Observation of water vapor in the stratosphere of Jupiter with the Odin space telescope
Artikel i vetenskaplig tidskrift, 2008
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 submillimeter wavelength 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 variability would be contradictory with an IDP steady flux, thus supporting the SL9 source hypothesis. © 2008 Elsevier Ltd.
Water
Odin space telescoope
Jupiter
Atmosphere
Spectroscopy
Författare
T. Cavalie
Centre national de la recherche scientifique (CNRS)
F. Billebaud
Centre national de la recherche scientifique (CNRS)
N. Biver
GEPI - Galaxies, Etoiles, Physique, Instrumentation
M. Dobrijevic
Centre national de la recherche scientifique (CNRS)
E. Lellouch
GEPI - Galaxies, Etoiles, Physique, Instrumentation
J. Brillet
Centre national de la recherche scientifique (CNRS)
A. Lecacheux
GEPI - Galaxies, Etoiles, Physique, Instrumentation
Åke Hjalmarson
Chalmers, Institutionen för radio- och rymdvetenskap, Radioastronomi och astrofysik
Aa. Sandqvist
Stockholm Observatory
U. Frisk
Swedish Space Corporation (SSC)
Michael Olberg
Chalmers, Institutionen för radio- och rymdvetenskap, Nationella anläggningen för radioastronomi
E.A. Bergin
Harvard-Smithsonian Center for Astrophysics
Planetary and Space Science
0032-0633 (ISSN)
Vol. 56 12 1573-1584Ämneskategorier
Astronomi, astrofysik och kosmologi
DOI
10.1016/j.pss.2008.04.013