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  2. Moons of Saturn - Wikipedia

    en.wikipedia.org/wiki/Moons_of_Saturn

    Phoebe was the first moon of Saturn to be studied in detail by Cassini, in June 2004; during this encounter Cassini was able to map nearly 90% of the moon's surface. Phoebe has a nearly spherical shape and a relatively high density of about 1.6 g/cm 3 . [ 30 ]

  3. Titan (moon) - Wikipedia

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

    Discovered in 1655 by the Dutch astronomer Christiaan Huygens, Titan was the first known moon of Saturn and the sixth known planetary satellite (after Earth's moon and the four Galilean moons of Jupiter). Titan orbits Saturn at 20 Saturn radii or 1,200,000 km above Saturn's apparent surface. From Titan's surface, Saturn subtends an arc of 5.09 ...

  4. Astronomers create first global map of Saturn's moon Titan - AOL

    www.aol.com/news/2019-11-24-first-global-map-of...

    Scientists finally have a comprehensive view of Titan, Saturn's largest moon. A team of astronomers has created the first global map of Titan by using the Cassini probe's over 100 fly-bys to ...

  5. Enceladus - Wikipedia

    en.wikipedia.org/wiki/Enceladus

    Enceladus is the sixth-largest moon of Saturn and the 18th-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.

  6. Geology of Titan - Wikipedia

    en.wikipedia.org/wiki/Geology_of_Titan

    Based on the observations, scientists announced "definitive evidence of lakes filled with methane on Saturn's moon Titan" in January 2007. [10] [11] The Cassini–Huygens team concluded that the imaged features are almost certainly the long-sought hydrocarbon lakes, the first stable bodies of surface liquid found outside Earth. [10]

  7. Chrysalis (hypothetical moon) - Wikipedia

    en.wikipedia.org/wiki/Chrysalis_(hypothetical_moon)

    The moon would have been torn apart by Saturn's tidal forces, somewhere between 200 and 100 million years ago. Up to 99% of the moon's mass would have been swallowed by Saturn, with the remaining 1% forming the rings of Saturn. [2] The origin of Saturn's rings from the destruction of a satellite has been previously proposed by other authors. [3]

  8. Hyperion (moon) - Wikipedia

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

    Hyperion / h aɪ ˈ p ɪər i ə n /, also known as Saturn VII, is the eighth-largest moon of Saturn. It is distinguished by its highly irregular shape, chaotic rotation, low density , and its unusual sponge-like appearance.

  9. Dione (moon) - Wikipedia

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

    Dione (/ d aɪ ˈ oʊ n i /), 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.