What do we know? Pre-Cassini

They have some detailed images of methane clouds at Titan's south pole.

http://www.gps.caltech.edu/~antonin/titan/

One of the surprising things is that cloud evolution should be so dynamic on Titan -- energy from the Sun is 100 times less than it is on Earth, so one might expect much slower evolution of the atmosphere.

It is possible that chemical reactions -- making and breaking atmospheric hydrocarbons -- contributes energy to the atmosphere and the formation/evolution of clouds.

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