What is Miranda (moon)?
'''Miranda''' is one of [[Uranus (planet)|Uranus']] [[Satellite (natural)|moons]]. It is the smallest, and the one which has the least rotation time. [[Gerard Kuiper]] discovered it in 1948, February 16th and named it after [[Miranda (Shakespeare)|Miranda]], Prospero's daughter in [[William Shakespeare]]'s play ''[[The Tempest]]''. Sometimes it is also called '''Uranus V'''. It's one of Uranus' strangest moons. Its complex surface may indicate partial melting of its interior, with icy material drifting to the surface. The [[probe]] [[Voyager 2]] made some [[photo]]s in 1986. These are the only images that exist, so far. Geologically, it is the most active body in the Uranus system. The grooves and troughs reach depths of a few kilometers (or miles) and expose materials of different albedos (reflectivity). The features suggest a long, complex geologic evolution of this satellite. == Gallery == <gallery> Image:Miranda_mosaic_in_color_-_Voyager_2.png|A picture of Miranda Image:Miranda scarp.jpg|[[Verona Rupes]], the highest known [[cliff]] in the [[Solar System]] Image:PIA00140 Miranda Fractures, Grooves and Craters.jpg|An array of fractures, grooves and craters. This clear-filter, narrow-angle view shows areas of older, heavily cratered terrain with a wide variety of forms. Image:Miranda5.jpg </gallery> {{commonscat}} <br />{{Uranus Footer}} {{sci-stub}} [[Category:Uranus' moons]]