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Uranus (pronounced "YOOR-ə-nus", or "yər-AYN-us") is the seventh planet from the Sun. It is a gas
giant and the third largest by diameter. It was named after the Greek
god Ouranos.
Physical characteristics
Composition
Uranus is composed primarily of rock and various ices, with only about 15% hydrogen and a little helium (in contrast to Jupiter and Saturn which
are mostly hydrogen). Uranus (and Neptune) are in many ways
similar to the cores of Jupiter and Saturn minus the massive liquid metallic hydrogen envelope. It appears that Uranus does not have a rocky core like Jupiter and Saturn but rather that its material is more or less uniformly distributed.
Uranus' cyan color is due to the absorption of red
light by atmospheric methane.
Axial tilt
One of the most distinctive features of Uranus is its axial tilt of almost ninety degrees. Consequently, for part of its orbit
one pole faces the Sun continually whilst the other pole faces away. At the other side of
Uranus' orbit the orientation of the poles towards the sun is reversed, and at the two sections of its orbit between these two
extremes the Sun rises and sets around the equator normally.
At the time of Voyager 2's passage in 1986, Uranus' south pole was pointed almost directly at the Sun. Note that the labelling of this pole as "south" is
actually in some dispute. Uranus can either be described as having an axial tilt of slightly more than 90°, or it can be
described as having an axial tilt of slightly less than 90° and rotating in a retrograde direction; these two descriptions are exactly equivalent as physical descriptions of the
planet but result in different definitions of which pole is the North Pole and
which is the South Pole.
One result of this odd orientation is that the polar regions of Uranus receive a greater energy input from the Sun than its
equatorial regions. Uranus is nevertheless hotter at its equator than at its poles, although the underlying mechanism which
causes this is unknown. The reason for Uranus' extreme axial tilt is also not known. It is speculated that perhaps during the
formation of the planet it collided with an enormous protoplanet, resulting in the skewed orientation.
It appears that Uranus' extreme axial tilt also results in extreme seasonal variations in its weather. During the Voyager 2
flyby, Uranus' banded cloud patterns were extremely bland and faint. Recent Hubble Space Telescope observations, however, show a more strongly banded appearance now that the
Sun is approaching Uranus' equator. By 2007 the Sun will be directly over Uranus'
equator.
Magnetic Field
Uranus' magnetic field is odd in that it is not centered on the
center of the planet and is tilted almost 60° with respect to the axis of rotation. It is probably generated by motion at
relatively shallow depths within Uranus. Neptune has a similarly displaced magnetic field, suggesting that this is not
necessarily a result of Uranus's axial tilt. The magnetotail is twisted
by the planet's rotation into a long corkscrew shape behind the planet. The magnetic field's source is unknown; the electrically
conductive, super-pressurized ocean of water and ammonia once thought to lie between the core and the atmosphere now appears to
be nonexistent.
This crescent view of Uranus was recorded by Voyager 2 on Jan 25, 1986, as the spacecraft left the planet behind.
Exploration of Uranus
Uranus was the first planet to be discovered that was not known in ancient times, although it had been observed on many
previous occasions but was always dismissed as simply another star. (The earliest recorded sighting was in 1690 when John Flamsteed cataloged it as 34 Tauri).
Sir William Herschel discovered the planet in 1781, and originally named it Georgium Sidus (George's Star) in honour of King George III of England. However, this name was not accepted outside of Britain. At the suggestion of Lalande, French astronomers started
calling it Herschel, while the German Johann Bode proposed the name Uranus, after the Greek
god. The latter name was not universally accepted until around 1850.
NASA's Voyager 2 is the only spacecraft to have visited the planet. Launched
in 1977, Voyager made its closest approach to Uranus on January 24, 1986 before continuing on its journey to Neptune.
