bacteria of the World Ocean and the Earth in Cosmic Dust at the International Space Station. ScientificWorldJournal 2018; 2018:7360147. [PMID: 29849510 PMCID: PMC5932454 DOI: 10.1155/2018/7360147] [Citation(s) in RCA: 16] [Impact Index Per Article: 2.7] [Reference Citation Analysis] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/03/2018] [Revised: 02/27/2018] [Accepted: 03/08/2018] [Indexed: 11/24/2022] Open
Abstract
Cosmic dust samples from the surface of the illuminator of the International Space Station (ISS) were collected by a crew member during his spacewalk. The sampler with tampon in a vacuum container was delivered to the Earth. Washouts from the tampon's material and the tampon itself were analyzed for the presence of bacterial DNA by the method of nested PCR with primers specific to DNA of the genus Mycobacteria, DNA of the strains of capsular bacteria Bacillus, and DNA encoding 16S ribosomal RNA. The results of amplification followed by sequencing and phylogenetic analysis indicated the presence of the bacteria of the genus Mycobacteria and the extreme bacterium of the genus Delftia in the samples of cosmic dust. It was shown that the DNA sequence of one of the bacteria of the genus Mycobacteria was genetically similar to that previously observed in superficial micro layer at the Barents and Kara seas' coastal zones. The presence of the wild land and marine bacteria DNA on the ISS suggests their possible transfer from the stratosphere into the ionosphere with the ascending branch of the global electric circuit. Alternatively, the wild land and marine bacteria as well as the ISS bacteria may all have an ultimate space origin.
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Olsson-Francis K, Ramkissoon NK, Price AB, Slade DJ, Macey MC, Pearson VK. The Study of Microbial Survival in Extraterrestrial Environments Using Low Earth Orbit and Ground-Based Experiments. J Microbiol Methods 2018. [DOI: 10.1016/bs.mim.2018.07.003] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 12/27/2022]
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Koskinen K, Rettberg P, Pukall R, Auerbach A, Wink L, Barczyk S, Perras A, Mahnert A, Margheritis D, Kminek G, Moissl-Eichinger C. Microbial biodiversity assessment of the European Space Agency's ExoMars 2016 mission. MICROBIOME 2017; 5:143. [PMID: 29070062 PMCID: PMC5657055 DOI: 10.1186/s40168-017-0358-3] [Citation(s) in RCA: 16] [Impact Index Per Article: 2.3] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 04/19/2017] [Accepted: 09/27/2017] [Indexed: 06/01/2023]
Abstract
BACKGROUND The ExoMars 2016 mission, consisting of the Trace Gas Orbiter and the Schiaparelli lander, was launched on March 14 2016 from Baikonur, Kazakhstan and reached its destination in October 2016. The Schiaparelli lander was subject to strict requirements for microbial cleanliness according to the obligatory planetary protection policy. To reach the required cleanliness, the ExoMars 2016 flight hardware was assembled in a newly built, biocontrolled cleanroom complex at Thales Alenia Space in Turin, Italy. In this study, we performed microbiological surveys of the cleanroom facilities and the spacecraft hardware before and during the assembly, integration and testing (AIT) activities. METHODS Besides the European Space Agency (ESA) standard bioburden assay, that served as a proxy for the microbiological contamination in general, we performed various alternative cultivation assays and utilised molecular techniques, including quantitative PCR and next generation sequencing, to assess the absolute and relative abundance and broadest diversity of microorganisms and their signatures in the cleanroom and on the spacecraft hardware. RESULTS Our results show that the bioburden, detected microbial contamination and microbial diversity decreased continuously after the cleanroom was decontaminated with more effective cleaning agents and during the ongoing AIT. The studied cleanrooms and change room were occupied by very distinct microbial communities: Overall, the change room harboured a higher number and diversity of microorganisms, including Propionibacterium, which was found to be significantly increased in the change room. In particular, the so called alternative cultivation assays proved important in detecting a broader cultivable diversity than covered by the standard bioburden assay and thus completed the picture on the cleanroom microbiota. CONCLUSION During the whole project, the bioburden stayed at acceptable level and did not raise any concern for the ExoMars 2016 mission. The cleanroom complex at Thales Alenia Space in Turin is an excellent example of how efficient microbiological control is performed.
