Difference between revisions of "Titan"
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Titan (tye'-tən, IPA /ˈtaɪtn̩/, Greek Τιτάν) or Saturn VI is the largest moon of Saturn and the second largest moon in the solar system, after Jupiter's moon Ganymede. It was discovered on 1655-03-25 by the Dutch astronomer Christiaan Huygens, and was the first satellite in the Solar System to be discovered after the Galilean moons of Jupiter. Titan is the only moon in our solar system to have a dense atmosphere. Until very recently, this atmosphere inhibited understanding of Titan's surface, but the moon is currently undergoing study by the Cassini-Huygens mission, and new information about it is continuously accumulating, through sources such as [[Daedalus]]. | Titan (tye'-tən, IPA /ˈtaɪtn̩/, Greek Τιτάν) or Saturn VI is the largest moon of Saturn and the second largest moon in the solar system, after Jupiter's moon Ganymede. It was discovered on 1655-03-25 by the Dutch astronomer Christiaan Huygens, and was the first satellite in the Solar System to be discovered after the Galilean moons of Jupiter. Titan is the only moon in our solar system to have a dense atmosphere. Until very recently, this atmosphere inhibited understanding of Titan's surface, but the moon is currently undergoing study by the Cassini-Huygens mission, and new information about it is continuously accumulating, through sources such as [[Daedalus]]. | ||
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+ | For further information on Titan, see the [http://www.spacesim.org/mission(about_the_planet).htm About the Planet] section of the [http://www.spacesim.com OCESS Website]. |
Revision as of 19:40, 10 April 2006
Titan (tye'-tən, IPA /ˈtaɪtn̩/, Greek Τιτάν) or Saturn VI is the largest moon of Saturn and the second largest moon in the solar system, after Jupiter's moon Ganymede. It was discovered on 1655-03-25 by the Dutch astronomer Christiaan Huygens, and was the first satellite in the Solar System to be discovered after the Galilean moons of Jupiter. Titan is the only moon in our solar system to have a dense atmosphere. Until very recently, this atmosphere inhibited understanding of Titan's surface, but the moon is currently undergoing study by the Cassini-Huygens mission, and new information about it is continuously accumulating, through sources such as Daedalus.
For further information on Titan, see the About the Planet section of the OCESS Website.