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SOLAR SYSTEM - OUTER PLANETS
Lesson 2 - Page 6

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URANUS

Uranus was discovered in 1781 by Sir William Herschel, seeing a featureless, bluish, green disk in his telescope. The atmosphere is mainly hydrogen with a minor percentage helium. A thin methane ice clouds was detected by Voyager 2. Deep within Uranus exists a superheated water ocean, perhaps 10,000 km deep which contains large concentrations of ionized chemicals. It is from this ocean that the magnetic field may originate. Beneath this ionic ocean is believed to be a core of molten rocky materials. Unlike the other gas giant there is no evidence of any significant internal heat source. Uranus also has rings! Observations have indicated the presences of 10 narrow rings and one broad ring, in addition to 100 or more ringlets.


Uranus


Ariel, a moon of Uranus with many craters.

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