The radioscience LaRa instrument onboard ExoMars 2020 to investigate the rotation and interior of mars. (January 2020)

• Record Type: Journal Article
• Authors: Dehant, Véronique; Le Maistre, Sébastien; Baland, Rose-Marie; Bergeot, Nicolas; Karatekin, Özgür; Péters, Marie-Julie; Rivoldini, Attilio; Ruiz Lozano, Luca; Temel, Orkun; Van Hoolst, Tim; Yseboodt, Marie; Mitrovic, Michel; Kosov, Alexander S.; Valenta, Vaclav; Thomassen, Lieven; Karki, Sumit; Al Khalifeh, Khaldoun; Craeye, Christophe; Gurvits, Leonid I.; Marty, Jean-Charles; Asmar, Sami W.; Folkner, William M.
• Is Part Of: Planetary and space science. Volume 180(2020)
• Publication Date: 2020-01
• Subjects: Space sciences -- Periodicals; Atmosphere, Upper -- Periodicals; Sciences spatiales -- Périodiques; Haute atmosphère -- Périodiques; 523
• DOI: 10.1016/j.pss.2019.104776
• Languages: English
• ISSNs: 0032-0633

Abstract

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 the ground stations on Earth (so-called ground segment). We describe the instrument, i.e. the transponder and its three antennas. We further detail the link budget and the expected noise level that will be reached. Finally, we detail the expected results, which encompasses the explanation of how we shall determine Mars' orientation parameters, and the way we shall deduce Mars' interior structure and Mars' atmosphere from them. Lastly, we explain briefly how we will be able to determine the Surface platform position. Highlights: Presentation and detailed description of the LaRa experiment, a scientific payload of the ExoMars 2020 surface platform. LaRa radio-science experiment X-band coherent transponder on ExoMars 2020 measure Mars' rotation and the core properties. LaRa will measure Mars' rotation and orientation with unprecedented accuracy. LaRa will constrain the physical state, dimension, and density of the Martian core. LaRa will constrain the global mass exchange between the planet and its atmosphere.