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| Titan
Titan is the fifteenth of Saturn's moons, and its largest. It has a diameter of 3,200 miles (5,150 kilometers), and orbits Saturn at a distance of 758,756 miles (1,221,830 kilometers). It was discovered by Christiaan Huygens in 1655. In Greek mythology the Titans were a family of giants, the children of Uranus and Gaia, who sought to rule the heavens but were overthrown and supplanted by the family of Zeus.
Titan is similar in composition to Ganymede, Callisto, Triton, and (probably) Pluto, being about half water ice and half rocky material. It may have a rocky center surrounded by several layers composed of different crystal forms of ice, and may have an interior that is still hot. Unlike almost every other satellite in the Solar System, Titan has a significant atmosphere. It is composed primarily of molecular nitrogen, with no more than 6% argon and a small amount of methane. There are also trace amounts of at least a dozen other organic compounds -- including ethane, hydrogen cyanide and carbon dioxide -- and water. The atmosphere is actually so thick that for centuries it was thought that Titan was actually larger than Ganymede. At the surface, the pressure is 50% higher than Earth's. At the surface, Titan's temperature is about -290° F. At this temperature water ice does not sublimate, meaning there is little wapor vapor in the atmosphere. But there are clouds in that atmosphere, most likely composed of methane, ethane, or other simple organics. Pictures of Titan's surface indicate that those clouds may actually produce enough "rain" to create rivers and lakes. In addition, Cassini found evidence of a "volcano" which may be responsible for replenishing Titan's atmosphere.
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ROBINSON LIBRARY --> Science. --> Astronomy. --> Solar System. This page was last updated on 08/09/2011. |
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