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Uranus
[General] [History] [Satellites]
[Rings] [Unknowns]
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PHYSICAL
DATA
- Sidereal period:
84.01 years
- Rotation period:
17.2 hours
- Mean orbital velocity: 6.80
km/s
- Mass (Earth is 1):
14.6
- Volume (Earth is 1):
67
- Mean Surface Temp: -210°C
- Distance from Sun: 2,735 to
3,004 million km
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Uranus wasn't discovered
until the 18th century. In 1781, William Herschel (1738-1822)
discovered Uranus. Six years later, Herschel found two of its
largest moons. Uranus is a gas planet, composed mostly of
hydrogen (83%) and helium (15%). It gets its blue color because
methane (which represents about 2% of the planet) absorbs red
light.
General
Uranus is a giant gas planet. It has a large diameter
and low density. Like Jupiter and Saturn, Uranus has a layered
atmosphere, high winds, and lots of hydrogen. On the other hand,
its winds are not as high, its atmospheric bands are not bold and
colorful, and it might have more rock in it than either Jupiter
and Saturn.
Aside from its color (see true and
false colors of Uranus, right), Uranus is best known for lying on
its side. It's possible a large planet-sized object collided with
it and tipped Uranus over. In any case, it is tilted almost
ninety degrees, making it difficult to say which is its north and
south poles. Either, its tilted 98 degrees and has a direct
rotation pattern rotation and is tilted by 88 degrees. Interestingly,
Uranus' original south pole points directly at the Sun but the
hottest area on the planet is around its equator. Puzzling. or it
has a retrograde
Uranus is about four times bigger than Earth (left). Located
2.9 billion miles from the Sun, it takes Uranus 84 years to
complete its circuit. Like the other gas planets, Uranus has
rings (but they are dark) and lots of moons (10 small ones and 5
large ones). It also has an extensive magnetic field that sort of
corkscrews behind the planet.
History
Unlike most planets, who were named for
Roman gods, Uranus was named from Greek mythology. According to
Greek lore, Uranus was the god of the sky and king of the other
gods. Originally thought to be a star, Uranus was call 34 Tauri.
When the English astronomer William Herschel (1738-1822)
discovered the planet, he wanted to name it after King George.
But ultimately it was decided to keep the theme of naming planets
after mythological figures.
Only one spacecraft has visited Uranus. Voyager 2, on its way
to Neptune, passed Uranus in 1986.
Satellites
Like Jupiter and Saturn, Uranus has many satellites. So
far there are 15 named moons and 2 newly discovered ones. Named
for literary characters (mostly Shakespeare), the five outer
satellites (right) were discovered before Voyager 2. Oberon and
Titania were discovered in 1787, and Umbriel and Ariel were
found in 1851. But Miranda wasn't discovered until 1948. The
inner moons, which are dark and small, were discovered by Voyager
2 in 1985-86. All the satellites have nearly circular
orbits.
| Satellite |
Distance |
Radius |
Mass |
Discovered By |
Year |
| Cordelia |
50 km |
13 km |
? |
Voyager 2 |
1986 |
| Ophelia |
54 km |
16 km |
? |
Voyager 2 |
1986 |
| Bianca |
59 km |
22 km |
? |
Voyager 2 |
1986 |
| Cressida |
62 km |
33 km |
? |
Voyager 2 |
1986 |
| Desdemona |
63 km |
29 km |
? |
Voyager 2 |
1986 |
| Juliet |
64 km |
42 km |
? |
Voyager 2 |
1986 |
| Portia |
66 km |
55 km |
? |
Voyager 2 |
1986 |
| Rosalind |
70 km |
27 km |
? |
Voyager 2 |
1986 |
| Belinda |
75 km |
34 km |
? |
Voyager 2 |
1986 |
| 1986u10 |
75 km |
20 km |
? |
Karkoschka |
1999 |
| Puck |
86 km |
77 km |
? |
Voyager 2 |
1985 |
| Miranda |
130 km |
236 km |
6.30 x 1019
kg |
Kuiper |
1948 |
| Ariel |
191 km |
579 km |
1.27 x 1021
kg |
Lassell |
1851 |
| Umbriel |
266 km |
585 km |
1.27 x 1021
kg |
Lassell |
1851 |
| Titania |
436 km |
789 km |
3.49 x 1021
kg |
Herschel |
1787 |
| Oberon |
583 km |
761 km |
3.03 x 1021
kg |
Herschel |
1787 |
| Caliban (proposed) |
7,200 km |
30 km |
? |
Gladman |
1997 |
| Sycorax (proposed) |
12,200 km |
60 km |
? |
Gladman |
1997 |
Rings
Uranus has rings (see right), just like the other gas
planets, but they are more difficult to detect and in fact
weren't discovered until 1977. The outer ring, Epsilon, is made
mostly of blocks of ice so it is the brightest ring. The other 10
rings tend to be darker and have more dust and rock material in
them. Two of Uranus's moons can be seen straddling the Epsilon
ring (below).
| Ring |
Distance |
Width |
| 1986u2R |
38,000 km |
2,500 km |
| 6 |
41,840 km |
1-3 km |
| 5 |
42,230 km |
2-3 km |
| 4 |
42,580 km |
2-3 km |
| Alpha |
44,720 km |
7-12 km |
| Beta |
45,670 km |
7-12 km |
| Eta |
47,190 km |
0-2 km |
| Gamma |
47,630 km |
1-4 km |
| Delta |
48,290 km |
3-9 km |
| 1986U1R |
50,020 km |
1-2 km |
| Epsilon |
51,140 km |
20-100 km |
* Distance is from the center of Uranus to the
inner edge of the ring.
Unknowns
- Was Uranus, like Jupiter, on its way to being a star but
never grew up?
- Why does its south pole face toward the Sun?
- What is its interior like?
- Why is Uranus at such a strange tilted axis tilted?
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Next Topic: Neptune
[General] [History] [Satellites]
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