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

Korablev, Oleg; Vandaele, Ann Carine; Montmessin, Franck; Fedorova, Anna A; Trokhimovskiy, Alexander; Forget, François; Lefèvre, Franck; Daerden, Frank; Thomas, Ian R; Trompet, Loïc; 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 S; Baggio, Lucio; Alday, Juan; Ivanov, Yuriy S; Ristic, Bojan; Mason, Jonathon; Willame, Yannick; Depiesse, Cédric; Hetey, Laszlo; Berkenbosch, Sophie; Clairquin, Roland; Queirolo, Claudio; Beeckman, Bram; Neefs, Eddy; Patel, Manish R; Bellucci, Giancarlo; López-Moreno, Jose-Juan; Wilson, Colin F; Etiope, Giuseppe; Zelenyi, Lev; Svedhem, Håkan and Vago, Jorge L (2019). No detection of methane on Mars from early ExoMars Trace Gas Orbiter observations. Nature, 568 pp. 517–520.

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DOI (Digital Object Identifier) Link: https://doi.org/10.1038/s41586-019-1096-4
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Abstract

The detection of methane on Mars has been interpreted as indicating that geochemical or biotic activities could persist on Mars today. A number of different measurements of methane show evidence of transient, locally elevated methane concentrations and seasonal variations in background methane concentrations. These measurements, however, are difficult to reconcile with our current understanding of the chemistry and physics of the Martian atmosphere, which-given methane's lifetime of several centuries-predicts an even, well mixed distribution of methane. 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 detections. We suggest that reconciliation between the present findings and the background methane concentrations found in the Gale crater would require an unknown process that can rapidly remove or sequester methane from the lower atmosphere before it spreads globally.

Item Type: Journal Item
Copyright Holders: 2019 The Author(s), under exclusive licence to Springer Nature Limited
ISSN: 1476-4687
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Item ID: 60547
SWORD Depositor: Jisc Publications-Router
Depositing User: Jisc Publications-Router
Date Deposited: 30 Apr 2019 09:23
Last Modified: 14 May 2019 03:53
URI: http://oro.open.ac.uk/id/eprint/60547
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