The achievements and potential of ISO archive for planetary studies

Details The achievements and potential of ISO archive for planetary studies The achievements and potential of ISO archive for planetary studies

Feb 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.511...41f&link_type=abstract

Exploiting the ISO Data Archive. Infrared Astronomy in the Internet Age, held in Siguenza, Spain 24-27 June, 2002. Edited by

Astronomy and Astrophysics

Astronomy

Scientific paper

The ISO observations of planetary objects have given several outstanding results. However, the potential from the ISO archive is still high as many observations, or some spectral ranges have not been analysed yet. The most strinking example being the ISOCAM observations of Jupiter and Saturn. This situation is due to the difficulty to reduce and calibrate the high flux (up to 106 Jy) planetary observations, to the lack of spectroscopic data or numerical tools to accurately analyse the data, and also because the planetary community focused on the most unexpected observations. The achievements and potential from ISO archive encompasses the atmospheric isotopic composition, the oxygen and hydrocarbon stratospheric chemistry in the Giant Planets and Titan, the cloud structure of Jupiter and Saturn, and the composition of planetary surfaces.

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