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This is an image of Titania.
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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.


Last modified November 20, 2000 by Jennifer Bergman.

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Titania

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...more

Miranda

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...more

Surface of Miranda

The 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...more

Oberon

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. ...more

Surface of Oberon

The 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...more

Surface of Oberon

The 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...more

Puck

Puck was discovered by Voyager 2 in 1986. Puck is one of the small moons, and is about as wide as a county....more

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. ...more

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