The depth of Jupiter's Great Red Spot constrained by the Juno gravity overflights - Archive ouverte HAL
Article Dans Une Revue Science Année : 2021

The depth of Jupiter's Great Red Spot constrained by the Juno gravity overflights

Marzia Parisi
  • Fonction : Auteur
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Daniele Durante
Scott J Bolton
Steven M Levin
Dustin R Buccino
Leigh N Fletcher
William M Folkner
Tristan Guillot
Luciano Iess
Cheng Li
Michael H Wong

Résumé

Jupiter’s Great Red Spot (GRS) is the largest atmospheric vortex in the Solar System and has been observed for at least two centuries. It has been unclear how deep the vortex extends beneath its visible cloud tops. We examined the gravity signature of the GRS using data from 12 encounters of the Juno spacecraft with the planet, including two direct overflights of the vortex. Localized density anomalies due to the presence of the GRS caused a shift in the spacecraft line-of-sight velocity. Using two different approaches to infer the GRS depth, which yielded consistent results, we conclude that the GRS is contained within the upper 500 kilometers of Jupiter’s atmosphere.
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Dates et versions

hal-03551811 , version 1 (01-02-2022)

Identifiants

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Marzia Parisi, Yohai Kaspi, Eli Galanti, Daniele Durante, Scott J Bolton, et al.. The depth of Jupiter's Great Red Spot constrained by the Juno gravity overflights. Science, 2021, 374 (6570), pp.964-968. ⟨10.1126/science.abf1396⟩. ⟨hal-03551811⟩
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