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  2. Moons of Saturn - Wikipedia

    en.wikipedia.org/wiki/Moons_of_Saturn

    Although the boundaries may be somewhat vague, Saturn's moons can be divided into ten groups according to their orbital characteristics. Many of them, such as Pan and Daphnis , orbit within Saturn's ring system and have orbital periods only slightly longer than the planet's rotation period. [ 46 ]

  3. Orbital period - Wikipedia

    en.wikipedia.org/wiki/Orbital_period

    Orbit insertion. v. t. e. The orbital period (also revolution period) is the amount of time a given astronomical object takes to complete one orbit around another object. In astronomy, it usually applies to planets or asteroids orbiting the Sun, moons orbiting planets, exoplanets orbiting other stars, or binary stars.

  4. Saturn - Wikipedia

    en.wikipedia.org/wiki/Saturn

    The Moon's orbit is inclined by several degrees relative to Saturn's, so occultations will only occur when Saturn is near one of the points in the sky where the two planes intersect (both the length of Saturn's year and the 18.6-Earth-year nodal precession period of the Moon's orbit influence the periodicity).

  5. Orbital resonance - Wikipedia

    en.wikipedia.org/wiki/Orbital_resonance

    One theory for why the resonance came to an end is that there was another moon around Saturn whose orbit destabilized about 100 million years ago, perturbing Saturn. [21] [22] The perihelion secular resonance between asteroids and Saturn6 = g − g 6) helps shape the asteroid belt (the subscript "6" identifies Saturn as the sixth planet ...

  6. Rhea (moon) - Wikipedia

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

    Rhea (/ ˈriː.ə /) is the second-largest moon of Saturn and the ninth-largest moon in the Solar System, with a surface area that is comparable to the area of Australia. It is the smallest body in the Solar System for which precise measurements have confirmed a shape consistent with hydrostatic equilibrium. Rhea has a nearly circular orbit ...

  7. Enceladus - Wikipedia

    en.wikipedia.org/wiki/Enceladus

    Enceladus is the sixth-largest moon of Saturn and the 19th-largest in the Solar System. It is about 500 kilometers (310 miles) in diameter, [5] about a tenth of that of Saturn 's largest moon, Titan. It is mostly covered by fresh, clean ice, making it one of the most reflective bodies of the Solar System.

  8. Dione (moon) - Wikipedia

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

    Dione (moon) Dione (/ daɪˈoʊni /), also designated Saturn IV, is the fourth-largest moon of Saturn. With a mean diameter of 1,123 km and a density of about 1.48 g/cm 3, Dione is composed of an icy mantle and crust overlying a silicate rocky core, with rock and water ice roughly equal in mass. Its trailing hemisphere is marked by large cliffs ...

  9. Prometheus (moon) - Wikipedia

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

    Contents. Prometheus (moon) For the asteroid, see 1809 Prometheus. Prometheus / prəˈmiːθiːəs / is an inner satellite of Saturn. It was discovered on 24 October 1980 from images taken by the Voyager 1 probe, and was provisionally designated S/1980 S 27. [ 6 ] In late 1985 it was officially named after Prometheus, a Titan in Greek mythology ...