A recent article in the New York Times highlighted that during the four years Cassini has been at Saturn, the level of liquid in the methane lakes of the southern hemisphere of Titan have dropped. The methane lakes were originally detected by radar instruments onboard the spacecraft. Because Cassini has had a unique opportunity to study the planet and it's moons over time, the changes can be linked to seasons on Titan.
Q: Why is this giant crater on Mimas oddly colored?
A: Because the outer solar system is a fascinating place! Could use some pink spice geysers though.
The so-nicknamed PacMan on Saturn's moon Mimas imaged with Cassini is just temperature variations over the surface possibly due to different surface materials.