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Affiliation(s)
- Kaisa Koskinen
- Department for Internal Medicine, Section of Infectious Diseases and Tropical Medicine, Medical University of Graz, Graz, Austria
- BioTechMed-Graz, Graz, Austria
| | - Petra Rettberg
- Radiation Biology Department, German Aerospace Center (DLR), Institute of Aerospace Medicine, Cologne, Germany
| | - Rüdiger Pukall
- Leibniz-Institute DSMZ - German Collection of Microorganisms and Cell Cultures, Braunschweig, Germany
| | - Anna Auerbach
- Department for Microbiology, University of Regensburg, Regensburg, Germany
| | - Lisa Wink
- Department for Internal Medicine, Section of Infectious Diseases and Tropical Medicine, Medical University of Graz, Graz, Austria
| | - Simon Barczyk
- Radiation Biology Department, German Aerospace Center (DLR), Institute of Aerospace Medicine, Cologne, Germany
| | - Alexandra Perras
- Department for Internal Medicine, Section of Infectious Diseases and Tropical Medicine, Medical University of Graz, Graz, Austria
- Department for Microbiology, University of Regensburg, Regensburg, Germany
| | - Alexander Mahnert
- Institute of Environmental Biotechnology, Graz University of Technology, Graz, Austria
| | | | | | - Christine Moissl-Eichinger
- Department for Internal Medicine, Section of Infectious Diseases and Tropical Medicine, Medical University of Graz, Graz, Austria
- BioTechMed-Graz, Graz, Austria
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22
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Beblo-Vranesevic K, Bohmeier M, Perras AK, Schwendner P, Rabbow E, Moissl-Eichinger C, Cockell CS, Pukall R, Vannier P, Marteinsson VT, Monaghan EP, Ehrenfreund P, Garcia-Descalzo L, Gómez F, Malki M, Amils R, Gaboyer F, Westall F, Cabezas P, Walter N, Rettberg P. The responses of an anaerobic microorganism, Yersinia intermedia MASE-LG-1 to individual and combined simulated Martian stresses. PLoS One 2017; 12:e0185178. [PMID: 29069099 PMCID: PMC5656303 DOI: 10.1371/journal.pone.0185178] [Citation(s) in RCA: 10] [Impact Index Per Article: 1.4] [Reference Citation Analysis] [Abstract] [MESH Headings] [Grants] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 03/03/2017] [Accepted: 09/07/2017] [Indexed: 11/18/2022] Open
Abstract
The limits of life of aerobic microorganisms are well understood, but the responses of anaerobic microorganisms to individual and combined extreme stressors are less well known. Motivated by an interest in understanding the survivability of anaerobic microorganisms under Martian conditions, we investigated the responses of a new isolate, Yersinia intermedia MASE-LG-1 to individual and combined stresses associated with the Martian surface. This organism belongs to an adaptable and persistent genus of anaerobic microorganisms found in many environments worldwide. The effects of desiccation, low pressure, ionizing radiation, varying temperature, osmotic pressure, and oxidizing chemical compounds were investigated. The strain showed a high tolerance to desiccation, with a decline of survivability by four orders of magnitude during a storage time of 85 days. Exposure to X-rays resulted in dose-dependent inactivation for exposure up to 600 Gy while applied doses above 750 Gy led to complete inactivation. The effects of the combination of desiccation and irradiation were additive and the survivability was influenced by the order in which they were imposed. Ionizing irradiation and subsequent desiccation was more deleterious than vice versa. By contrast, the presence of perchlorates was not found to significantly affect the survival of the Yersinia strain after ionizing radiation. These data show that the organism has the capacity to survive and grow in physical and chemical stresses, imposed individually or in combination that are associated with Martian environment. Eventually it lost its viability showing that many of the most adaptable anaerobic organisms on Earth would be killed on Mars today.
