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  2. Rings of Saturn - Wikipedia

    en.wikipedia.org/wiki/Rings_of_Saturn

    A Cassini image of the faint D Ring, with the inner C Ring below. The D Ring is the innermost ring, and is very faint. In 1980, Voyager 1 detected within this ring three ringlets designated D73, D72 and D68, with D68 being the discrete ringlet nearest to Saturn.

  3. Prometheus (moon) - Wikipedia

    en.wikipedia.org/wiki/Prometheus_(moon)

    Prometheus is a shepherd satellite for the inner edge of Saturn's narrow F Ring. Pandora orbits just outside the F Ring, and has traditionally been viewed as an outer shepherd of the ring; however, recent studies indicate that only Prometheus contributes to the confinement of the ring. [9] [10]

  4. Ring system - Wikipedia

    en.wikipedia.org/wiki/Ring_system

    Ring system. The moons Prometheus (right) and Pandora (left) orbit just inside and outside, respectively, the F ring of Saturn, but only Prometheus is thought to function as a shepherd moon. A ring system is a disc or torus orbiting an astronomical object that is composed of solid material such as gas, dust, meteoroids, planetoids or moonlets ...

  5. Pan (moon) - Wikipedia

    en.wikipedia.org/wiki/Pan_(moon)

    Pan is the innermost named moon of Saturn. [ 4 ] It is a small, ravioli [ 5 ] -shaped moon approximately 35 kilometres across and 23 km wide that orbits within the Encke Gap in Saturn's A Ring. Pan is a ring shepherd and is responsible for keeping the Encke Gap free of ring particles. It is sometimes described as having the appearance of a walnut.

  6. Daphnis (moon) - Wikipedia

    en.wikipedia.org/wiki/Daphnis_(moon)

    Daphnis (moon) Daphnis is an inner satellite of Saturn. It is also known as Saturn XXXV; its provisional designation was S/2005 S 1. [6][7] Daphnis is about 8 kilometers in diameter, and orbits the planet in the Keeler Gap within the A ring.

  7. Moons of Saturn - Wikipedia

    en.wikipedia.org/wiki/Moons_of_Saturn

    It is estimated that the A Ring contains 7,000–8,000 propellers larger than 0.8 km in size and millions larger than 0.25 km. [4] In April 2014, NASA scientists reported the possible consolidation of a new moon within the A Ring, implying that Saturn's present moons may have formed in a similar process in the past when Saturn's ring system was ...

  8. Cassini–Huygens - Wikipedia

    en.wikipedia.org/wiki/Cassini–Huygens

    [123] [124] A final Titan flyby on April 22, 2017, changed the orbit again to fly through the gap between Saturn and its inner ring days later on April 26. Cassini passed about 3,100 km (1,900 mi) above Saturn's cloud layer and 320 km (200 mi) from the visible edge of the inner ring; it successfully took images of Saturn's atmosphere and began ...

  9. Orbital resonance - Wikipedia

    en.wikipedia.org/wiki/Orbital_resonance

    In the rings of Saturn, the Cassini Division is a gap between the inner B Ring and the outer A Ring that has been cleared by a 2:1 resonance with the moon Mimas. (More specifically, the site of the resonance is the Huygens Gap, which bounds the outer edge of the B Ring.)