In 2016 the spacecraft Juno completed its first three perijove passes, respectively on Aug. 27 (PJ-1), Oct. 19 (PJ-2), and Dec. 11 (PJ-3), at an altitude of about 4000 km above the cloud level. Measurements of the spacecraft range rate were carried out across closest approach in all three passes, thanks to a coherent, two-way tracking at X band (7.2-8.4 GHz) from the antennas of the Deep Space Network. In PJ-1 a second downlink frequency at Ka band (32.5 GHz) allowed a good calibration of the path delay variations due to the Io plasma torus. During PJ-3, dedicated to radio science and Jupiter gravity determination, the full onboard Ka band system was activated, enabling a coherent radio link at 32.5-34 GHz and high accuracy range rate measurements. After removal of media effects (earth troposphere and Io plasma torus), tracking data from all three passes were combined to obtain a first cut determination of Jupiter gravity field. We report on this preliminary solution, and compare it with the theoretical expectations available in the literature.

The gravity field of Jupiter after the first three orbits of Juno

TORTORA, PAOLO;ZANNONI, MARCO;
2017

Abstract

In 2016 the spacecraft Juno completed its first three perijove passes, respectively on Aug. 27 (PJ-1), Oct. 19 (PJ-2), and Dec. 11 (PJ-3), at an altitude of about 4000 km above the cloud level. Measurements of the spacecraft range rate were carried out across closest approach in all three passes, thanks to a coherent, two-way tracking at X band (7.2-8.4 GHz) from the antennas of the Deep Space Network. In PJ-1 a second downlink frequency at Ka band (32.5 GHz) allowed a good calibration of the path delay variations due to the Io plasma torus. During PJ-3, dedicated to radio science and Jupiter gravity determination, the full onboard Ka band system was activated, enabling a coherent radio link at 32.5-34 GHz and high accuracy range rate measurements. After removal of media effects (earth troposphere and Io plasma torus), tracking data from all three passes were combined to obtain a first cut determination of Jupiter gravity field. We report on this preliminary solution, and compare it with the theoretical expectations available in the literature.
2017
Geophysical Research Abstracts
1
1
Iess, Luciano; Buccino, Dustin R.; Durante, Daniele; Folkner, William M.; Parisi, Marzia; Tortora, Paolo; Zannoni, Marco; Anderson, John D.; Asmar, Sami W.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/608160
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