Skip to Main content Skip to Navigation

Investigations of the Mars Upper Atmosphere with ExoMars Trace Gas Orbiter

Miguel Lopez-Valverde 1 Jean-Claude Gérard 2 Francisco González-Galindo 1 Ann-Carine Vandaele 3 Ian Thomas 3 Oleg Korablev 4 Nikolai Ignatiev 4 Anna Fedorova 4 Franck Montmessin 5 Anni Määttänen 5 Sabrina Guilbon 5 Franck Lefèvre 5 Manish R. Patel 6 Sergio Jiménez-Monferrer Maya García-Comas 1 Alejandro Cardesin 7 Colin F. Wilson 8 R. T. Clancy 9 Armin Kleinböhl 10 Daniel J. Mccleese 10 David M. Kass 10 Nick M. Schneider 11 Michael S. Chaffin 11 Josè Juan Lopez-Moreno 1 Julio Rodríguez 1
1 IAA - Instituto de Astrofísica de Andalucía
2 LPAP - Laboratoire de Physique Atmosphérique et Planétaire
3 BIRA-IASB - Belgian Institute for Space Aeronomy / Institut d'Aéronomie Spatiale de Belgique
4 IKI - Space Research Institute of the Russian Academy of Sciences
5 IMPEC - LATMOS
LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales
6 School of Physical Sciences [Milton Keynes]
7 ESAC - European Space Astronomy Centre
8 Department of Physics [Oxford]
9 SSI - Space Science Institute [Boulder]
10 JPL - Jet Propulsion Laboratory
11 LASP - Laboratory for Atmospheric and Space Physics [Boulder]
Abstract : The Martian mesosphere and thermosphere, the region above about 60 km, is not the primary target of the ExoMars 2016 mission but its Trace Gas Orbiter (TGO) can explore it and address many interesting issues, either in-situ during the aerobraking period or remotely during the regular mission. In the aerobraking phase TGO peeks into thermospheric densities and temperatures, in a broad range of latitudes and during a long continuous period. TGO carries two instruments designed for the detection of trace species, NOMAD and ACS, which will use the solar occultation technique. Their regular sounding at the terminator up to very high altitudes in many different molecular bands will represent the first time that an extensive and precise dataset of densities and hopefully temperatures are obtained at those altitudes and local times on Mars. But there are additional capabilities in TGO for studying the upper atmosphere of Mars, and we review them briefly. Our simulations suggest that airglow emissions from the UV to the IR might be observed outside the terminator. If eventually confirmed from orbit, they would supply new information about atmospheric dynamics and variability. However, their optimal exploitation requires a special spacecraft pointing, currently not considered in the regular operations but feasible in our opinion. We discuss the synergy between the TGO instruments, specially the wide spectral range achieved by combining them. We also encourage coordinated operations with other Mars-observing missions capable of supplying simultaneous measurements of its upper atmosphere.
Keywords : Mars ExoMars NOMAD ACS Upper atmosphere Aerobraking Airglow Remote sounding
Document type :
Journal articles
Complete list of metadatas
https://hal-insu.archives-ouvertes.fr/insu-01681392
Contributor : Catherine Cardon <>
Submitted on : Thursday, January 11, 2018 - 4:12:15 PM
Last modification on : Friday, January 10, 2020 - 3:42:35 PM

Links full text

openaccess

Identifiers

Collections

INSU | CNRS | UVSQ | UNIV-PARIS-SACLAY | SORBONNE-UNIVERSITE | LATMOS | UPMC | SU-SCIENCES

Citation

Miguel Lopez-Valverde, Jean-Claude Gérard, Francisco González-Galindo, Ann-Carine Vandaele, Ian Thomas, et al.. Investigations of the Mars Upper Atmosphere with ExoMars Trace Gas Orbiter. Space Science Reviews, Springer Verlag, 2018, 214 (1), pp.artcle 29. ⟨10.1007/s11214-017-0463-4⟩. ⟨insu-01681392⟩

Export

BibTeX TEI DC DCterms EndNote

Share

Metrics

Record views

464

Contact

Informations

CCSD