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Affiliation(s)
- Kristina Beblo-Vranesevic
- Radiation Biology Department, Institute of Aerospace Medicine, German Aerospace Center (DLR), Cologne, Germany
- * E-mail:
| | - Maria Bohmeier
- Radiation Biology Department, Institute of Aerospace Medicine, German Aerospace Center (DLR), Cologne, Germany
| | - Alexandra K. Perras
- Department of Internal Medicine, Medical University of Graz, Graz, Austria
- Department of Microbiology and Archaea, University of Regensburg, Regensburg, Germany
| | - Petra Schwendner
- School of Physics and Astronomy, UK Center for Astrobiology, University of Edinburgh, Edinburgh, United Kingdom
| | - Elke Rabbow
- Radiation Biology Department, Institute of Aerospace Medicine, German Aerospace Center (DLR), Cologne, Germany
| | - Christine Moissl-Eichinger
- Department of Internal Medicine, Medical University of Graz, Graz, Austria
- BioTechMed Graz, Graz, Austria
| | - Charles S. Cockell
- School of Physics and Astronomy, UK Center for Astrobiology, University of Edinburgh, Edinburgh, United Kingdom
| | - Rüdiger Pukall
- German Collection of Microorganisms and Cell Cultures, Leibniz Institute DSMZ, Braunschweig, Germany
| | | | - Viggo T. Marteinsson
- MATIS—Prokaria, Reykjavík, Iceland
- Faculty of Food Science and Nutrition, University of Iceland, Reykjavík, Iceland
| | | | - Pascale Ehrenfreund
- Leiden Observatory, Universiteit Leiden, Leiden, Netherland
- Space Policy Institute, George Washington University, Washington DC, United States of America
| | - Laura Garcia-Descalzo
- Instituto Nacional de Técnica Aeroespacial—Centro de Astrobiología (INTA-CAB), Madrid, Spain
| | - Felipe Gómez
- Instituto Nacional de Técnica Aeroespacial—Centro de Astrobiología (INTA-CAB), Madrid, Spain
| | | | | | - Frédéric Gaboyer
- Centre de Biophysique Moléculaire, Centre National de la Recherche Scientifique (CNRS), Orléans, France
| | - Frances Westall
- Centre de Biophysique Moléculaire, Centre National de la Recherche Scientifique (CNRS), Orléans, France
| | | | | | - Petra Rettberg
- Radiation Biology Department, Institute of Aerospace Medicine, German Aerospace Center (DLR), Cologne, Germany
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23
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Leuko S, Bohmeier M, Hanke F, Böettger U, Rabbow E, Parpart A, Rettberg P, de Vera JPP. On the Stability of Deinoxanthin Exposed to Mars Conditions during a Long-Term Space Mission and Implications for Biomarker Detection on Other Planets. Front Microbiol 2017; 8:1680. [PMID: 28966605 PMCID: PMC5605620 DOI: 10.3389/fmicb.2017.01680] [Citation(s) in RCA: 15] [Impact Index Per Article: 2.1] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 05/23/2017] [Accepted: 08/21/2017] [Indexed: 11/13/2022] Open
Abstract
Outer space, the final frontier, is a hostile and unforgiving place for any form of life as we know it. The unique environment of space allows for a close simulation of Mars surface conditions that cannot be simulated as accurately on the Earth. For this experiment, we tested the resistance of Deinococcus radiodurans to survive exposure to simulated Mars-like conditions in low-Earth orbit for a prolonged period of time as part of the Biology and Mars experiment (BIOMEX) project. Special focus was placed on the integrity of the carotenoid deinoxanthin, which may serve as a potential biomarker to search for remnants of life on other planets. Survival was investigated by evaluating colony forming units, damage inflicted to the 16S rRNA gene by quantitative PCR, and the integrity and detectability of deinoxanthin by Raman spectroscopy. Exposure to space conditions had a strong detrimental effect on the survival of the strains and the 16S rRNA integrity, yet results show that deinoxanthin survives exposure to conditions as they prevail on Mars. Solar radiation is not only strongly detrimental to the survival and 16S rRNA integrity but also to the Raman signal of deinoxanthin. Samples not exposed to solar radiation showed only minuscule signs of deterioration. To test whether deinoxanthin is able to withstand the tested parameters without the protection of the cell, it was extracted from cell homogenate and exposed to high/low temperatures, vacuum, germicidal UV-C radiation, and simulated solar radiation. Results obtained by Raman investigations showed a strong resistance of deinoxanthin against outer space and Mars conditions, with the only exception of the exposure to simulated solar radiation. Therefore, deinoxanthin proved to be a suitable easily detectable biomarker for the search of Earth-like organic pigment-containing life on other planets.
