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Atmospheric Science with InSight

Spiga, Aymeric and Banfield, Don and Teanby, Nicholas A. and Forget, François and Lucas, Antoine and Kenda, Balthasar and Rodriguez Manfredi, Jose Antonio and Widmer-Schnidrig, Rudolf and Murdoch, Naomi and Lemmon, Mark T. and Garcia, Raphaël F. and Martire, Léo and Karatekin, Özgür and Le Maistre, Sébastien and Van Hove, Bart and Dehant, Véronique and Lognonné, Philippe and Mueller, Nils and Lorenz, Ralph and Mimoun, David and Rodriguez, Sébastien and Beucler, Éric and Daubar, Ingrid and Golombek, Matthew P. and Bertrand, Tanguy and Nishikawa, Yasuhiro and Millour, Ehouarn and Rolland, Lucie and Brissaud, Quentin and Kawamura, Taichi and Mocquet, Antoine and Martin, Roland and Clinton, John and Stutzmann, Éléonore and Spohn, Tilman and Smrekar, Suzanne and Banerdt, William B. Atmospheric Science with InSight. (2018) Space Science Reviews, 214 (109). 1-64. ISSN 0038-6308

(Document in English)

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Official URL: https://doi.org/10.1007/s11214-018-0543-0


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.

Item Type:Article
HAL Id:hal-01902145
Audience (journal):International peer-reviewed journal
Uncontrolled Keywords:
Institution:Université de Toulouse > Institut Supérieur de l'Aéronautique et de l'Espace - ISAE-SUPAERO (FRANCE)
Laboratory name:
Deposited By: Naomi Murdoch
Deposited On:23 Oct 2018 12:43

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