Saturn's B and C rings disappear behind the immense planet
Saturn's B and C rings disappear behind the immense planet.
Where they meet the limb, the rings appear to bend slightly owing to
upper-atmospheric refraction.
Crenulations,
irregularly wavy or serrated features, in the planet's clouds denote the
locations of turbulent belt/zone boundaries.
The view was obtained with the Cassini spacecraft wide-angle
camera on Aug. 16, 2006 at a distance of approximately 256,000 kilometers
(159,000 miles) from Saturn.
-- SPACE.com Staff
Credit: NASA/JPL/Space
Science Institute
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