Space Science Reviews

, 214:109 | Cite as

Atmospheric Science with InSight

  • Aymeric Spiga
  • Don Banfield
  • Nicholas A. Teanby
  • François Forget
  • Antoine Lucas
  • Balthasar Kenda
  • Jose Antonio Rodriguez Manfredi
  • Rudolf Widmer-Schnidrig
  • Naomi Murdoch
  • Mark T. Lemmon
  • Raphaël F. Garcia
  • Léo Martire
  • Özgür Karatekin
  • Sébastien Le Maistre
  • Bart Van Hove
  • Véronique Dehant
  • Philippe Lognonné
  • Nils Mueller
  • Ralph Lorenz
  • David Mimoun
  • Sébastien Rodriguez
  • Éric Beucler
  • Ingrid Daubar
  • Matthew P. Golombek
  • Tanguy Bertrand
  • Yasuhiro Nishikawa
  • Ehouarn Millour
  • Lucie Rolland
  • Quentin Brissaud
  • Taichi Kawamura
  • Antoine Mocquet
  • Roland Martin
  • John Clinton
  • Éléonore Stutzmann
  • Tilman Spohn
  • Suzanne Smrekar
  • William B. Banerdt
Part of the following topical collections:
  1. The InSight Mission to Mars II


In November 2018, for the first time a dedicated geophysical station, the InSight lander, will be deployed on the surface of Mars. Along with the two main geophysical packages, the Seismic Experiment for Interior Structure (SEIS) and the Heat-Flow and Physical Properties Package (HP3), the InSight lander holds a highly sensitive pressure sensor (PS) and the Temperature and Winds for InSight (TWINS) instrument, both of which (along with the InSight FluxGate (IFG) Magnetometer) form the Auxiliary Sensor Payload Suite (APSS). Associated with the RADiometer (RAD) instrument which will measure the surface brightness temperature, and the Instrument Deployment Camera (IDC) which will be used to quantify atmospheric opacity, this will make InSight capable to act as a meteorological station at the surface of Mars. While probing the internal structure of Mars is the primary scientific goal of the mission, atmospheric science remains a key science objective for InSight. InSight has the potential to provide a more continuous and higher-frequency record of pressure, air temperature and winds at the surface of Mars than previous in situ missions. In the paper, key results from multiscale meteorological modeling, from Global Climate Models to Large-Eddy Simulations, are described as a reference for future studies based on the InSight measurements during operations. We summarize the capabilities of InSight for atmospheric observations, from profiling during Entry, Descent and Landing to surface measurements (pressure, temperature, winds, angular momentum), and the plans for how InSight’s sensors will be used during operations, as well as possible synergies with orbital observations. In a dedicated section, we describe the seismic impact of atmospheric phenomena (from the point of view of both “noise” to be decorrelated from the seismic signal and “signal” to provide information on atmospheric processes). We discuss in this framework Planetary Boundary Layer turbulence, with a focus on convective vortices and dust devils, gravity waves (with idealized modeling), and large-scale circulations. Our paper also presents possible new, exploratory, studies with the InSight instrumentation: surface layer scaling and exploration of the Monin-Obukhov model, aeolian surface changes and saltation / lifing studies, and monitoring of secular pressure changes. The InSight mission will be instrumental in broadening the knowledge of the Martian atmosphere, with a unique set of measurements from the surface of Mars.


Mars InSight Atmospheric science Planetary atmospheres 



Bertrand, Forget, Garcia, Kenda, Lognonné, Millour, Mimoun, Murdoch, Spiga acknowledge financial support from Centre National d’Études Spatiales (CNES). Spiga acknowledges computing support from Institut du développement et des ressources en informatique scientifique (IDRIS). Banfield, Lemmon, Lorenz acknowledge financial support from National Aeronautics and Space Administration (NASA). Banerdt, Daubar, Golombek, Mueller, Smrekar acknowledge that a portion of this research was carried out at the Jet Propulsion Laboratory (JPL), California Institute of Technology, under a contract with the National Aeronautics and Space Administration (NASA). Teanby is supported by the UK Space Agency. Karatekin, Le Maistre, Van Hove, Dehant are financially supported by the Belgian PRODEX program managed by the European Space Agency (ESA), in collaboration with the Belgian Federal Science Policy Office. Kenda, Lognonné, Lucas, Rodriguez acknowledge financial support from the UnivEarthS LabEx program of Sorbonne Paris Cite (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02). Rodriguez and Lucas acknowledge financial support from the French National Research Agency (ANR-APOSTIC-11-BS56-002 and ANR-12-BS05-001-3/EXO-DUNES). Forget and Spiga thank Luca Montabone and Mike Wolff from Space Science Institute for providing unpublished data: respectively dust opacity for MY33 and MRO/MARCI cloud opacity estimates. This paper was written with the collaborative tools Overleaf and Git. We acknowledge two anonymous reviewers for thorough and constructive comments which helped us to improve the paper.


