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  2. Titan (moon) - Wikipedia

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

    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 degrees, and if it were visible through the moon's thick atmosphere, it would appear 11.4 times larger in the sky, in diameter, than the Moon from Earth, which subtends 0.48° of arc.

  3. Geology of Titan - Wikipedia

    en.wikipedia.org/wiki/Geology_of_Titan

    An image of Titan's surface from the Huygens lander. Titan is the only object in the outer Solar System where a spacecraft has landed and conducted surface operations. The geology of Titan encompasses the geological characteristics of Titan, the largest moon of Saturn. Titan's density of 1.881 g/cm 3 indicates that it is roughly 40–60% rock ...

  4. Huygens (spacecraft) - Wikipedia

    en.wikipedia.org/wiki/Huygens_(spacecraft)

    Huygens (/ ˈ h ɔɪ ɡ ən z / HOY-gənz) was an atmospheric entry robotic space probe that landed successfully on Saturn's moon Titan in 2005. Built and operated by the European Space Agency (ESA), launched by NASA, it was part of the Cassini–Huygens mission and became the first spacecraft to land on Titan and the farthest landing from Earth a spacecraft has ever made. [3]

  5. Lakes of Titan - Wikipedia

    en.wikipedia.org/wiki/Lakes_of_Titan

    Lakes of liquid ethane and methane exist on the surface of Titan, Saturn's largest moon. This was confirmed by the Cassini–Huygens space probe, as had been suspected since the 1980s. [2] The large bodies of liquid are known as maria (seas) and the small ones as lacūs (lakes). [3]

  6. List of geological features on Titan - Wikipedia

    en.wikipedia.org/wiki/List_of_geological...

    This is a list of named geological features on Saturn's moon Titan. Official names for these features have only been announced since the 2000s, as Titan's surface was virtually unknown before the arrival of the Cassini–Huygens probe. [1] [2] Some features were known by informal nicknames beforehand; these names are noted where appropriate ...

  7. Cassini’s radar images captured the unexplained bright regions in Ligeia Mare, the second-largest liquid body on Titan’s surface. The sea is 50% larger than Lake Superior and is made up of ...

  8. Category:Surface features of Titan (moon) - Wikipedia

    en.wikipedia.org/wiki/Category:Surface_features...

    Pages in category "Surface features of Titan (moon)" The following 32 pages are in this category, out of 32 total. This list may not reflect recent changes. *

  9. Kraken Mare - Wikipedia

    en.wikipedia.org/wiki/Kraken_Mare

    Kraken Mare / ˈ k r ɑː k ən ˈ m ɑːr eɪ / is the largest known hydrocarbon sea on the surface of Saturn's moon Titan. It was discovered by the space probe Cassini in 2006, and was named in 2008 after the Kraken, a legendary sea monster. [1] It covers an area slightly bigger than the Caspian Sea on Earth, making it the largest known lake ...