URANUS, major planetin the solar system, equivalent in brightness to a sixth-magnitude star. It ranks seventh in order of distance from the sun, revolving outside the orbit of Saturn
and inside the orbit of Neptune. Uranus was accidentally discovered in
1781 by the British astronomer Sir William Herschel and was originally
named the Georgium Sidus (Star of George) in honor of his royal patron
King George III of Great Britain. The planet was later, for a time,
called Herschel in honor of its discoverer. The name Uranus, which was first proposed by the German astronomer Johann Elert Bode (1747-1826), was in use by the late 19th century.
Uranus has an equatorial radius of 25,559 km (15,882
mi), and its average distance from the sun is 2,870,972,200 km
(1,783,939,400 mi). Uranus takes 84.02 earth years for a single
revolution, or orbit, around the sun and 17.24 hr to complete a
rotation about its axis; the direction of rotation is retrograde
(opposite to that of earth). Uranus's atmosphere consists largely of
hydrogen and helium, with a trace of methane. Through a telescope the
planet appears as a small, bluish-green disk with a faint green
periphery. Compared to the earth, Uranus has a mass 14.371 times
greater and a volume 63.1 times greater. The magnetic field of Uranus
has its axis tilted 59° from the rotational axis and appears to exhibit
other significant anomalies.
| BRIEF SURVEY OF URANUS |
| Distance from Sun |
|
| Perihelion (closest) |
2,735,560,000 km (1,699,800,000 mi) |
| Aphelion |
3,006,390,000 km (1,868,080,000 mi) |
| Distance from Earth |
|
| Minimum |
2,581,900,000 km (1,604,300,000 mi) |
| Maximum |
3,157,300,000 km (1,961,900,000 mi) |
| Period of revolution |
84.02 earth years |
| Rotation period (sidereal day) |
17.24 hr (retrograde) |
| Eccentricity of orbit |
0.047 |
| Inclination of orbit |
0.77° |
| Mass (earth = 1) |
14.371 |
| Radius at equator |
25,559 km (15,882 mi) |
| Mean density (earth = 1) |
0.236 |
| Surface gravity (earth = 1) |
0.86 |
| Atmospheric pressure at surface (earth = 1) |
>1000 bars |
| Effective temperature |
-216° C (-357° F) |
| Known natural satellites (as of Feb. 2004) |
27 |
Uranus has 11 rings, known (in increasing order of
distance from the planet) as 1986U2R, 6, 5, 4, Alpha, Beta, Eta, Gamma,
Delta, Lambda, and Epsilon. These rings form a belt with a width of
about 13,150 km (about 8170 mi), extending from about 38,000 km (23,610
mi) to 51,150 km (31,780 mi) from the planet's center. Nine of these
rings were discovered in 1977. While recording the occultation of a
star behind the planet, the American astronomer James L. Elliot
(1943- ), working with a team from the Kuiper
Airborne Observatory of the National Aeronautics and Space
Administration (NASA), discovered the presence of what were eventually
identified as six rings encircling the equator of Uranus; three more
rings were identified by a team at the Perth Observatory in Australia.
In January 1986, during the exploratory flight of NASA's Voyager 2, these nine rings were photographed and measured, as were two new ones.
| Principal Satellites of Uranus |
| Name |
Mean distance from Neptune |
Diameter |
| Cordelia |
49,800 km (30,900 mi) |
40 km (25 mi) |
| Ophelia |
53,800 km (33,400 mi) |
42 km (26 mi) |
| Bianca |
59,200 km (36,800 mi) |
51 km (32 mi) |
| Cressida |
61,800 km (38,400 mi) |
80 km (50 mi) |
| Desdemona |
62,700 km (39,000 mi) |
64 km (40 mi) |
| Juliet |
64,400 km (40,000 mi) |
93 km (58 mi) |
| Portia |
66,100 km (41,100 mi) |
135 km (84 mi) |
| Rosalind |
69,900 km (43,400 mi) |
72 km (45 mi) |
| Belinda |
75,300 km (46,800 mi) |
80 km (50 mi) |
| Puck |
86,000 km (53,400 mi) |
162 km (101 mi) |
| Miranda |
129,900 km (80,700 mi) |
471 km (293 mi) |
| Ariel |
190,900 km (118,600 mi) |
1158 km (720 mi) |
| Umbriel |
266,000 km (165,300 mi) |
1169 km (726 mi) |
| Titania |
436,300 km (271,100 mi) |
1578 km (981 mi) |
| Oberon |
583,500 km (362,600 mi) |
1522 km (946 mi) |
| Caliban |
7,231,000 km (4,493,000 mi) |
98 km (61 mi) |
| Sycorax |
12,179,000 km (7,568,000 mi) |
190 km (118 mi) |
In addition to its rings, Uranus has at least 27
satellites. The two largest moons, Oberon and Titania, were discovered
by Herschel in 1787. The next two, Umbriel and Ariel, were found in
1851 by the British astronomer William Lassell (1799-1880). Miranda,
thought before Voyager 2's flyby in 1986 to be the innermost
moon, was discovered in 1948 by the American astronomer Gerard Peter
Kuiper. Ten smaller satellites-Cordelia, Ophelia, Bianca, Cressida,
Desdemona, Juliet, Portia, Rosalind, Belinda, and Puck-were revealed by
Voyager 2 in 1985-86, along with a much smaller moon
provisionally identified as S/1986 U10. The spacecraft also recorded
surface details of the large, previously discovered moons, including
Oberon's cratered surface, Titania's rifts and fractures, Miranda's
grooved markings, and evidence of flow on Ariel. Eleven additional
satellites were identified by astronomers from 1997 through 2003.