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

Marzia Parisi, Yohai Kaspi, Eli Galanti, Daniele Durante, Scott J Bolton, Steven M Levin, Dustin R. Buccino, Leigh N Fletcher, William M. Folkner, Tristan Guillot, Ravit Helled, Luciano Iess, Cheng Li, Kamal Oudrhiri, Michael H Wong

Research output: Contribution to journalArticlepeer-review

Abstract

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.

Original languageEnglish
Article numbereabf1396
Pages (from-to)964-968
Number of pages4
JournalScience (American Association for the Advancement of Science)
Volume374
Issue number6570
DOIs
StatePublished - 28 Oct 2021

All Science Journal Classification (ASJC) codes

  • General

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