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Affiliation(s)
- Stefan Leuko
- German Aerospace Center, Research Group "Astrobiology", Radiation Biology Department, Institute of Aerospace MedicineKöln, Germany
| | - Maria Bohmeier
- German Aerospace Center, Research Group "Astrobiology", Radiation Biology Department, Institute of Aerospace MedicineKöln, Germany
| | - Franziska Hanke
- German Aerospace Center, Institute of Optical Sensor SystemsBerlin, Germany
| | - Ute Böettger
- German Aerospace Center, Institute of Optical Sensor SystemsBerlin, Germany
| | - Elke Rabbow
- German Aerospace Center, Research Group "Astrobiology", Radiation Biology Department, Institute of Aerospace MedicineKöln, Germany
| | - Andre Parpart
- German Aerospace Center, Research Group "Astrobiology", Radiation Biology Department, Institute of Aerospace MedicineKöln, Germany
| | - Petra Rettberg
- German Aerospace Center, Research Group "Astrobiology", Radiation Biology Department, Institute of Aerospace MedicineKöln, Germany
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Abstract
The endospore-forming bacteria have persisted on earth perhaps 3Ga, leveraging the flexibility of their distinctive lifestyle to adapt to a remarkably wide range of environments. This process of adaptation can be investigated through the simple but powerful technique of laboratory evolution. Evolved strains can be analyzed by whole genome sequencing and an array of omics technologies. The intensively studied, genetically tractable endospore-former, Bacillus subtilis, is an ideal subject for laboratory evolution experiments. Here, we describe the use of the B. subtilis model system to study the adaptation of these bacteria to reduced and stringent selection for endospore formation, as well as to novel environmental challenges of low atmospheric pressure, high ultraviolet radiation, and unfavourable growth temperatures. In combination with other approaches, including comparative genomics and environmental field work, laboratory evolution may help elucidate how these bacteria have so successfully adapted to life on earth, and perhaps beyond.
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Affiliation(s)
- Daniel R Zeigler
- Bacillus Genetic Stock Center, The Ohio State University, Columbus, OH, USA
| | - Wayne L Nicholson
- Department of Microbiology and Cell Science, University of Florida, Gainesville, FL, USA
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25
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Karouia F, Peyvan K, Pohorille A. Toward biotechnology in space: High-throughput instruments for in situ biological research beyond Earth. Biotechnol Adv 2017; 35:905-932. [PMID: 28433608 DOI: 10.1016/j.biotechadv.2017.04.003] [Citation(s) in RCA: 23] [Impact Index Per Article: 3.3] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/20/2016] [Revised: 03/27/2017] [Accepted: 04/12/2017] [Indexed: 12/18/2022]
Abstract
Space biotechnology is a nascent field aimed at applying tools of modern biology to advance our goals in space exploration. These advances rely on our ability to exploit in situ high throughput techniques for amplification and sequencing DNA, and measuring levels of RNA transcripts, proteins and metabolites in a cell. These techniques, collectively known as "omics" techniques have already revolutionized terrestrial biology. A number of on-going efforts are aimed at developing instruments to carry out "omics" research in space, in particular on board the International Space Station and small satellites. For space applications these instruments require substantial and creative reengineering that includes automation, miniaturization and ensuring that the device is resistant to conditions in space and works independently of the direction of the gravity vector. Different paths taken to meet these requirements for different "omics" instruments are the subjects of this review. The advantages and disadvantages of these instruments and technological solutions and their level of readiness for deployment in space are discussed. Considering that effects of space environments on terrestrial organisms appear to be global, it is argued that high throughput instruments are essential to advance (1) biomedical and physiological studies to control and reduce space-related stressors on living systems, (2) application of biology to life support and in situ resource utilization, (3) planetary protection, and (4) basic research about the limits on life in space. It is also argued that carrying out measurements in situ provides considerable advantages over the traditional space biology paradigm that relies on post-flight data analysis.
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Affiliation(s)
- Fathi Karouia
- University of California San Francisco, Department of Pharmaceutical Chemistry, San Francisco, CA 94158, USA; NASA Ames Research Center, Exobiology Branch, MS239-4, Moffett Field, CA 94035, USA; NASA Ames Research Center, Flight Systems Implementation Branch, Moffett Field, CA 94035, USA.
| | | | - Andrew Pohorille
- University of California San Francisco, Department of Pharmaceutical Chemistry, San Francisco, CA 94158, USA; NASA Ames Research Center, Exobiology Branch, MS239-4, Moffett Field, CA 94035, USA.
