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  2. 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]

  3. Climate of Titan - Wikipedia

    en.wikipedia.org/wiki/Climate_of_Titan

    Haze in Titan's atmosphere contributes to an anti-greenhouse effect by reflecting sunlight back into space, making its surface significantly colder than its upper atmosphere. [3] This partially compensates for the greenhouse warming, and keeps the surface somewhat cooler than would otherwise be expected from the greenhouse effect alone. [ 6 ]

  4. Anti-greenhouse effect - Wikipedia

    en.wikipedia.org/wiki/Anti-greenhouse_effect

    This acts to reduce solar energy reaching the surface and lets infrared energy escape, cooling Titan's surface. Titan has both a greenhouse and an anti-greenhouse effect which compete with one another. The greenhouse effect warms Titan by 21 K while the anti-greenhouse effect cools Titan by 9 K, so the net warming is 12 K (= 21 K - 9 K). [3] [4]

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

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

    On Titan, clouds spew methane - which is a gas on Earth - in liquid form due to the frigid climate. "Titan is really an Earth-like world with a diverse set of very familiar surface morphologies ...

  6. 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 ...

  7. Geology of Titan - Wikipedia

    en.wikipedia.org/wiki/Geology_of_Titan

    Mosaic of three Huygens images of channel system on Titan. The possibility of hydrocarbon seas on Titan was first suggested based on Voyager 1 and 2 data that showed Titan to have a thick atmosphere of approximately the correct temperature and composition to support them, but direct evidence was not obtained until 1995 when data from Hubble and other observations suggested the existence of ...

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