The radioscience LaRa instrument onboard ExoMars 2020 to investigate the rotation and interior of Mars
Veronique Dehant, Sebastien Le Maistre, Rose-Marie Baland, Nicolas, Bergeot, Ozgur Karatekin, Marie-Julie Peters, Attilio Rivoldini, Luca Ruiz, Lozano, Orkun Temel, Tim Van Hoolst, Marie Yseboodt, Michel Mitrovic,, Alexander Kosov, Vaclav Valenta, Lieven Thomassen, Sumit Karki

TL;DR
The LaRa instrument on ExoMars 2020 aims to precisely measure Mars' rotation and interior structure using radio Doppler shift data, enhancing understanding of Mars' geophysical properties.
Contribution
This paper details the design, setup, and expected scientific outcomes of the LaRa experiment, including its capabilities to analyze Mars' interior and rotational dynamics.
Findings
Expected improvement in Mars' rotation parameter measurements
Potential to reveal Mars' interior structure and atmosphere
Methodology for determining surface platform position
Abstract
LaRa (Lander Radioscience) is an experiment on the ExoMars 2020 mission that uses the Doppler shift on the radio link due to the motion of the ExoMars platform tied to the surface of Mars with respect to the Earth ground stations (e.g. the deep space network stations of NASA), in order to precisely measure the relative velocity of the lander on Mars with respect to the Earth. The LaRa measurements shall improve the understanding of the structure and processes in the deep interior of Mars by obtaining the rotation and orientation of Mars with a better precision compared to the previous missions. In this paper, we provide the analysis done until now for the best realization of these objectives. We explain the geophysical observation that will be reached with LaRa (Length-of-day variations, precession, nutation, and possibly polar motion). We develop the experiment set up, which includes…
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