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26
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Moissl-Eichinger C, Cockell C, Rettberg P. Venturing into new realms? Microorganisms in space. FEMS Microbiol Rev 2016; 40:722-37. [PMID: 27354346 DOI: 10.1093/femsre/fuw015] [Citation(s) in RCA: 59] [Impact Index Per Article: 7.4] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Accepted: 05/23/2016] [Indexed: 12/15/2022] Open
Abstract
One of the biggest challenges of science is the determination of whether extraterrestrial life exists. Although potential habitable areas might be available for complex life, it is more likely that microbial life could exist in space. Many extremotolerant and extremophilic microbes have been found to be able to withstand numerous, combined environmental factors, such as high or low temperatures and pressures, high-salt conditions, high doses of radiation, desiccation or nutrient limitations. They may even survive the transit from one planet to another. Terrestrial Mars-analogue sites are one focus of researchers, in order to understand the microbial diversity in preparation for upcoming space missions aimed at the detection of life. However, such missions could also pose a risk with respect to contamination of the extraterrestrial environment by accidentally transferred terrestrial microorganisms. Closer to the Earth, the International Space Station is the most enclosed habitat, where humans work and live-and with them numerous microorganisms. It is still unknown how microbes adapt to this environment, possibly even creating a risk for the crew. Information on the microbiology of the ISS will have an impact on the planning and implementation of long-term human spaceflights in order to ensure a safe, stable and balanced microbiome on board.
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Affiliation(s)
- Christine Moissl-Eichinger
- Department for Internal Medicine, Medical University of Graz, 8036 Graz, Austria BioTechMed Graz, 8010 Graz, Austria
| | - Charles Cockell
- UK Centre for Astrobiology, School of Physics and Astronomy, University of Edinburgh, Edinburgh EH10 4EP, UK
| | - Petra Rettberg
- Radiation Biology Department, Institute of Aerospace Medicine, German Aerospace Center (DLR), 51147 Cologne, Germany
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27
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Horneck G, Walter N, Westall F, Grenfell JL, Martin WF, Gomez F, Leuko S, Lee N, Onofri S, Tsiganis K, Saladino R, Pilat-Lohinger E, Palomba E, Harrison J, Rull F, Muller C, Strazzulla G, Brucato JR, Rettberg P, Capria MT. AstRoMap European Astrobiology Roadmap. ASTROBIOLOGY 2016; 16:201-43. [PMID: 27003862 PMCID: PMC4834528 DOI: 10.1089/ast.2015.1441] [Citation(s) in RCA: 42] [Impact Index Per Article: 5.3] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 12/01/2015] [Accepted: 01/27/2016] [Indexed: 05/07/2023]
Abstract
The European AstRoMap project (supported by the European Commission Seventh Framework Programme) surveyed the state of the art of astrobiology in Europe and beyond and produced the first European roadmap for astrobiology research. In the context of this roadmap, astrobiology is understood as the study of the origin, evolution, and distribution of life in the context of cosmic evolution; this includes habitability in the Solar System and beyond. The AstRoMap Roadmap identifies five research topics, specifies several key scientific objectives for each topic, and suggests ways to achieve all the objectives. The five AstRoMap Research Topics are • Research Topic 1: Origin and Evolution of Planetary Systems • Research Topic 2: Origins of Organic Compounds in Space • Research Topic 3: Rock-Water-Carbon Interactions, Organic Synthesis on Earth, and Steps to Life • Research Topic 4: Life and Habitability • Research Topic 5: Biosignatures as Facilitating Life Detection It is strongly recommended that steps be taken towards the definition and implementation of a European Astrobiology Platform (or Institute) to streamline and optimize the scientific return by using a coordinated infrastructure and funding system.
