دورية أكاديمية

No detection of methane on Mars from early ExoMars Trace Gas Orbiter observations

التفاصيل البيبلوغرافية
العنوان: No detection of methane on Mars from early ExoMars Trace Gas Orbiter observations
المؤلفون: Korablev, Oleg, Vandaele, Ann Carine, Montmessin, Franck, Fedorova, Anna A., Trokhimovskiy, Alexander, Forget, François, Lefèvre, Franck, Daerden, Frank, Thomas, Ian R., Trompet, Loic, Erwin, Justin T., Aoki, Shohei, Robert, Séverine, Neary, Lori, Viscardy, Sébastien, Grigoriev, Alexey V., Ignatiev, Nikolay I., Shakun, Alexey, Patrakeev, Andrey, Belyaev, Denis A., Bertaux, Jean-Loup, Olsen, Kevin, Baggio, Lucio, Alday, Juan, Ivanov, Yuriy S., Ristic, Bojan, Mason, Jon, Willame, Yannick, Depiesse, Cédric, Hetey, Laszlo, Berkenbosch, Sophie, Clairquin, Roland, Queirolo, Claudio, Beeckman, Bram, Neefs, Eddy, Patel, Manish R., Bellucci, Giancarlo, López-Moreno, José-Juan, Wilson, Colin F., Etiope, Giuseppe, Zelenyi, Lev, Svedhem, Håkan, Vago, Jorge L., Alonso-Rodrigo, Gustavo, Altieri, Francesca, Anufreychik, Konstantin, Arnold, Gabriele E., Bauduin, Sophie, Bolsée, David, Carrozzo, Giacomo, Clancy, R. Todd, Cloutis, Edward A., Crismani, Matteo, da Pieve, Fabiana, d'Aversa, Emiliano, Duxbury, Natalia, Encrenaz, Thérèse, Fouchet, Thierry, Funke, Bernd, Fussen, Didier, Garcia-Comas, Maia, Gérard, Jean-Claude, Giuranna, Marco, Gkouvelis, Leo, Gonzalez-Galindo, Francisco, Grassi, Davide, Guerlet, Sandrine, Hartogh, Paul, Holmes, James A., Hubert, Benoît, Kaminski, Jacek W., Karatekin, Özgür, Kasaba, Yasumasa, Kass, David, Khatuntsev, Igor, Kleinböhl, Armin, Kokonkov, Nikita, Krasnopolsky, Vladimir, Kuzmin, Ruslan, Lacombe, Gaetan, Lanciano, Orietta, Lellouch, Emmanuel, Lewis, Stephen, Luginin, Mikhail, Liuzzi, Giuliano, López-Puertas, Manuel, Lopez-Valverde, Miguel, Määttänen, Anni, Mahieux, Arnaud, Marcq, Emmanuel, Martin-Torres, Javier, Maslov, Igor, Medvedev, Alexander, Millour, Ehouarn, Moshkin, Boris, Mumma, Michael J., Nakagawa, Hiromu, Novak, Robert E., Oliva, Fabrizio, Patsaev, Dmitry, Piccialli, Arianna, Quantin-Nataf, Cathy, Renotte, Etienne, Ritter, Birgit, Rodin, Alexander, Schmidt, Frédéric, Schneider, Nick, Shematovich, Valery, Smith, Michael D., Teanby, Nicholas A., Thiemann, Ed, Thomas, Nicolas, Vander Auwera, Jean, Vázquez, Luis, Villanueva, Geronimo, Vincendon, Matthieu, Whiteway, James, Wilquet, Valérie, Wolff, Michael J., Wolkenberg, Paulina, Yelle, Roger, Young, Roland, Zasova, Ludmila, Paz Zorzano, Maria
المساهمون: Space Research Institute of the Russian Academy of Sciences (IKI), Russian Academy of Sciences Moscow (RAS), Belgian Institute for Space Aeronomy / Institut d'Aéronomie Spatiale de Belgique (BIRA-IASB), PLANETO - LATMOS, Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS), Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Météorologie Dynamique (UMR 8539) (LMD), Institut national des sciences de l'Univers (INSU - CNRS)-École polytechnique (X)-École des Ponts ParisTech (ENPC)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Département des Géosciences - ENS Paris, École normale supérieure - Paris (ENS-PSL), Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-École normale supérieure - Paris (ENS-PSL), Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL), Department of Physics Oxford, University of Oxford, Main Astronomical Observatory of NAS of Ukraine (MAO), National Academy of Sciences of Ukraine = Національна академія наук України = Académie nationale des sciences d'Ukraine (NASU / НАН України), School of Physical Sciences Milton Keynes, Faculty of Science, Technology, Engineering and Mathematics Milton Keynes, The Open University Milton Keynes (OU)-The Open University Milton Keynes (OU), Istituto di Astrofisica e Planetologia Spaziali - INAF (IAPS), Istituto Nazionale di Astrofisica (INAF), Instituto de Astrofísica de Andalucía (IAA), Consejo Superior de Investigaciones Cientificas España = Spanish National Research Council Spain (CSIC), Istituto Nazionale di Geofisica e Vulcanologia - Sezione di Roma (INGV), Istituto Nazionale di Geofisica e Vulcanologia, Faculty of Environmental Science and Engineering Cluj-Napoca, Babes-Bolyai University Cluj-Napoca (UBB), European Space Research and Technology Centre (ESTEC), Agence Spatiale Européenne = European Space Agency (ESA), Instituto Universitario de Microgravedad "Ignacio Da Riva" (IDR), Universidad Politécnica de Madrid (UPM), DLR Institut für Planetenforschung, Deutsches