Observation of water vapor in the stratosphere of Jupiter with the Odin Space Telescope. - Archive ouverte HAL Accéder directement au contenu
Article Dans Une Revue Planetary and Space Science Année : 2008

Observation of water vapor in the stratosphere of Jupiter with the Odin Space Telescope.

Résumé

The water vapor line at 557 GHz has been observed with the Odin space telescope with a high signal-to-noise ratio and a high spectral resolution on November 8, 2002. The analysis of this observation as well as a re-analysis of previously published observations obtained with the SubmillimeterWavelength Astronomy Satellite seem to favor a cometary origin (Shoemaker-Levy 9) for water in the stratosphere of Jupiter, in agreement with the ISO observation results. Our model predicts that the water line should become fainter and broader from 2007. The observation of such a temporal variablity would be contradictory with an IDP steady flux, thussupporting the SL9 source hypothesis.
Fichier principal
Vignette du fichier
cavalie2008-19.pdf (515.74 Ko) Télécharger le fichier
Origine : Fichiers produits par l'(les) auteur(s)
Loading...

Dates et versions

hal-00261908 , version 1 (10-03-2008)

Identifiants

Citer

T. Cavalié, F. Billebaud, N. Biver, M. Dobrijevic, E. Lellouch, et al.. Observation of water vapor in the stratosphere of Jupiter with the Odin Space Telescope.. Planetary and Space Science, 2008, 56 (12), pp.1573-1584. ⟨10.1016/j.pss.2008.04.013⟩. ⟨hal-00261908⟩
240 Consultations
176 Téléchargements

Altmetric

Partager

Gmail Facebook X LinkedIn More