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Affiliation(s)
- Gerda Horneck
- European Astrobiology Network Association
- Institute of Aerospace Medicine, German Aerospace Center (DLR), Köln, Germany
| | | | - Frances Westall
- Centre National de la Recherche Scientifique–Centre de Biophysique Moléculaire, Orleans, France
| | - John Lee Grenfell
- Institute for Planetary Research, German Aerospace Center (DLR), Berlin, Germany
| | - William F. Martin
- Institute of Molecular Evolution, Heinrich-Heine University of Düsseldorf, Düsseldorf, Germany
| | - Felipe Gomez
- INTA Centre for Astrobiology, Torrejón de Ardoz, Madrid, Spain
| | - Stefan Leuko
- Institute of Aerospace Medicine, German Aerospace Center (DLR), Köln, Germany
| | - Natuschka Lee
- Department of Ecology and Environmental Science, Umeå University, Umeå, Sweden
- Department of Microbiology, Technical University München, München, Germany
| | - Silvano Onofri
- Department of Ecological and Biological Sciences, University of Tuscia, Viterbo, Italy
| | - Kleomenis Tsiganis
- Department of Physics, Section of Astrophysics, Astronomy and Mechanics, Aristotle University of Thessaloniki, Thessaloniki, Greece
| | - Raffaele Saladino
- Department of Agrobiology and Agrochemistry, University of Tuscia, Viterbo, Italy
| | | | - Ernesto Palomba
- INAF–Institute for Space Astrophysics and Planetology, Rome, Italy
| | - Jesse Harrison
- Department of Microbiology and Ecosystem Science, University of Vienna, Vienna, Austria
| | - Fernando Rull
- Department of Condensed Matter Physics, Crystallography and Mineralogy, Valladolid University, Valladolid, Spain
| | | | | | | | - Petra Rettberg
- Institute of Aerospace Medicine, German Aerospace Center (DLR), Köln, Germany
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28
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Onofri S, de Vera JP, Zucconi L, Selbmann L, Scalzi G, Venkateswaran KJ, Rabbow E, de la Torre R, Horneck G. Survival of Antarctic Cryptoendolithic Fungi in Simulated Martian Conditions On Board the International Space Station. ASTROBIOLOGY 2015; 15:1052-9. [PMID: 26684504 DOI: 10.1089/ast.2015.1324] [Citation(s) in RCA: 45] [Impact Index Per Article: 5.0] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/27/2023]
Abstract
UNLABELLED Dehydrated Antarctic cryptoendolithic communities and colonies of the rock inhabitant black fungi Cryomyces antarcticus (CCFEE 515) and Cryomyces minteri (CCFEE 5187) were exposed as part of the Lichens and Fungi Experiment (LIFE) for 18 months in the European Space Agency's EXPOSE-E facility to simulated martian conditions aboard the International Space Station (ISS). Upon sample retrieval, survival was proved by testing colony-forming ability, and viability of cells (as integrity of cell membrane) was determined by the propidium monoazide (PMA) assay coupled with quantitative PCR tests. Although less than 10% of the samples exposed to simulated martian conditions were able to proliferate and form colonies, the PMA assay indicated that more than 60% of the cells and rock communities had remained intact after the "Mars exposure." Furthermore, a high stability of the DNA in the cells was demonstrated. The results contribute to assessing the stability of resistant microorganisms and biosignatures on the surface of Mars, data that are valuable information for further search-for-life experiments on Mars. KEY WORDS Endoliths-Eukaryotes-Extremophilic microorganisms-Mars-Radiation resistance.
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Affiliation(s)
- Silvano Onofri
- 1 Department of Ecological and Biological Sciences, University of Tuscia , Viterbo, Italy
| | - Jean-Pierre de Vera
- 2 Institute of Planetary Research, German Aerospace Center (DLR) , Berlin, Germany
| | - Laura Zucconi
- 1 Department of Ecological and Biological Sciences, University of Tuscia , Viterbo, Italy
| | - Laura Selbmann
- 1 Department of Ecological and Biological Sciences, University of Tuscia , Viterbo, Italy
| | - Giuliano Scalzi
- 1 Department of Ecological and Biological Sciences, University of Tuscia , Viterbo, Italy
| | | | - Elke Rabbow
- 4 Institute of Aerospace Medicine, German Aerospace Center (DLR) , Cologne, Germany
| | - Rosa de la Torre
- 5 Department of Earth Observation, Spanish Aerospace Research Establishment-INTA , Torrejón de Ardoz, Madrid, Spain
| | - Gerda Horneck
- 4 Institute of Aerospace Medicine, German Aerospace Center (DLR) , Cologne, Germany
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Omairi T, Wainwright M. Fluorescent minerals--A potential source of UV protection and visible light for the growth of green algae and cyanobacteria in extreme cosmic environments. LIFE SCIENCES IN SPACE RESEARCH 2015; 6:87-91. [PMID: 26256632 DOI: 10.1016/j.lssr.2015.07.004] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 03/30/2015] [Revised: 07/03/2015] [Accepted: 07/06/2015] [Indexed: 06/04/2023]
Abstract
We propose that green algae (Chlorella variabilis and Dunaliella tertiolecta) and cyanobacteria (Synechococcus elongatus and Nostoc commune) can grow inside fluorescent rock minerals which convert damaging UV light to visible light, thereby allowing these organisms to survive and thrive in UV-rich environments without (or with limited) visible light, which would otherwise be inimical to them. The four microorganisms were incubated inside fluorescent rocks composed of fluorite, calcite and pyrite. The resultant growth was then measured following exposure to UV radiation, with the use of optical density and measurement of chlorophyll concentration. Results show that the microorganisms were shielded from harmful UV in these semi-transparent rocks, while at the same time benefiting from the fact that the minerals converted UV to visible light; this have been shown by a statistically significant increase in their growth, which although lower than when the cells were incubated in sunlight, was significantly higher than in controls incubated in the dark.
