Detections of H2O lines on all four giant planets and Titan. More lines have been detected on the individual targets, for illustration only the 39.37µm line (resolved into 2 components on Jupiter by the FP) is shown.
These results have been discussed in the paper:
"Oxygen in the Stratospheres of the Giant Planets and Titan", H. Feuchtgruber and al., 1998 presented at the conference:
"The Universe as seen by ISO"
(Proceedings: ESA SP-427).
and in the article:
"ISO's Astronomical Harvest Continues" M. Kessler et al., published in the ESA Bulletin Nr. 99 (September 1999).
This figure is also available in high-resolution (300 dpi) format: EPS GIF
Return to the Introduction Page | Solar System Gallery