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Uranus: Moons and Rings |
Moons
Uranus’s moons have had a long and tangled history. The first two moons, Titania and Oberon, were discovered in 1787 by the man who had discovered Uranus six years earlier, William Herschel. He named them after the king and queen of fairies in Shakespeare’s A Midsummer Night’s Dream, provoking a protest from the German ambassador (among others) who felt that the satellites should be given a more international and classical name. The name stuck, however, and now all of the moons of Uranus have been given the names of characters drawn from the works of either Shakespeare or Pope.
Naming the moons of Uranus, however, proved less troublesome than keeping track of them. Most are so small that they cannot be detected from Earth. Scientists were tracking the small satellites until the Hubble Space Telescope could be launched. But by the time Hubble sighted Uranus, Ophelia and Cordelia were lost. Due to the influence these moons exerted on the rings, however, they were eventually found again. A decade later, scientists going over the pictures taken by Voyager 2 discovered another moon. Several years later another was found. Now Uranus boasts 21 moons—five more than the leading contender, Saturn, which has fifteen. It is likely that at least one more small satellite is still hiding somewhere in the complicated web of moons and rings that encircle Uranus. In order from the planet, the satellites are 1999U3 (still unnamed), Cordelia, Ophelia, Bianca, Cressida, Desdemona, Juliet, Portia, Rosalind, Belinda, 1986U10 (still unnamed), Puck, Miranda, Ariel, Umbriel, Titania, Oberon, Caliban, and 1999U2 (still unnamed).
| Name |
Distance (km) |
Radius (km) |
Mass (kg) |
Discoverer (Year) |
| 1986U10 |
75,000 |
20 |
Unknown |
Karkoschka (1999) |
| 1999U1 |
10,000,000 |
20 |
Unknown |
Kavelaars |
| 1999U2 |
25,000,000 |
15 |
Unknown |
Gladman (1999) |
| 1999U3 |
20,000 |
Unknown |
Unknown |
Holman (1999) |
| Ariel |
191,000 |
579 |
1.27 x 1021 |
Lassell (1985) |
| Belinda |
75,000 |
34 |
Unknown |
Voyager (1986) |
| Bianca |
59,000 |
22 |
Unknown |
Voyager (1986) |
| Caliban |
7,100,000 |
30 |
Unknown |
Gladman (1997) |
| Cordelia |
50,000 |
13 |
Unknown |
Voyager (1986) |
| Cressida |
62,000 |
33 |
Unknown |
Voyager (1986) |
| Desdemona |
63,000 |
29 |
Unknown |
Voyager (1986) |
| Juliet |
64,000 |
42 |
Unknown |
Voyager (1986) |
| Miranda |
130,000 |
236 |
6.30 x 1019 |
Kuiper (1948) |
| Oberon |
583,000 |
761 |
3.03 x 1021 |
Herschel (1787) |
| Ophelia |
54,000 |
16 |
Unknown |
Voyager (1986) |
| Portia |
66,000 |
55 |
Unknown |
Voyager (1986) |
| Puck |
86,000 |
77 |
Unknown |
Voyager (1986) |
| Rosalind |
70,000 |
27 |
Unknown |
Voyager (1986) |
| Sycorax |
12,200,000 |
60 |
Unknown |
Nicholson (1997) |
| Titania |
436,000 |
789 |
3.49 x 1021 |
Herschel (1787) |
| Umbriel |
266,000 |
585 |
1.27 x 1021 |
Lassell (1851) |
 Rings
Voyager 2 discovered Uranus’s faint rings. Interestingly enough, two of the moons that the probe discovered, Cordelia and Ophelia, have some part in maintaining them. They are “shepherd” moons that keep the constituent particles of the ring in tight order. Cordelia and Ophelia maintain the epsilon ring.
Copyright © 2000 by Gary Chan and Matthew McDermott. All rights reserved.
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