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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. 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 ...

  5. Orbital inclination - Wikipedia

    en.wikipedia.org/wiki/Orbital_inclination

    Orbital inclination measures the tilt of an object's orbit around a celestial body. It is expressed as the angle between a reference plane and the orbital plane or axis of direction of the orbiting object. For a satellite orbiting the Earth directly above the Equator, the plane of the satellite's orbit is the same as the Earth's equatorial ...

  6. 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 ...

  7. Fornjot (moon) - Wikipedia

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

    Fornjot / ˈfɔːrnjoʊt / or Saturn XLII is the outermost named moon of Saturn. Its discovery was announced by Scott S. Sheppard, David C. Jewitt, Jan Kleyna, and Brian G. Marsden on 4 May 2005 from observations taken between 12 December 2004, and 11 March 2005. It had the largest semi-major axis among all the known moons of Saturn [ 3 ]

  8. Atlas (moon) - Wikipedia

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

    Contents. Atlas (moon) Atlas is an inner satellite of Saturn which was discovered by Richard Terrile in 1980 from Voyager photos and was designated S/1980 S 28. [ 5 ] In 1983 it was officially named after Atlas of Greek mythology, because it "holds the rings on its shoulders" like the Titan Atlas held the sky up above the Earth. [ 6 ]

  9. 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.