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Hydrogen peroxide at the poles of Ganymede.
Trumbo, Samantha K; Brown, Michael E; Bockelée-Morvan, Dominique; de Pater, Imke; Fouchet, Thierry; Wong, Michael H; Cazaux, Stéphanie; Fletcher, Leigh N; de Kleer, Katherine; Lellouch, Emmanuel; Mura, Alessandro; Poch, Olivier; Quirico, Eric; Rodriguez-Ovalle, Pablo; Showalter, Mark R; Tiscareno, Matthew S; Tosi, Federico.
Afiliação
  • Trumbo SK; Cornell Center for Astrophysics and Planetary Science, Cornell University, Ithaca, NY 14853, USA.
  • Brown ME; Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA.
  • Bockelée-Morvan D; LESIA, Observatoire de Paris, Université PSL, Sorbonne Université, Université Paris Cité, CNRS, Meudon 92195, France.
  • de Pater I; Departments of Astronomy and of Earth and Planetary Science, University of California, Berkeley, CA 94720, USA.
  • Fouchet T; LESIA, Observatoire de Paris, Université PSL, Sorbonne Université, Université Paris Cité, CNRS, Meudon 92195, France.
  • Wong MH; Center for Integrative Planetary Science, University of California, Berkeley, CA 94720-3411, USA.
  • Cazaux S; Faculty of Aerospace Engineering, Delft University of Technology, Delft, Netherlands.
  • Fletcher LN; Leiden Observatory, Leiden University, P.O. Box 9513, NL 2300 RA, Leiden, Netherlands.
  • de Kleer K; School of Physics and Astronomy, University of Leicester, Leicester LE1 7RH, UK.
  • Lellouch E; Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA.
  • Mura A; LESIA, Observatoire de Paris, Université PSL, Sorbonne Université, Université Paris Cité, CNRS, Meudon 92195, France.
  • Poch O; Istituto Nazionale di AstroFisica-Istituto di Astrofisica e Planetologia Spaziali (INAF-IAPS), Rome, Italy.
  • Quirico E; Université Grenoble Alpes, Centre National de la Recherche Scientifique (CNRS), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Grenoble 38000, France.
  • Rodriguez-Ovalle P; Université Grenoble Alpes, Centre National de la Recherche Scientifique (CNRS), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Grenoble 38000, France.
  • Showalter MR; LESIA, Observatoire de Paris, Université PSL, Sorbonne Université, Université Paris Cité, CNRS, Meudon 92195, France.
  • Tiscareno MS; SETI Institute, Mountain View, CA 94043, USA.
  • Tosi F; SETI Institute, Mountain View, CA 94043, USA.
Sci Adv ; 9(29): eadg3724, 2023 Jul 21.
Article em En | MEDLINE | ID: mdl-37478185
ABSTRACT
Ganymede is the only satellite in the solar system known to have an intrinsic magnetic field. Interactions between this field and the Jovian magnetosphere are expected to funnel most of the associated impinging charged particles, which radiolytically alter surface chemistry across the Jupiter system, to Ganymede's polar regions. Using observations obtained with JWST as part of the Early Release Science program exploring the Jupiter system, we report the discovery of hydrogen peroxide, a radiolysis product of water ice, specifically constrained to the high latitudes. This detection directly implies radiolytic modification of the polar caps by precipitation of Jovian charged particles along partially open field lines within Ganymede's magnetosphere. Stark contrasts between the spatial distribution of this polar hydrogen peroxide, those of Ganymede's other radiolytic oxidants, and that of hydrogen peroxide on neighboring Europa have important implications for understanding water-ice radiolysis throughout the solar system.

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2023 Tipo de documento: Article

Texto completo: 1 Base de dados: MEDLINE Idioma: En Ano de publicação: 2023 Tipo de documento: Article