Astrodude Space

Titania: Uranus’s Largest Moon with Striking Geological Features

Titania is the largest moon of Uranus, discovered by William Herschel on January 11, 1787. It is named after the queen of the fairies in Shakespeare’s A Midsummer Night’s Dream. Titania’s surface is marked by a complex network of faults and valleys, evidence of past geological activity. It is the eighth-largest moon in the Solar System, with a diameter of about 1,578 km (981 miles). Titania appears to be composed of roughly equal parts rock and ice.

Its surface resembles that of Uranus’s moon Ariel, with a mixture of small impact craters and large canyons and fault systems. A prominent system of valleys extends for nearly 1,600 km (1,000 miles). Evidence from the Voyager 2 mission suggests that Titania was once geologically active, with tectonic extension causing fissures to open in its icy crust. Bright deposits—possibly frost—are visible on the sun-facing walls of some valleys.

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