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Other Moons of Urnaus
The Uranian system contains several smaller, irregular moons that we know very little about. These satellites are extremely small, and many were not discovered until the Voyager 2 encounter with Uranus or by astronomers using the Hubble space telescope. Because of their small size, it is possible that some of these moons may be captured asteroids or comets. These recent discoveries bring the total number of Uranian moons to 21. Below is a listing of the largest of these moons in the order of their orbit from Uranus. Images that appear on this page are the best available at this time. You may also access information on one of the moons by clicking on its name below:

Cordelia
Cordelia is the innermost of Uranus' moons. With a diameter of only 9 miles (15 km), it is one of the smallest moons in the Solar System. It was named after the daughter of Lear in Shakespeare's King Lear. Cordelia was discovered by Voyager 2 in 1986. Not much is known about Cordelia except that it appears to be the inner shepherd satellite for the epsilon ring of Uranus. It is also one of two moons that orbit inside the synchronous orbit radius of Uranus.
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Voyager 2 Image of Cordelia
NASA / JPL |
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Statistics for Cordelia
|
|
| Discovered by...... |
Voyager 2 |
| Year of Discovery...... |
1986 |
| Diameter...... |
16.1 miles (26 km) |
| Mean Distance from Jupiter...... |
30,905 miles (49,750 km) |
| Rotational Period...... |
unknown |
| Orbital Period...... |
0.335 days |
| Orbital Eccentricity...... |
0 |
| Orbital Inclination...... |
0.14 degrees |
| Apparent Magnitude...... |
24.1 |
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Ophelia
Ophelia is the second of Uranus' moons. It was named after the daughter of Polonius in Shakespeare's play, Hamlet. Ophelia was discovered by Voyager 2 in 1986. Not much is known about this moon except that it appears to be the shepherd satellite of Uranus' epsilon ring. It is the second of two moons that orbit inside the synchronous orbit radius of Uranus.
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Voyager 2 Image of Ophelia
NASA / JPL |
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Statistics for Ophelia
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| Discovered by...... |
Voyager 2 |
| Year of Discovery...... |
1986 |
| Diameter...... |
19.8 miles (32 km) |
| Mean Distance from Jupiter...... |
33,396 miles (57,760 km) |
| Rotational Period...... |
unknown |
| Orbital Period...... |
0.376 days |
| Orbital Eccentricity...... |
0.001 |
| Orbital Inclination...... |
0.09 degrees |
| Apparent Magnitude...... |
23.8 |
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Bianca
Bianca is the third of Uranus' moons. It was named after the sister of Katherine in Shakespeare's play, The Taming of the Shrew. Bianca was discovered in 1986 by the Voyager 2 spacecraft. Very little is known about Bianca.
Statistics for Bianca
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| Discovered by...... |
Voyager 2 |
| Year of Discovery...... |
1986 |
| Diameter...... |
27.3 miles (44 km) |
| Mean Distance from Jupiter...... |
36,750 miles (59,160 km) |
| Rotational Period...... |
unknown |
| Orbital Period...... |
0.435 days |
| Orbital Eccentricity...... |
0.001 |
| Orbital Inclination...... |
0.16 degrees |
| Apparent Magnitude...... |
23.0 |
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Cressida
Cressida is the fourth moon of Uranus. It was named after the daughter of Calchas in Shakespeare's play, Troilus and Cressida. Cressida was discovered by Voyager 2 in 1986. Not much is known about Cressida at this time.
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Voyager 2 Image of Cressida
NASA / JPL |
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Statistics for Cressida
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| Discovered by...... |
Voyager 2 |
| Year of Discovery...... |
1986 |
| Diameter...... |
40.9 miles (66 km) |
| Mean Distance from Jupiter...... |
38,372 miles (61,770 km) |
| Rotational Period...... |
unknown |
| Orbital Period...... |
0.464 days |
| Orbital Eccentricity...... |
0.0 |
| Orbital Inclination...... |
1.04 degrees |
| Apparent Magnitude...... |
22.2 |
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Desdemona
Desdemona is the fifth of Uranus' known moons. It was named after the wife of Othello in Shakespeare's play, Othello. This moon was discovered by the Voyager 2 spacecraft in 1986. Little else is known about Othello.