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Affiliation(s)
- Tareq Omairi
- Department of Molecular Biology and Biotechnology, University of Sheffield, Sheffield S10 2TN, UK.
| | - Milton Wainwright
- Department of Molecular Biology and Biotechnology, University of Sheffield, Sheffield S10 2TN, UK
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30
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Thiel CS, Tauber S, Schütte A, Schmitz B, Nuesse H, Moeller R, Ullrich O. Functional activity of plasmid DNA after entry into the atmosphere of earth investigated by a new biomarker stability assay for ballistic spaceflight experiments. PLoS One 2014; 9:e112979. [PMID: 25426925 PMCID: PMC4245111 DOI: 10.1371/journal.pone.0112979] [Citation(s) in RCA: 10] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 09/04/2014] [Accepted: 10/17/2014] [Indexed: 11/18/2022] Open
Abstract
Sounding rockets represent an excellent platform for testing the influence of space conditions during the passage of Earth's atmosphere and re-entry on biological, physical and chemical experiments for astrobiological purposes. We designed a robust functionality biomarker assay to analyze the biological effects of suborbital spaceflights prevailing during ballistic rocket flights. During the TEXUS-49 rocket mission in March 2011, artificial plasmid DNA carrying a fluorescent marker (enhanced green fluorescent protein: EGFP) and an antibiotic resistance cassette (kanamycin/neomycin) was attached on different positions of rocket exterior; (i) circular every 90 degree on the outer surface concentrical of the payload, (ii) in the grooves of screw heads located in between the surface application sites, and (iii) on the surface of the bottom side of the payload. Temperature measurements showed two major peaks at 118 and 130°C during the 780 seconds lasting flight on the inside of the recovery module, while outer gas temperatures of more than 1000°C were estimated on the sample application locations. Directly after retrieval and return transport of the payload, the plasmid DNA samples were recovered. Subsequent analyses showed that DNA could be recovered from all application sites with a maximum of 53% in the grooves of the screw heads. We could further show that up to 35% of DNA retained its full biological function, i.e., mediating antibiotic resistance in bacteria and fluorescent marker expression in eukariotic cells. These experiments show that our plasmid DNA biomarker assay is suitable to characterize the environmental conditions affecting DNA during an atmospheric transit and the re-entry and constitute the first report of the stability of DNA during hypervelocity atmospheric transit indicating that sounding rocket flights can be used to model the high-speed atmospheric entry of organics-laden artificial meteorites.
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Affiliation(s)
- Cora S. Thiel
- Institute of Anatomy, Faculty of Medicine, University of Zurich, Zurich, Switzerland
- * E-mail: (CT); (OU)
| | - Svantje Tauber
- Institute of Anatomy, Faculty of Medicine, University of Zurich, Zurich, Switzerland
- Department of Machine Design, Engineering Design and Product Development, Institute of Mechanical Engineering, Otto-von-Guericke-University Magdeburg, Magdeburg, Germany
| | | | | | - Harald Nuesse
- Institute of Medical Physics and Biophysics, University of Muenster, Münster, Germany
| | - Ralf Moeller
- German Aerospace Center (DLR e.V.), Institute of Aerospace Medicine, Radiation Biology Department, Research Group Astrobiology, Linder Hoehe, Cologne (Köln), Germany
| | - Oliver Ullrich
- Institute of Anatomy, Faculty of Medicine, University of Zurich, Zurich, Switzerland
- Department of Machine Design, Engineering Design and Product Development, Institute of Mechanical Engineering, Otto-von-Guericke-University Magdeburg, Magdeburg, Germany
- Zurich Center for Integrative Human Physiology (ZIHP), University of Zurich, Zurich, Switzerland
- * E-mail: (CT); (OU)
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31
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Pratt SN, Austin DE. Bacterial spores survive electrospray charging and desolvation. JOURNAL OF THE AMERICAN SOCIETY FOR MASS SPECTROMETRY 2014; 25:712-721. [PMID: 24566985 DOI: 10.1007/s13361-014-0827-x] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 06/05/2013] [Revised: 01/03/2014] [Accepted: 01/03/2014] [Indexed: 06/03/2023]
Abstract
The survivability of Bacillus subtilis spores and vegetative Escherichia coli cells after electrospray from aqueous suspension was tested using mobility experiments at atmospheric pressure. E. coli did not survive electrospray charging and desolvation, but B. subtilis did. Experimental conditions ensured that any surviving bacteria were de-agglomerated, desolvated, and electrically charged. Based on mobility measurements, B. subtilis spores survived even with 2,000-20,000 positive charges. B. subtilis was also found to survive introduction into vacuum after either positive or negative electrospray. Attempts to measure the charge distribution of viable B. subtilis spores using electrostatic deflection in vacuum were inconclusive; however, viable spores with low charge states (less than 42 positive or less than 26 negative charges) were observed.
