Missions to Uranus
| Mission |
Country |
Launch Date |
Arrival Date |
Type |
Encounter Characteristics |
|
| Voyager 2 |
USA |
August 20, 1977 |
January 24, 1986 |
Flyby |
7000 images of Uranus, its rings, and its satellites |
An Overview of Space Exploration
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The bland aquamarine face of Uranus bears witness to the fact that Uranus is enshrouded in clouds. The planet appears to be blue-green because the atmosphere absorbs the red wavelengths of the visible
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Uranus has // Call the moon count function defined in the document head print_moon_count('uranus'); fascinating moons and a complicated ring system. The ring system is a completely different form of ring
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The Giant planets do not have the same kind of structure inside that the terrestrial planets do. Their evolution was quite different than that of the terrestrial planets, and they have much more gas and
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Uranus is the tilted planet. Its spin axis, which defines the locations of its North and South Poles, is tilted almost 98° away from the "upright" direction perpendicular to its orbital plane. In other
...moreAtmospheres of the giant planets have definitely evolved from their formation out of the primitive solar nebula. How much they have evolved remains to be seen, however. Because of their enormous gravity,
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The major gaseous constituent of the atmosphere is methane. At the uppermost reaches of the atmosphere, near the thermosphere, methane gas breaks apart due to the influence of energetic photons or charged
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Motions in the atmosphere include wind. The major winds in the Uranian atmosphere are the zonal winds which consist of westward flowing zones and eastward flowing belts. The other major means of motion
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This is the temperature profile of Uranus' entire atmosphere. The horizontal lines indicate the boundaries between the troposphere, the stratosphere, the mesosphere, and the thermosphere.
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