Stringent upper limit of CH 4 on Mars based on SOFIA/EXES observations

Discovery of CH 4 in the Martian atmosphere has led to much discussion since it could be a signature of biological and/or geological activities on Mars. However, the presence of CH 4 and its temporal and spatial variations are still under discussion because of the large uncertainties embedded in the...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2018-02, Vol.610, p.A78
Hauptverfasser:	Aoki, S., Richter, M.J., DeWitt, C., Boogert, A., Encrenaz, T., Sagawa, H., Nakagawa, H., Vandaele, A. C., Giuranna, M., Greathouse, T. K., Fouchet, T., Geminale, A., Sindoni, G., McKelvey, M., Case, M., Kasaba, Y.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Physics Sciences of the Universe
Online-Zugang:	Volltext
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