Titania (moon)

Titania (moon)

Titania is the largest of the moons of Uranus and the eighth largest moon in the Solar System at a diameter of 1,578 kilometres (981 mi). Discovered by William Herschel in 1787, Titania is named after the queen of the fairies in Shakespeare's A Midsummer Night's Dream. Its orbit lies inside Uranus' magnetosphere.

Titania consists of approximately equal amounts of ice and rock, and is probably differentiated into a rocky core and an icy mantle. A layer of liquid water may be present at the core–mantle boundary. The surface of Titania, which is relatively dark and slightly red in color, appears to have been shaped by both impacts and endogenic processes. It is covered with numerous impact craters reaching up to 326 kilometres (203 mi) in diameter, but is less heavily cratered than the surface of Uranus' outermost moon, Oberon. Titania probably underwent an early endogenic resurfacing event which obliterated its older, heavily cratered surface. Titania's surface is cut by a system of enormous canyons and scarps, the result of the expansion of its interior during the later stages of its evolution. Like all major moons of Uranus, Titania probably formed from an accretion disk which surrounded the planet just after its formation.

Infrared spectroscopy conducted from 2001 to 2005 revealed the presence of water ice as well as frozen carbon dioxide on the surface of Titania, which in turn suggested that the moon may possess a tenuous carbon dioxide atmosphere with a surface pressure of about one 10 trillionth of a bar. Measurements during Titania's occultation of a star put an upper limit on the surface pressure of any possible atmosphere at 10–20 nbar.

As of 2012, the Uranian system has been studied up close only once, by the spacecraft Voyager 2 in January 1986. It took several images of Titania, which allowed mapping of about 40% of the moon’s surface.

Read more about Titania (moon):  Discovery and Naming, Orbit, Composition and Internal Structure, Surface Features, Atmosphere, Origin and Evolution, Exploration

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Titania (moon) - Exploration
... So far the only close-up images of Titaniahave been from the Voyager 2 probe, which photographed the moonduring its flyby of Uranus in January 1986 ... Since the closest distance between Voyager 2 and Titaniawas only 365,200 kilometres (226,900 mi), the best images of this moonhave a spatial resolution of about 3.4 km (only Miranda and Ariel ... At the time of the flyby, the southern hemisphere of Titania(like those of the other moons was pointed towards the Sun, so the northern (dark) hemisphere could not be ...