Zentrum für Luft- und Raumfahrt Berlin (DLR), Spectroscopie de l'atmosphère, Service de Chimie Quantique et Photophysique, Université libre de Bruxelles (ULB), Space Science Institute Boulder (SSI), Department of Geography Winnipeg, University of Winnipeg, NASA Goddard Space Flight Center (GSFC), Lomonosov Moscow State University (MSU), Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Atmosphérique et Planétaire (LPAP), Université de Liège, Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research (MPS), Max-Planck-Gesellschaft, Institute of Geophysics Warsaw, Polska Akademia Nauk = Polish Academy of Sciences = Académie polonaise des sciences (PAN), Royal Observatory of Belgium = Observatoire Royal de Belgique (ROB), Graduate School of Information Sciences Sendai, Tohoku University Sendai, Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), Institute for Astrophysics and Computational Sciences Washington, Catholic University of America, Agenzia Spaziale Italiana (ASI), Department of Computer Science, Electrical and Space Engineering Luleå, Luleå University of Technology = Luleå Tekniska Universitet (LUT), Laboratoire de Géologie de Lyon - Terre, Planètes, Environnement (LGL-TPE), École normale supérieure de Lyon (ENS de Lyon)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut national des sciences de l'Univers (INSU - CNRS)-Université Jean Monnet - Saint-Étienne (UJM)-Centre National de la Recherche Scientifique (CNRS), Advanced Mechanical and Optical Systems SA (AMOS), Moscow Institute of Physics and Technology Moscow (MIPT), Géosciences Paris Sud (GEOPS), Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS), Laboratory for Atmospheric and Space Physics Boulder (LASP), University of Colorado Boulder, Institute of Astronomy of the Russian Academy of Sciences (INASAN), School of Earth Sciences Bristol, University of Bristol Bristol, Universität Bern / University of Bern (UNIBE), Universidad Complutense de Madrid = Complutense University of Madrid Madrid (UCM), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales Paris (CNES), Centre for Research in Earth and Space Science Toronto (CRESS), York University Toronto, Lunar and Planetary Laboratory Tucson (LPL), University of Arizona
المصدر: ISSN: 0028-0836.
بيانات النشر: HAL CCSD
Nature Publishing Group
سنة النشر: 2019
المجموعة: Université de Versailles Saint-Quentin-en-Yvelines: HAL-UVSQ
مصطلحات موضوعية: [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]
الوصف: International audience ; The detection of methane on Mars has been interpreted as indicating that geochemical or biotic activities could persist on Mars today1. A number of different measurements of methane show evidence of transient, locally elevated methane concentrations and seasonal variations in background methane concentrations2,3,4,5. These measurements, however, are difficult to reconcile with our current understanding of the chemistry and physics of the Martian atmosphere6,7, which—given methane’s lifetime of several centuries—predicts an even, well mixed distribution of methane1,6,8. Here we report highly sensitive measurements of the atmosphere of Mars in an attempt to detect methane, using the ACS and NOMAD instruments onboard the ESA-Roscosmos ExoMars Trace Gas Orbiter from April to August 2018. We did not detect any methane over a range of latitudes in both hemispheres, obtaining an upper limit for methane of about 0.05 parts per billion by volume, which is 10 to 100 times lower than previously reported positive detections2,4. We suggest that reconciliation between the present findings and the background methane concentrations found in the Gale crater4 would require an unknown process that can rapidly remove or sequester methane from the lower atmosphere before it spreads globally.
نوع الوثيقة: article in journal/newspaper
اللغة: English
العلاقة: insu-02099757; https://insu.hal.science/insu-02099757Test; https://insu.hal.science/insu-02099757/documentTest; https://insu.hal.science/insu-02099757/file/2019%2520Korablev%2520TGO%2520methane%2520Nature_accepted-3.pdfTest
DOI: 10.1038/s41586-019-1096-4
الإتاحة: https://doi.org/10.1038/s41586-019-1096-4Test
https://insu.hal.science/insu-02099757Test
https://insu.hal.science/insu-02099757/documentTest
https://insu.hal.science/insu-02099757/file/2019%2520Korablev%2520TGO%2520methane%2520Nature_accepted-3.pdfTest
حقوق: info:eu-repo/semantics/OpenAccess
رقم الانضمام: edsbas.A6FB2B32
قاعدة البيانات: BASE