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Voyager 2 encounters with Uranus and Neptune. August 25 th , 1989. January 24 th , 1986. August 25 th , 1989. The English astronomer, William Herschel, discovered Uranus in 1781. McDonald Observatory image of Uranus and some of its moons. *. *. *. *. *. *. *.
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Voyager 2 encounters with Uranus and Neptune August 25th, 1989 January 24th, 1986 August 25th, 1989
The English astronomer, William Herschel, discovered Uranus in 1781
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Uranus is the only planet whose axis of rotation lies in its orbital plane (tilt of 98°), probably caused by a large impact.
Comparison of the densities and compositions of the Jovian planets
Approach of Viking 2 on July 15, 1985 of Uranus and 4 of its moons (composite).
False color (left) and true color images of Uranus, taken by Viking 2
Some of the rings of Uranus, discovered by the Viking spacecraft
Rings of the planet Uranus, with two shepherd moons which keep the ring particles in place, discovered by the Viking spacecraft
Continuous distribution of small particles throughout the ring system of Uranus. Picture taken while the Viking spacecraft was in the shadow of Uranus. These dust lanes were previously unknown. 96 second exposure, hence, background stars form streaks.
Epsilon ring of Uranus, and three of the moons discovered by the Viking spacecraft
5 km high scarp on Miranda – Miranda may have split apart and reassembled
Umbriel - 1,168 km in diameter Resolution of this Viking image is ~ 10 km. Umbriel is highly cratered, particularly on its southern hemisphere (right). It is the darkest moon of Uranus, with an albedo of ~ 16 %, like our moon. It also is the moon with lowest internally-generated geologic activity. The bright spot at the top of the image (near the equator) may be frost.
Titania – 1,580 in diameter; heavily cratered but also has long scarps
Oberon – 1,520 km in diameter; bright surface markings, many impact craters