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  2. Titan (moon) - Wikipedia

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

    Huygens in situ image from Titan's surface—the only image from the surface of a body permanently farther away than Mars Same image with contrast enhanced Huygens was an atmospheric probe that touched down on Titan on January 14, 2005, [ 114 ] discovering that many of its surface features seem to have been formed by fluids at some point in the ...

  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. 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 ...

  6. Lakes of Titan - Wikipedia

    en.wikipedia.org/wiki/Lakes_of_Titan

    A flyby of Titan's southern polar regions in October 2007 revealed similar, though far smaller, lakelike features. [15] Infrared specular reflection off Jingpo Lacus, a north polar body of liquid. Image of Titan taken during Huygens' descent, showing hills and topographical features that resemble a shoreline and drainage channels.

  7. Radar study puts spotlight on Saturn moon Titan's ... - AOL

    www.aol.com/news/radar-study-puts-spotlight...

    Titan, shrouded in a smog-like orange haze, is the only known world other than Earth exhibiting liquid seas on the surface, though they are not composed of water but rather nitrogen and the ...

  8. 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]

  9. Xanadu (Titan) - Wikipedia

    en.wikipedia.org/wiki/Xanadu_(Titan)

    Radar images taken by Cassini have revealed dunes, hills, rivers and valleys present on Xanadu. The features are likely carved in water ice by liquid methane or ethane. [2] Water ice behaves similarly to rock at the pressures and temperatures present on Titan's surface.