Statistics for Desdemona
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| Discovered by...... |
Voyager 2 |
| Year of Discovery...... |
1986 |
| Diameter...... |
36 miles (58 km) |
| Mean Distance from Jupiter...... |
38,925 miles (62,660 km) |
| Rotational Period...... |
unknown |
| Orbital Period...... |
0.474 days |
| Orbital Eccentricity...... |
0.0 |
| Orbital Inclination...... |
0.16 degrees |
| Apparent Magnitude...... |
22.5 |
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Juliet
Juliet is the sixth moon of Uranus. It was named after the famous and tragic heroine in Shakespeare's play, Romeo and Juliet. Juliet was discovered in 1986 by Voyager 2. Not much else is known about Juliet at this time.
Statistics for Juliet
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| Discovered by...... |
Voyager 2 |
| Year of Discovery...... |
1986 |
| Diameter...... |
52.2 miles (84 km) |
| Mean Distance from Jupiter...... |
39,981 miles (64,360 km) |
| Rotational Period...... |
unknown |
| Orbital Period...... |
0.493 days |
| Orbital Eccentricity...... |
0.001 |
| Orbital Inclination...... |
0.06 degrees |
| Apparent Magnitude...... |
21.5 |
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Portia
Portia is the seventh of Uranus' moons. It was named after a rich heiress in Shakespeare's play, Merchant of Venice. Portia was one of several new moons discovered by Voyager 2 in 1986. Very little is known about Portia.
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Voyager 2 Image of Portia
NASA / JPL |
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Statistics for Portia
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| Discovered by...... |
Voyager 2 |
| Year of Discovery...... |
1986 |
| Diameter...... |
68.3 miles (110 km) |
| Mean Distance from Jupiter...... |
41,062 miles (66,100 km) |
| Rotational Period...... |
unknown |
| Orbital Period...... |
0.513 days |
| Orbital Eccentricity...... |
0.0 |
| Orbital Inclination...... |
0.09 degrees |
| Apparent Magnitude...... |
21.0 |
|

Rosalind
Rosalind is the eighth moon of Uranus. It was named after the daughter of the banished Duke in Shakespeare's play, As You Like It. Rosalind was discovered by the Voyager 2 spacecraft in 1986. Not much is known about Rosalind.
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Voyager 2 Image of Rosalind
NASA / JPL |
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Statistics for Rosalind
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| Discovered by...... |
Voyager 2 |
| Year of Discovery...... |
1986 |
| Diameter...... |
33.5 miles (54 km) |
| Mean Distance from Jupiter...... |
43,441 miles (69,930 km) |
| Rotational Period...... |
unknown |
| Orbital Period...... |
0.559 days |
| Orbital Eccentricity...... |
0.0 |
| Orbital Inclination...... |
0.28 degrees |
| Apparent Magnitude...... |
22.5 |
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Belinda
Belinda is the ninth of Uranus' known moons. It was named after the heroine in Alexander Pope's The Rape of the Lock. Belinda was another of the moons discovered by Voyager 2 in 1986. We know very little about Belinda.
Statistics for Belinda
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| Discovered by...... |
Voyager 2 |
| Year of Discovery...... |
1986 |
| Diameter...... |
42.2 miles (68 km) |
| Mean Distance from Jupiter...... |
46,752 miles (75,260 km) |
| Rotational Period...... |
unknown |
| Orbital Period...... |
0.624 days |
| Orbital Eccentricity...... |
0.0 |
| Orbital Inclination...... |
0.03 degrees |
| Apparent Magnitude...... |
22.1 |
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Puck
Puck is the tenth moon of Uranus. It was named after a mischievous fairy in Shakespeare's play, Midsummer Night's Dream. Puck was discovered in 1986 by the Voyager 2 spacecraft. It was the only new moon discovered early enough in the mission that the observation schedule could be changed in order to get pictures. With an albedo of less than 0.1, Puck is extremely dark. Little else is known about this small moon.
