Journal article
In situ and remote observations of the ultraviolet footprint of the moon Callisto by the Juno spacecraft
Nature communications, Vol.16(1), 7791
09/01/2025
DOI: 10.1038/s41467-025-62520-4
PMCID: PMC12402282
PMID: 40890092
Abstract
Jupiter exhibits peculiar multiwavelength auroral emissions resulting from the electromagnetic interactions of Io, Europa, and Ganymede with the magnetospheric plasma flow. Characterizing the faint auroral footprint of the fourth Galilean moon, Callisto, has always been challenging because of its expected weakness and its proximity to Jupiter's bright main aurora. Here, we report on unusual magnetospheric conditions that led to an equatorward shift of Jupiter's main auroral oval unveiling the auroral footprints of the four Galilean moons in a single observation. Remote observations by the Juno spacecraft reveal a double-spot structure, characteristic of the footprints of the other three moons, with a maximum ultraviolet brightness of 137
15 kR. Concurrent observations within Callisto's flux tube reveal field-aligned electrons with a characteristic energy of 10 keV, depositing an energy flux of 55 mW.m
in Jupiter's atmosphere. The electron properties are consistent with the triggering of radio emissions with intensities lower than 5 × 10
W.m
.Hz
.
Details
- Title: Subtitle
- In situ and remote observations of the ultraviolet footprint of the moon Callisto by the Juno spacecraft
- Creators
- J Rabia - Centre National de la Recherche ScientifiqueV Hue - Aix-Marseille UniversitéC K Louis - Université Paris CitéN André - Centre National de la Recherche ScientifiqueQ Nénon - Centre National de la Recherche ScientifiqueJ R Szalay - Princeton UniversityR Prangé - Université Paris CitéL Lamy - Université Paris CitéP Zarka - Centre National de la Recherche ScientifiqueB Collet - Aix-Marseille UniversitéF Allegrini - Southwest Research InstituteR W Ebert - Southwest Research InstituteT K Greathouse - Southwest Research InstituteB Bonfond - University of LiègeG R Gladstone - Southwest Research InstituteA H Sulaiman - University of MinnesotaW S Kurth - University of IowaJ E P Connerney - Goddard Space Flight CenterP Louarn - Institut de Recherche en Astrophysique et PlanétologieE Penou - Institut de Recherche en Astrophysique et PlanétologieA Kamran - Institut de Recherche en Astrophysique et PlanétologieD Santos-Costa - Southwest Research InstituteR S Giles - Southwest Research InstituteJ A Kammer - Southwest Research InstituteM H Versteeg - Southwest Research InstituteS J Bolton - Southwest Research Institute
- Resource Type
- Journal article
- Publication Details
- Nature communications, Vol.16(1), 7791
- DOI
- 10.1038/s41467-025-62520-4
- PMID
- 40890092
- PMCID
- PMC12402282
- NLM abbreviation
- Nat Commun
- ISSN
- 2041-1723
- eISSN
- 2041-1723
- Publisher
- NATURE PORTFOLIO
- Grant note
- EUR TESS N°ANR-18-EURE-0018 / Agence Nationale de la Recherche (French National Research Agency) A*MIDEX AMX-22-CPJ-04 / Aix-Marseille Université (Aix-Marseille University)
- Language
- English
- Date published
- 09/01/2025
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9984958293802771
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