Saturn
Cloud formations, storms, and strong winds define the observed surface
   - low density atmosphere, rich in hydrogen and helium – less dense than water!
- sunlight shines less brightly than on Jupiter, so clouds are cooler
- ice common
Numerous, beautiful rings!
   - made of ice (shiny) – cometary remnants?
- 1,000s of rings in total
- only a few meters wide (RSaturn = 6 × 107 meters)
- shepherd moons push and hold the rings in place
  Many major and minor moons – accreted asteroids?
   - Titan: 
       rock and ice, nitrogen atmosphere (smoggy, inverse greenhouse effect), very cold
- Tethys: 
       rock and ice, cracked, cratered and old
- Enceladus: 
       recent geological activity (lightly cratered regions), heated by tides
|  
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  Tethys and Diones
 |  Mimas
 |  Inside the Rings
 | 
|  Shadowed rings
 |  Red Cloud Feature
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| Images of Saturn, its primary moons, and its glorious rings.  [NASA] |