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Voyager 2 Image of Puck
NASA / JPL |
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Statistics for Puck
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| Discovered by...... |
Stephen Synnott |
| Year of Discovery...... |
1985 |
| Diameter...... |
95.6 miles (154 km) |
| Mean Distance from Jupiter...... |
53,430 miles (86,010 km) |
| Rotational Period...... |
unknown |
| Orbital Period...... |
0.762 days |
| Orbital Eccentricity...... |
0.0 |
| Orbital Inclination...... |
0.31 degrees |
| Apparent Magnitude...... |
20.2 |
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Caliban
Caliban [KAL-u-ban] is the sixteenth of Uranus' known moons. It is the smaller of the two moons that have just recently been discovered. The official designation of this moon is Uranus XVI (S/1997 U 1). The name Caliban was chosen by the discoverers and will most likely be accepted by the International Astronomical Union (IAU). It was named after the savage and deformed slave of the magician Prospero in Shakespeare's The Tempest. Caliban was discovered in 1997 by Brett Gladman, Phil Nicholson, Joseph Burns, and JJ Kavelaars using the 200-inch Hale Telescope. It is one of the dimmest moons to have ever been discovered by a ground-based telescope. Very little is known about this moon, due to the recent nature of its discovery. What we do know is that it is about 38 miles (60 km) in diameter and orbits Uranus at a distance of about 4.4 million miles (7.2 million kilometers). Its orbit appears to be retrograde. Astronomers believe that Caliban is probably an asteroid that was captured by the gravity of Uranus. It is probably composed of a mixture of rock and ice. The picture below shows the original image from which Caliban was discovered.
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Discovery Image of Caliban
Brett Gladman, Canadian Institute
for Theoretical Astrophysics |
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Statistics for Caliban
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| Discovered by...... |
Gladman, Nicholson, Burns, & Kavelaars |
| Year of Discovery...... |
1997 |
| Diameter...... |
37.2 miles (60 km) |
| Mean Distance from Jupiter...... |
4,470,000 miles (7,200,000 km) |
| Rotational Period...... |
unknown |
| Orbital Period...... |
579.7 days |
| Orbital Eccentricity...... |
0.159 |
| Orbital Inclination...... |
140.9 degrees |
| Apparent Magnitude...... |
22.4 |
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Sycorax
Sycorax is the seventeenth and outermost of Uranus' known moons. It is the larger of the two moons that have just recently been discovered. The official designation of this moon is Uranus XVII (S/1997 U 2). The name Sycorax was chosen by the discoverers and will most likely be accepted by the International Astronomical Union (IAU). It was named after Caliban's mother, a witch in Shakespeare's The Tempest. In the story, she imprisoned the fairy Ariel for disobedience. Sycorax was discovered in 1997 by Brett Gladman, Phil Nicholson, Joseph Burns, and JJ Kavelaars using the 200-inch Hale Telescope. It is one of the dimmest moons to have ever been discovered by a ground-based telescope. Very little is known about this moon, due to the recent nature of its discovery. What we do know is that it is about 75 miles (120 km) in diameter and orbits Uranus at a distance of about 7.6 million miles (12.2 million kilometers). Its orbit appears to be retrograde. Astronomers believe that Sycorax is probably a captured asteroid. It is thought to be composed of a mixture of rock and ice. The picture below shows the original image from which Sycorax was discovered.
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Discovery Image of Caliban
Brett Gladman, Canadian Institute
for Theoretical Astrophysics |
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Statistics for Sycorax
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| Discovered by...... |
Gladman, Nicholson, Burns, & Kavelaars |
| Year of Discovery...... |
1997 |
| Diameter...... |
75 miles (120 km) |
| Mean Distance from Jupiter...... |
7,580,000 miles (12,200,000 km) |
| Rotational Period...... |
unknown |
| Orbital Period...... |
1288.3 |
| Orbital Eccentricity...... |
0.522 |
| Orbital Inclination...... |
159.4 degrees |
| Apparent Magnitude...... |
20.8 |
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