Daphnis is a small moon of Saturn, discovered by the Cassini spacecraft in 2005. It is located within the Keeler Gap of Saturn's A Ring and is only about 8 kilometers in diameter. One of the most remarkable features of Daphnis is a narrow, wavy ridge that runs along its equator. This ridge is thought to have formed as a result of the gravitational interactions between Daphnis and the surrounding ring particles, which cause the moon's equatorial regions to become raised and create the ridge-like feature. Another interesting feature of Daphnis is its influence on the surrounding ring material. As the moon orbits Saturn within the Keeler Gap, it creates waves and disturbances in the surrounding ring material, which can be seen as a series of "propeller" features on either side of the moon. Despite its small size, Daphnis is a fascinating moon that provides important insights into the dynamics of Saturn's rings and the interactions between moons and ring particles. The Cassini spacecraft captured stunning images of Daphnis and its surrounding environment during its mission, which have helped to deepen our understanding of this unique moon and the Saturnian system as a whole.
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