EGU2020-22228
https://doi.org/10.5194/egusphere-egu2020-22228
EGU General Assembly 2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

The ExoMars Trace Gas Orbiter – First Martian Year in Orbit

Håkan Svedhem1, Oleg Korablev2, Igor Mitrofanov2, Daniel Rodionov2, Nicholas Thomas3, AnnCarine Vandaele4, Jorge L. Vago1, Francois Forget5, and Colin Wilson6
Håkan Svedhem et al.
  • 1ESA/ESTEC, Noordwijk, The Netherlands (hsvedhem@cosmos.esa.int)
  • 2Space Research Institute, IKI, Moscow, Russia
  • 3University of Bern, Bern, Switzerland
  • 4BIRA/BISA, Brussels, Belgium
  • 5LMD, Paris, France
  • 6University of Oxford, Oxford, UK

The Trace Gas Orbiter, TGO, has in March 2020 concluded its first Martian year in its 400km, 74 degrees inclination, science orbit. It has been a highly successful year, starting with the rise, plateau and decay of the major Global Dust Storm in the summer of 2018. This has enabled interesting results to be derived on the water vapour distribution, dynamic behaviour and upward transport as a consequence of the dust storm. The characterisation of the minor species and trace gasses is continuing and a large number of profiles is produced every day. A dedicated search of methane has shown that there is no methane above an altitude of a few km, with an upper limit established at about 20 ppt (2∙10-11). The solar occultation technique used by the spectrometers has definitely proven its strength, both for its high sensitivity and for its capability of making high resolution altitude profiles of the atmosphere. Climatological studies have been initiated and will become more important now that a full year has passed, even if the full potential will be visible only after a few Martian years of operation. The FREND instrument has characterised the hydrogen in the shallow sub-surface on a global scale at a spatial resolution much better than previous missions have been able. It has found areas at surprisingly low latitudes with significant amounts of sub-surface hydrogen, most likely in the form of water ice. The CaSSIS camera has made a high number of images over a large variety of targets, including the landing sites of the 2020 ESA and NASA rovers, Oxia Planum and the Jezero Crater. Stereo imaging has enabled topographic information and precise 3-D landscape synthesis.

This presentation will summarise the highlights of the first Martian year and discuss planned activities for the near and medium term future.

The ExoMars programme is a joint activity by the European Space Agency (ESA) and ROSCOSMOS, Russia. It consists of the ExoMars 2016 mission, launched 14 March 2016, with the Trace Gas Orbiter, TGO, and the Entry Descent and Landing Demonstrator, EDM, named Schiaparelli, and the ExoMars 2020 mission, to be launched in July/August 2020, carrying a Rover and a surface science platform to the surface of Mars.

How to cite: Svedhem, H., Korablev, O., Mitrofanov, I., Rodionov, D., Thomas, N., Vandaele, A., Vago, J. L., Forget, F., and Wilson, C.: The ExoMars Trace Gas Orbiter – First Martian Year in Orbit, EGU General Assembly 2020, Online, 4–8 May 2020, EGU2020-22228, https://doi.org/10.5194/egusphere-egu2020-22228, 2020