Titania

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Details

Titania is Uranus' largest moon, about 1,600 kilometers across. Voyager 2 saw long fault valleys and other signs of crustal extension, showing that this gray icy moon was not simply a frozen, inactive sphere.

Titania matters because it anchors the Uranian moon system by size. It is Uranus' largest moon, discovered by William Herschel in 1787 and finally seen up close when Voyager 2 passed the Uranian system almost two centuries later. The image did not reveal a featureless ice ball.

What Voyager 2 saw were signs of tectonic extension in an icy crust. NASA describes long fault valleys, some nearly 1,000 miles long, and reflective deposits along sun-facing valley walls that may be frost. Those features make Titania feel like a world that changed after it formed, rather than a passive frozen remnant.

That is why Titania belongs on this scale. It is not as famous as the Galilean moons or Titan, but it gives Uranus a major satellite with its own geological signature. Titania shows that even the distant, underexplored Uranian system contains moons whose surfaces record internal stress and crustal motion.

699km
Visual creditzelario12, using Voyager 2 imagery by NASA / JPL / CC BY-SA 2.0Source: Wikimedia Commons

Key facts

Category
Moons
Object class
Large icy moon
Composition
Water ice and silicate rock
Scale fact
1,600 kmdiameter
Estimated age
~4.5 billion years
Host
Uranus

Scale context

Where Titania sits on the full axis

By size on the journey, Titania sits between Rhea and Haumea. The band below compares Titania with nearby Large icy moon objects so the size jump stays easy to read.

Shared physical scale
3,938km
Rhea1,528 km
Titania1,600 km
Titan5,150 km

Together, these objects make the size change around Titania easy to compare at a glance.

Sources

References for Titania

Measurements and descriptive context are compiled by the Scale of Space team from the references below. If you find an error, please let us know.

Between the smallest and the largest, perspective is everything.

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