CAVALIÉ, T.; LELLOUCH, E.,; HARTOGH, P.,; MORENO, R.,; BILLEBAUD, F.; BOCKELÉE-MORVAN, D.,; BIVER, N.,; CASSIDY, T.,; COURTIN, R.,; CROVISIER, J.,; DOBRIJEVIC, M.; FEUCHTGRUBER, H.,; GONZÁLEZ, A.,; GREATHOUSE, T.,; JARCHOW, C.,; KIDGER, M.,; LARA, L. M.,; RENGEL, M.,; ORTON, G.,; SAGAWA, H.,; DE VAL-BORRO, M.,

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CAVALIÉ, T.
Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
Observatoire aquitain des sciences de l'univers [OASU]
ASP 2014

LELLOUCH, E.,
Laboratoire d'études spatiales et d'instrumentation en astrophysique [LESIA]

HARTOGH, P.,
Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]

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Este ítem está publicado en

SF2A-2014: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics. Eds.: J. Ballet, F. Martins, F. Bournaud, R. Monier, C. Reylé, pp.173-176, 2014-06-03, Paris. 2014-12p. 173 - 176

Resumen en inglés

This paper reviews the recent findings of the Herschel Solar System Observations Key Program (Hartogh et al. 2009b), as well as ground-based supporting observations, regarding the origin of external oxygen in the environments of Jupiter and Saturn. Herschel-HIFI and PACS observations have been used to shown that the Shoemaker-Levy 9 comet is the source of Jupiter’s stratospheric water, and that Enceladus (and its geysers) are most probably the source of water for Saturn and Titan.< Leer menos

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Laboratoire d'Astrophysique de Bordeaux (LAB) - UMR 5804