The ESA’s JUICE mission will provide a thorough investigation of the Jupiter system and the Galilean moons during its nominal tour, comprising flybys of Europa and Callisto, and an orbital phase about Ganymede at the end of the mission. The 3GM experiment will exploit accurate Doppler and range measurements to determine the moons’ orbits and gravity fields (both static and tidal) and infer their interior structure. This paper presents the attainable accuracies of the Callisto geodesy experiment and addresses the effect of different flybys mean anomaly distribution and geometry on the estimation of the tidal Love number k2.

Analysis of 3GM Callisto gravity experiment of the JUICE mission / DI BENEDETTO, Mauro; Cappuccio, Paolo; Molli, Serena; Federici, Lorenzo; Zavoli, Alessandro. - 175:(2020), pp. 4965-4977. (Intervento presentato al convegno AAS/AIAA Astrodynamics Specialist Conference 2020 tenutosi a Virtual Event).

Analysis of 3GM Callisto gravity experiment of the JUICE mission

Mauro Di Benedetto
;
Paolo Cappuccio;Serena Molli;Lorenzo Federici;Alessandro Zavoli
2020

Abstract

The ESA’s JUICE mission will provide a thorough investigation of the Jupiter system and the Galilean moons during its nominal tour, comprising flybys of Europa and Callisto, and an orbital phase about Ganymede at the end of the mission. The 3GM experiment will exploit accurate Doppler and range measurements to determine the moons’ orbits and gravity fields (both static and tidal) and infer their interior structure. This paper presents the attainable accuracies of the Callisto geodesy experiment and addresses the effect of different flybys mean anomaly distribution and geometry on the estimation of the tidal Love number k2.
2020
AAS/AIAA Astrodynamics Specialist Conference 2020
spaceflight; trajectory; radio science
04 Pubblicazione in atti di convegno::04b Atto di convegno in volume
Analysis of 3GM Callisto gravity experiment of the JUICE mission / DI BENEDETTO, Mauro; Cappuccio, Paolo; Molli, Serena; Federici, Lorenzo; Zavoli, Alessandro. - 175:(2020), pp. 4965-4977. (Intervento presentato al convegno AAS/AIAA Astrodynamics Specialist Conference 2020 tenutosi a Virtual Event).
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/1563349
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