The moons of Uranus
Uranus has 27 known moons. The first two were discovered by
William Herschel on March
13, 1787, and named, by his son, after characters from Shakespeare's A Midsummer Nights Dream, as Titania and Oberon. Two more moons discovered by
William Lassell in 1851 were
named Ariel and Umbriel; Gerard Kuiper discovered the moon Miranda in 1948. All moons of Uranus
are named after characters from Shakespeare or Alexander Pope.
The flyby of the Voyager 2 space probe in January 1986 led to the discovery of a further 10 moons, and another satellite S/1986 U 10 was later found after studying old
Voyager photographs. Eleven additional moons have since been identified using telescopes.
Uranus has a faint planetary ring system, composed of dark
particulate matter up to 10 metres in diameter. This ring system was discovered in March 1977 by James L.
Elliot, Edward W.
Dunham, and Douglas J.
Mink, using the Kuiper Airborne
Observatory.
Uranus' natural satellites
| Name |
Diameter (km) |
Mass (kg) |
Mean orbital
radius (km) |
Orbital period |
| Cordelia |
40 |
4.5 × 1016 ? |
49,770 |
0.335034 days |
| Ophelia |
42 |
5.4 × 1016 ? |
53,790 |
0.376400 days |
| Bianca |
51 |
9.3 × 1016 ? |
59,170 |
0.434579 days |
| Cressida |
80 |
3.43 × 1017 ? |
61,780 |
0.463570 days |
| Desdemona |
64 |
1.78 × 1017 ? |
62,680 |
0.473650 days |
| Juliet |
93 |
5.57 × 1017 ? |
64,350 |
0.493065 days |
| Portia |
135 |
1.68 × 1018 ? |
66,090 |
0.513196 days |
| Rosalind |
72 |
2.54 × 1017 ? |
69,940 |
0.558460 days |
| S/2003 U2* |
10 |
Unknown |
74,800 |
0.618 days |
| Belinda |
80 |
3.57 × 1017 ? |
75,260 |
0.623527 days |
| S/1986 U10* |
20 |
Unknown |
76,420 |
0.638 days |
| Puck |
162 |
2.89 × 1018 ? |
86,010 |
0.761833 days |
| S/2003 U1* |
10 |
Unknown |
97,734 |
0.923 days |
| Miranda |
472 |
6.6 × 1019 |
129,390 |
1.413479 days |
| Ariel |
1158 |
1.35 × 1021 |
191,020 |
2.520379 days |
| Umbriel |
1170 |
1.17 × 1021 |
266,300 |
4.144177 days |
| Titania |
1578 |
3.52 × 1021 |
435,910 |
8.705872 days |
| Oberon |
1523 |
3.01 × 1021 |
583,520 |
13.463239 days |
| S/2001 U3* |
12 |
Unknown |
4,276,000 |
-266.6 days** |
| Caliban |
98 |
7.3 × 1017 ? |
7,231,000 |
-579.7 days** |
| Stephano |
20 |
6 × 1015 ? |
8,004,000 |
-677.4 days** |
| Trinculo |
10 |
Unknown |
8,504,000 |
-759.0 days** |
| Sycorax |
190 |
5.4 × 1018 ? |
12,179,000 |
-1288.3 days** |
| S/2003 U3* |
11 |
Unknown |
14,345,000 |
1694.8 days |
| Prospero |
30 |
2.1 × 1016 ? |
16,256,000 |
-1977.3 days** |
| Setebos |
30 |
2.1 × 1016 ? |
17,418,000 |
-2234.8 days** |
| S/2001 U2* |
12 |
Unknown |
20,901,000 |
-2823.4 days** |
*Awaiting confirmation and naming
**negative orbital periods indicate a retrograde
orbit around Uranus (opposite to the planet's rotation)
Sources: [1] , [2]
Note: These sources give no information on the masses for the small satellites; some data have changed
greatly so it is unlikely that these old values are correct.
Some asteroids share the same names as moons of Uranus: 171 Ophelia, 218 Bianca, 593 Titania, 666 Desdemona, 2758 Cordelia.
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