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  2. Vid Flumina - Wikipedia

    en.wikipedia.org/wiki/Vid_Flumina

    Synthetic aperture radar image mosaic of Titan's north polar region. Vid Flumina is a river system (termed Flumen) of liquid methane and ethane on Saturn's moon Titan.It is more than 400 km (249 mi) long and flows into Titan's second largest hydrocarbon sea, Ligeia Mare. [1]

  3. Climate of Titan - Wikipedia

    en.wikipedia.org/wiki/Climate_of_Titan

    In September 2006, Cassini imaged a large cloud at a height of 40 km over Titan's north pole. Although methane is known to condense in Titan's atmosphere, the cloud was more likely to be ethane, as the detected size of the particles was only 1–3 micrometers and ethane can also freeze at these altitudes

  4. Atmosphere of Titan - Wikipedia

    en.wikipedia.org/wiki/Atmosphere_of_Titan

    The atmosphere of Titan is the dense layer of gases surrounding Titan, the largest moon of Saturn.Titan is the only natural satellite of a planet in the Solar System with an atmosphere that is denser than the atmosphere of Earth and is one of two moons with an atmosphere significant enough to drive weather (the other being the atmosphere of Triton). [4]

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

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

    NASA's Cassini spacecraft, which explored Saturn and its icy moons, including the majestic Titan, ended its mission with a death plunge into the giant ringed planet in 2017. Cassini's radar ...

  6. Explorer of Enceladus and Titan - Wikipedia

    en.wikipedia.org/.../Explorer_of_Enceladus_and_Titan

    Investigate the habitability and potential for life in ocean worlds on both Enceladus and Titan; Investigate Titan as an Earth-like world with an evolving climate and landscape. These goals would be accomplished by measuring the nature, abundance and isotopic properties of solid- and vapor-phase species in Enceladus' plume and Titan's upper ...

  7. Atmospheric super-rotation - Wikipedia

    en.wikipedia.org/wiki/Atmospheric_super-rotation

    Titans obliquity at 26.7° is high enough to cause seasonal variations within the stratospheric spin. [4] Attempts to model super-rotation on the gas giants, including Titan, has been abundant. The first observations of Titan in the 1980's revealed little information about circulation within the atmosphere due to the low contrast photochemical ...

  8. Titan Lake In-situ Sampling Propelled Explorer - Wikipedia

    en.wikipedia.org/wiki/Titan_Lake_In-situ...

    Titan Lake In-situ Sampling Propelled Explorer (TALISE) is a Spanish space probe proposed in 2012 [1] that would splash-down in Ligeia Mare, the second largest lake on Saturn's moon Titan. TALISE would navigate across the lake for six months to one year.

  9. Dragonfly (Titan space probe) - Wikipedia

    en.wikipedia.org/wiki/Dragonfly_(Titan_space_probe)

    Titan's dense atmosphere and low gravity mean that the flight power for a given mass is a factor of about 40 times lower than on Earth. [3] The atmosphere has 1.45 times the pressure and about four times the density of Earth's, and local gravity (13.8% of Earth's) make flight easier than on Earth, although cold temperatures, lower light levels ...