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Montage of Uranus five largest satellites taken by NASA Voyager 2. From to right to left in order of decreasing distance from Uranus are Oberon, Titania, Umbriel, Ariel, and Miranda.
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During its routine yearly monitoring of the weather on our solar system's outer planets, NASA's Hubble Space Telescope has uncovered a new mysterious dark storm on Neptune (right) and provided a fresh look at a long-lived storm circling around the north polar…
Ver en NASA ↗On Jan. 18, 1986, NASA Voyager 2 discoverd three Uranus satellites. All three lie outside the orbits of Uranus nine known rings, the outermost of which, the epsilon ring, is seen at upper right.
Ver en NASA ↗P-29499 Rings of Uranus
Ver en NASA ↗This view from NASA's Cassini spacecraft features a blue planet, Uranus, imaged by Cassini for the first time. Uranus is a pale blue in this natural color image because its visible atmosphere contains methane gas and few aerosols or clouds.
Ver en NASA ↗This silhouetted image of the rings of Uranus was taken by NASA Voyager 2 spacecraft on Jan. 24, 1986, just 27 minutes before its closest approach to the planet.
Ver en NASA ↗NASA Voyager 2 took this wide-angle image of Uranus rings as the spacecraft neared the plane of the rings less than an hour before closest approach to the planet.
Ver en NASA ↗An infrared composite image of the two hemispheres of Uranus obtained with Keck Telescope adaptive optics.
Ver en NASA ↗Uranus rings, photographed by NASA Voyager 2 in 1986 as it approached the plane of the Uranian ring system.
Ver en NASA ↗P29501C Moon from Voyager 2 Uranus flyby
Ver en NASA ↗P-29507 Rings Voyager 2 flyby of Uranus
Ver en NASA ↗NASA Voyager 2 returned this picture of the Uranus rings on Jan. 22, 1986, from a distance of 2.52 million kilometers 1.56 million miles. All nine known rings are visible in this image.
Ver en NASA ↗P-25517 3 UP COMPOSITE Voyager 2 and Uranus
Ver en NASA ↗The terminator region of Titania, one of Uranus five large moons, was captured in this Voyager 2 image obtained in the early morning hours of Jan. 24, 1986.
Ver en NASA ↗Miranda, innermost of Uranus large satellites, is seen at close range in this Voyager 2 image, taken Jan. 24, 1986, as part of a high-resolution mosaicing sequence.
Ver en NASA ↗NASA scientists have made the first observation of a polar cyclone on Uranus.
Ver en NASA ↗This family portrait of Uranus five largest moons was compiled from images sent back Jan. 20, 1986, by NASA Voyager 2 spacecraft. Even in these distant views, the satellites exhibit distinct differences in appearance.
Ver en NASA ↗Voyager 2 has discovered two hepherd satellites associated with the rings of Uranus. The two moons, designated 1986U7 and 1986U8, are seen here on either side of the bright epsilon ring; all nine of the known Uranian rings are visible.
Ver en NASA ↗The outer rings of Uranus are visible in this image, obtained by NASA Voyager 2 on Jan. 23, 1986. The outermost and brightest ring, called epsilon, is visible along with the fainter and narrower delta and gamma rings from left.
Ver en NASA ↗This Voyager 2 image of Miranda was taken Jan. 23, 1986, as the spacecraft neared Uranus. Miranda is the innermost of the five Uranian satellites known from Earth-based observations.
Ver en NASA ↗NASA Voyager 2 acquired this high-resolution image of the epsilon ring of Uranus on Jan. 23, 1986. This clear-filter image from Voyager narrow-angle camera has a resolution of about 10 km 6 mi.
Ver en NASA ↗On Jan. 23, 1986, NASA Voyager 2 discovered a tenth ring orbiting Uranus. The tenth ring is about midway between the bright, outermost epsilon ring and the next ring down, called delta.
Ver en NASA ↗This image captured by NASA Voyager 2 in 1986 revealed a continuous distribution of small particles throughout the Uranus ring system. This unique geometry, the highest phase angle at which Voyager imaged the rings, allowed us to see lanes of fine dust.
Ver en NASA ↗This false-color view of the rings of Uranus was made from images taken by NASA Voyager 2 on Jan. 21, 1986. All nine known rings are visible here; the somewhat fainter, pastel lines seen between them are contributed by the computer enhancement.
Ver en NASA ↗Contenido y metadatos proporcionados por la NASA Image and Video Library.