The "C Ring" is one of the several rings that make up the structure of the planet Saturn. It is located between the B Ring and the D Ring and is known for its relatively narrow width. The C Ring is primarily composed of ice particles and small rocky debris, which reflect sunlight, giving it a faint appearance compared to the brighter B Ring. Discovered by the Pioneer 11 spacecraft in the 1970s, the C Ring is less dense than its neighboring rings. It contains gaps and divisions, which are influenced by the gravitational pull of nearby moons, such as Mimas and Enceladus. These interactions contribute to the dynamic nature of Saturn's ring system.