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Predicting the weather on Titan?

Monday, January 30, 2006

False-colour Images of Titan
False-colour Images of Titan (obtained by the Cassini-Huygens Visual Infrared Mapping Spectrometer)
Credits: NASA/JPL/University of Arizona
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Using recent Cassini, Huygens and Earth-based observations, scientists have been able to create a computer model which explains the formation of several types of ethane and methane clouds on Titan.
Clouds have been observed recently on Titan, Saturn’s largest moon, through the thick haze, using near-infrared spectroscopy and images of the south pole and temperate regions near 40° South. Recent observations from Earth-based telescopes and the NASA/ESA/ASI Cassini spacecraft are now providing an insight into cloud climatology.

More:ESA Science-Predicting the weather on Titan