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Assessment of a 2016 mission concept: The search for trace gases in the atmosphere of Mars
Authors:Richard W Zurek  Augustin Chicarro  Mark A Allen  Jean-Loup Bertaux  RTodd Clancy  Frank Daerden  Vittorio Formisano  James B Garvin  Gerhard Neukum  Michael D Smith
Institution:1. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA;2. European Space Agency, ESTEC, 2200 AG Noordwijk, The Netherlands;3. CNRS Service d’Aeronomie du CNRS, Verrières-le-Buisson, France;4. Space Science Institute, 4750 Walnut St., Suite 205, Boulder, CO 80301, USA;5. Belgian Institute for Space Aeronomy, Ringlaan 3, B-1180 Brussels, Belgium;6. IFSI Roma, Italy;7. Goddard Space Flight Center, Greenbelt, MD 20771, USA;8. Freie Universitaet Berlin, Malteserstr. 74-100, D-12249 Berlin, Germany;1. Research and Scientific Support Dept., ESA/ESTEC, Noordwijk, Netherlands;2. Arkansas Center for Space and Planetary Sciences, University of Arkansas, Fayetteville, AR 72701;3. Space Physics Research Laboratory, University of Michigan, Ann Arbor, MI 48109-2143, USA;4. Department of Physics, University of California, Berkeley, CA94720, USA;1. Laboratory of Theoretical Spectroscopy, V.E. Zuev Institute of Atmospheric Optics SB RAS, 1, Academician Zuev square, Tomsk 634021, Russia;2. National Research Tomsk State University, pr. Lenina 36, Tomsk 634050 Russia;3. Service de Chimie Quantique et Photophysique, Université Libre de Bruxelles, C.P. 160/09, 50 Avenue F. D. Roosevelt, B-1050 Brussels, Belgium;4. Univ. Grenoble Alpes, LIPhy, F-38000 Grenoble, France;5. CNRS, LIPhy, F-38000 Grenoble, France;1. Laboratory of Theoretical Spectroscopy, V.E. Zuev Institute of Atmospheric Optics SB RAS 1, Akademician Zuev Square, 634021 Tomsk, Russia;2. Physical Department of Tomsk State University, 36, Lenin Ave., 634050 Tomsk, Russia;1. Institute of Physics, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University in Torun, Grudziadzka 5, 87-100 Torun, Poland;2. Instituto de Estructura de la Materia, IEM-CSIC, Serrano 123, 28006 Madrid, Spain;3. National Institute of Standards and Technology, 100 Bureau Drive, Gaithersburg, MD 20899, USA;4. Laboratoire Interuniversitaire des Systèmes Atmosphériques, UMR CNRS 7583, Université Paris Est Créteil (UPEC), Université Paris Diderot (UPD), Institut Pierre-Simon Laplace, 94010 Créteil Cedex, France;1. Laboratory of Theoretical Spectroscopy, V.E. Zuev Institute of Atmospheric Optics, SB RAS, 1, Academician Zuev square, 634021 Tomsk, Russia;2. Groupe de Spectrométrie Moléculaire et Atmosphérique, UMR CNRS 7331, Université de Reims, U.F.R. Sciences, B.P. 1039, 51687 Reims Cedex 2, France;3. Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA;4. Tomsk State University, 36 Lenin Avenue, 634050 Tomsk, Russia
Abstract:The reported detection of methane in the atmosphere of Mars as well as its potentially large seasonal spatial variations challenge our understanding of both the sources and sinks of atmospheric trace gases. The presence of methane suggests ongoing exchange between the subsurface and the atmosphere of potentially biogenic trace gases, while the spatial and temporal variations cannot be accounted for with current knowledge of martian photochemistry. A Joint Instrument Definition Team (JIDT) was asked to assess concepts for a mission that might follow up on these discoveries within the framework of a series of joint missions being considered by ESA and NASA for possible future exploration of Mars. The following is based on the report of the JIDT to the space agencies (Zurek et al., 2009); a synopsis of the report was presented at the Workshop on Mars Methane held in Frascati, Italy, in November 2009. To summarize, the JIDT believed that a scientifically exciting and credible mission could be conducted within the evolving capabilities of the science/telecommunications orbiter being considered by ESA and NASA for possible launch in the 2016 opportunity for Mars.
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