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This is an image of Titania.
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NASA

Surface of Titania

The surface of Titania is typical of an icy moon. It appears to be resurfaced, and changed for it is lightly cratered with grooves and ridges similar to those found on Ganymede extending for many kilometers over the entire surface. These indicate that there has been activity in the interior of Titania in the past.


Last modified November 20, 2000 by Jennifer Bergman.

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Titania

Titania was discovered by W. Herschel in 1787. It has a standoff distance of 435,840 km. Titania is about as wide as the state of California is long, being 1580 km (1053 miles) in size. The surface features...more

Miranda

Miranda was discovered by G. Kuiper in 1948. It has a standoff distance of 129,780 km. Miranda one of the smallest icy moons, and is as wide as the distance from Los Angeles to San Francisco, being 47...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 indicate that there has been activity inside Miranda...more

Oberon

Oberon was discovered by W. Herschel in 1787. It has a standoff distance of 582,600 km. Oberon is about as wide as the state of California is long, being 1520 km (1013 miles) in size. The surface features...more

Surface of Oberon

The surface of Oberon is typical of an icy moon. It appears to be resurfaced, and changed for it is lightly cratered with grooves and ridges similar to those found on Ganymede extending for many kilometers...more

Surface of Oberon

The surface of Oberon is typical of an icy moon. It appears to be resurfaced, and changed for it is lightly cratered with grooves and ridges similar to those found on Ganymede extending for many kilometers...more

Puck

Puck was discovered by Voyager 2 in 1986. It has a standoff distance of 86,010 km. Puck is one of the small moons, and is about as wide as a county at 150 km (100 miles) long. As a small moon, the composition...more

Surface of Titania

The surface of Titania is typical of an icy moon. It appears to be resurfaced, and changed for it is lightly cratered with grooves and ridges similar to those found on Ganymede extending for many kilometers...more

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