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hiphotos195948 Miranda, one of the moons of Uranus, seen from Voyager 2, 24 January 1986. High-resolution image of Miranda, also designated Uranus V, the smallest and innermost of Uranus' five moons, taken from the Voyager unmanned spacecraft from a distance of approximately 31,000 kilometers (19,000 miles), shortly before the spacecraft's closest approach to the Uranian moon. The high resolution of 600 meters (2,000 feet) reveals fractures, grooves and craters, as well as features of different albedos (reflectancea). This view encompasses areas of older, heavily cratered terrain with a wide variety of forms. The grooves and troughs reach depths of a few kilometers (or miles) and expose materials of different albedos. The great variety of directions of fractures and troughs, and the different densities of impact craters on them, signify a long, complex geologic evolution of this satellite.//
DC
hiphotos195982 Miranda, one of the moons of Uranus, seen from Voyager 2, 24 January 1986. High-resolution image of Miranda, also designated Uranus V, the smallest and innermost of Uranus' five moons. The Voyager unmanned spacecraft was approximately 36,000 kilometers (22,000 miles) away from Miranda. This narrow-angle image, part of a mosaicing sequence, shows an area about 250 km (150 miles) across, at a resolution of about 800 meters (2,600 feet). Two distinct terrain types are visible: a rugged, higher-elevation terrain (right) and a lower, striated terrain. Numerous craters on the rugged, higher terrain indicate that it is older than the lower terrain. Several scarps, probably faults, cut the different terrains. The impact crater is about 25 km (15 miles) across.//
DC

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