This is an image of Titania.
Click on image for full size
NASA
Surface of Titania
The surface of Titania is like many icy moons. It does not have many craters. Instead it has grooves similar to those found on
Ganymede. These grooves extend for many kilometers over the surface.
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Titania was discovered by W. Herschel in 1787. Titania is about as wide as the state of California is long. The surface features of this moon are hard to see in this image. The surface suggests that Titania
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Miranda was discovered by G. Kuiper in 1948. Miranda one of the smallest icy moons, and is as wide as the distance from Los Angeles to San Francisco. The surface features of this moon are hard to see in
...moreThe surface of Miranda is very unusual. It is not like any other moon in the solar system. Miranda has many craters but also very big grooves. These show that there has been activity inside Miranda in
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Oberon was discovered by W. Herschel in 1787. Oberon is about as wide as the state of California is long. Oberon is probably one of the icy moons.
...moreThe surface of Oberon is like many icy moons. It appears to be changed for it does not have many craters. Instead it has grooves similar to those found on Ganymede. These grooves extend for ma ny kilometers
...moreThe surface of Oberon is like many icy moons. It appears to be changed for it does not have many craters. Instead it has grooves similar to those found on Ganymede. These grooves extend for ma ny kilometers
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Puck was discovered by Voyager 2 in 1986. Puck is one of the small moons, and is about as wide as a county.
...moreThe surface of Titania is like many icy moons. It does not have many craters. Instead it has grooves similar to those found on Ganymede. These grooves extend for many kilometers over the surface.
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