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Copyright information

© Springer Nature B.V. 2018

Authors and Affiliations

  • Aymeric Spiga
    • 12
    • 9
  • Don Banfield
    • 2
  • Nicholas A. Teanby
    • 17
  • François Forget
    • 9
  • Antoine Lucas
    • 10
  • Balthasar Kenda
    • 10
  • Jose Antonio Rodriguez Manfredi
    • 14
  • Rudolf Widmer-Schnidrig
    • 18
  • Naomi Murdoch
    • 6
  • Mark T. Lemmon
    • 11
  • Raphaël F. Garcia
    • 6
  • Léo Martire
    • 6
  • Özgür Karatekin
    • 8
  • Sébastien Le Maistre
    • 8
  • Bart Van Hove
    • 8
  • Véronique Dehant
    • 8
  • Philippe Lognonné
    • 10
    • 12
  • Nils Mueller
    • 1
    • 16
  • Ralph Lorenz
    • 13
  • David Mimoun
    • 6
  • Sébastien Rodriguez
    • 10
    • 12
  • Éric Beucler
    • 4
  • Ingrid Daubar
    • 1
  • Matthew P. Golombek
    • 1
  • Tanguy Bertrand
    • 3
  • Yasuhiro Nishikawa
    • 10
  • Ehouarn Millour
    • 9
  • Lucie Rolland
    • 15
  • Quentin Brissaud
    • 5
  • Taichi Kawamura
    • 10
  • Antoine Mocquet
    • 4
  • Roland Martin
    • 19
  • John Clinton
    • 7
  • Éléonore Stutzmann
    • 10
  • Tilman Spohn
    • 16
  • Suzanne Smrekar
    • 1
  • William B. Banerdt
    • 1
  1. 1.Jet Propulsion LaboratoryCalifornia Institute of TechnologyPasadenaUSA
  2. 2.Cornell Center for Astrophysics and Planetary ScienceCornell UniversityIthacaUSA
  3. 3.NASA Ames Research CenterMountain ViewUSA
  4. 4.Laboratoire de Planétologie et GéodynamiqueUniversité de NantesNantesFrance
  5. 5.Division of Geological and Planetary SciencesCalifornia Institute of TechnologyPasadenaUSA
  6. 6.Institut Supérieur de l’Aéronautique et de l’Espace (ISAE-SUPAERO)Université de ToulouseToulouseFrance
  7. 7.ETHZurichSwitzerland
  8. 8.Royal Observatory of BelgiumBrusselsBelgium
  9. 9.Laboratoire de Météorologie Dynamique (LMD/IPSL)Sorbonne Université, Centre National de la Recherche Scientifique, École Polytechnique, École Normale SupérieureParisFrance
  10. 10.Institut de Physique du Globe de ParisUniversité Paris DiderotParisFrance
  11. 11.Texas A&M universityCollege StationUSA
  12. 12.Institut Universitaire de FranceParisFrance
  13. 13.Applied Physics LaboratoryJohns Hopkins UniversityLaurelUSA
  14. 14.CABMadridSpain
  15. 15.Geoazur, Université Côte d’AzurObservatoire de la Côte d’AzurNiceFrance
  16. 16.DLR, German Aerospace CenterInstitute of Planetary ResearchBerlinGermany
  17. 17.School of Earth SciencesUniversity of BristolBristolUK
  18. 18.Institut für GeophysikUniversität StuttgartStuttgartGermany
  19. 19.Géoscience Environnement Toulouse, Observatoire midi-PyrénéesUniversité de ToulouseToulouseFrance

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