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Affiliation(s)
- Sara N Pratt
- Department of Chemistry and Biochemistry, Brigham Young University, Provo, UT, 84602, USA
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32
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Yang W, Han L, Mandlaa M, Chen H, Jiang M, Zhang Z, Xu H. Spaceflight-induced enhancement of 2-keto-L-gulonic acid production by a mixed culture of Ketogulonigenium vulgare
and Bacillus thuringiensis. Lett Appl Microbiol 2013; 57:54-62. [DOI: 10.1111/lam.12083] [Citation(s) in RCA: 9] [Impact Index Per Article: 0.8] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 12/02/2012] [Revised: 03/17/2013] [Accepted: 04/01/2013] [Indexed: 11/28/2022]
Affiliation(s)
- W. Yang
- Institute of Applied Ecology; Chinese Academy of Sciences; Shenyang China
- University of Chinese Academy of Sciences; Beijing China
| | - L. Han
- Fermentation & Biotechnology Laboratory; Northeast Pharmaceutical Group Co. Ltd.; Shenyang China
| | - M. Mandlaa
- Institute of Applied Ecology; Chinese Academy of Sciences; Shenyang China
- University of Chinese Academy of Sciences; Beijing China
| | - H. Chen
- Fermentation & Biotechnology Laboratory; Northeast Pharmaceutical Group Co. Ltd.; Shenyang China
| | - M. Jiang
- Fermentation & Biotechnology Laboratory; Northeast Pharmaceutical Group Co. Ltd.; Shenyang China
| | - Z. Zhang
- Institute of Applied Ecology; Chinese Academy of Sciences; Shenyang China
| | - H. Xu
- Institute of Applied Ecology; Chinese Academy of Sciences; Shenyang China
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Westall F. Microbial Scale Habitability on Mars. HABITABILITY OF OTHER PLANETS AND SATELLITES 2013. [DOI: 10.1007/978-94-007-6546-7_11] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 01/28/2023]
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Rabbow E, Rettberg P, Barczyk S, Bohmeier M, Parpart A, Panitz C, Horneck G, von Heise-Rotenburg R, Hoppenbrouwers T, Willnecker R, Baglioni P, Demets R, Dettmann J, Reitz G. EXPOSE-E: an ESA astrobiology mission 1.5 years in space. ASTROBIOLOGY 2012; 12:374-86. [PMID: 22680684 DOI: 10.1089/ast.2011.0760] [Citation(s) in RCA: 29] [Impact Index Per Article: 2.4] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 05/20/2023]
Abstract
The multi-user facility EXPOSE-E was designed by the European Space Agency to enable astrobiology research in space (low-Earth orbit). On 7 February 2008, EXPOSE-E was carried to the International Space Station (ISS) on the European Technology Exposure Facility (EuTEF) platform in the cargo bay of Space Shuttle STS-122 Atlantis. The facility was installed at the starboard cone of the Columbus module by extravehicular activity, where it remained in space for 1.5 years. EXPOSE-E was returned to Earth with STS-128 Discovery on 12 September 2009 for subsequent sample analysis. EXPOSE-E provided accommodation in three exposure trays for a variety of astrobiological test samples that were exposed to selected space conditions: either to space vacuum, solar electromagnetic radiation at >110 nm and cosmic radiation (trays 1 and 3) or to simulated martian surface conditions (tray 2). Data on UV radiation, cosmic radiation, and temperature were measured every 10 s and downlinked by telemetry. A parallel mission ground reference (MGR) experiment was performed on ground with a parallel set of hardware and samples under simulated space conditions. EXPOSE-E performed a successful 1.5-year mission in space.
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Affiliation(s)
- Elke Rabbow
- Radiation Biology Department, Institute of Aerospace Medicine, German Aerospace Center (DLR) , Cologne, Germany.
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