Named for a Shakespearean queen, which is the largest of the moons of Uranus?
"and ""The Rape of the Lock"" (although at present only Ariel, Umbriel, and Belinda have names drawn from the latter; all the rest are from Shakespeare). At first, the outermost moons were all named after characters from one play, ""The Tempest""; but with Margaret being named from ""Much Ado About Nothing"" that trend has ended. Some asteroids share names with moons of Uranus: 171 Ophelia, 218 Bianca, 593 Titania, 666 Desdemona, 763 Cupido, and 2758 Cordelia. The Uranian satellite system is the least massive among those of the giant planets. Indeed, the combined mass of the five major satellites is"
"low for crater with such a large diameter indicating that the relief has relaxed since the impact. The surface of the dome has only few superimposed smaller craters, which means that it was modified later. Gertrude (crater) Gertrude is the largest known crater on Uranus's moon Titania. It is about 326 km across, 1/5 of Titania's diameter. It is named after the mother of Hamlet in William Shakespeare's play ""Hamlet"". Features on Titania are named after female Shakespearean characters. The crater rim of Gertrude is elevated by 2 km over the crater floor. In the center of the crater there"
"Gertrude (crater) Gertrude is the largest known crater on Uranus's moon Titania. It is about 326 km across, 1/5 of Titania's diameter. It is named after the mother of Hamlet in William Shakespeare's play ""Hamlet"". Features on Titania are named after female Shakespearean characters. The crater rim of Gertrude is elevated by 2 km over the crater floor. In the center of the crater there is a large dome, which resulted from the uplift of the surface immediately after the impact. The dome has the diameter of about 150 km and is 2–3 km high. The rim and dome are"
"Oberon (moon) Oberon, also designated , is the outermost major moon of the planet Uranus. It is the second-largest and second most massive of the Uranian moons, and the ninth most massive moon in the Solar System. Discovered by William Herschel in 1787, Oberon is named after the mythical king of the fairies who appears as a character in Shakespeare's ""A Midsummer Night's Dream"". Its orbit lies partially outside Uranus's magnetosphere. It is likely that Oberon formed from the accretion disk that surrounded Uranus just after the planet's formation. The moon consists of approximately equal amounts of ice and rock,"
"about 40% of its surface. Titania was discovered by William Herschel on January 11, 1787, the same day he discovered Uranus's second largest moon, Oberon. He later reported the discoveries of four more satellites, although they were subsequently revealed as spurious. For nearly fifty years following their discovery, Titania and Oberon would not be observed by any instrument other than William Herschel's, although the moon can be seen from Earth with a present-day high-end amateur telescope. All of Uranus's moons are named after characters created by William Shakespeare or Alexander Pope. The name Titania was taken from the Queen of"
"notes Citations Sources Puck (moon) Puck ( ) is an inner moon of Uranus. It was discovered in December 1985 by the ""Voyager 2"" spacecraft. The name ""Puck"" follows the convention of naming Uranus's moons after characters from Shakespeare. The orbit of Puck lies between the rings of Uranus and the first of Uranus's large moons, Miranda. Puck is approximately spherical in shape and has diameter of about 162 km. It has a dark, heavily cratered surface, which shows spectral signs of water ice. Puck—the largest inner moon of Uranus—was discovered from the images taken by ""Voyager 2"" on 30"
"Puck (moon) Puck ( ) is an inner moon of Uranus. It was discovered in December 1985 by the ""Voyager 2"" spacecraft. The name ""Puck"" follows the convention of naming Uranus's moons after characters from Shakespeare. The orbit of Puck lies between the rings of Uranus and the first of Uranus's large moons, Miranda. Puck is approximately spherical in shape and has diameter of about 162 km. It has a dark, heavily cratered surface, which shows spectral signs of water ice. Puck—the largest inner moon of Uranus—was discovered from the images taken by ""Voyager 2"" on 30 December 1985. It"
"Moons of Uranus Uranus is the seventh planet of the Solar System; it has 27 known moons, all of which are named after characters from the works of William Shakespeare and Alexander Pope. Uranus's moons are divided into three groups: thirteen inner moons, five major moons, and nine irregular moons. The inner moons are small dark bodies that share common properties and origins with Uranus's rings. The five major moons are massive enough to have reached hydrostatic equilibrium, and four of them show signs of internally driven processes such as canyon formation and volcanism on their surfaces. The largest of"
"was given the temporary designation S/1985 U 1. The moon was later named after the character Puck who appears in Shakespeare's ""A Midsummer Night's Dream"", a little sprite who travels around the globe at night with the fairies. In Celtic mythology and English folklore, a ""Puck"" is a mischievous sprite, imagined as an evil demon by Christians. It is also designated Uranus XV. Puck is the largest small inner moon of Uranus, which orbits inside the orbit of Miranda. It is intermediate in size between Portia (the second-largest inner moon) and Miranda (the smallest of the five large classical moons)."
"Ophelia (moon) Ophelia ( ) is a moon of Uranus. It was discovered from the images taken by ""Voyager 2"" on January 20, 1986, and was given the temporary designation S/1986 U 8. It was not seen until the Hubble Space Telescope recovered it in 2003. Ophelia was named after the daughter of Polonius, Ophelia, in William Shakespeare's play ""Hamlet"". It is also designated Uranus VII. Other than its orbit, radius of 21 km and geometric albedo of 0.08 virtually nothing is known about it. At the Voyager 2 images Ophelia appears as an elongated object, the major axis pointing"
"of energy. Possible capture processes include gas drag in the protoplanetary disk and many-body interactions and capture during the fast growth of Uranus's mass (so called ""pull-down""). Sycorax (moon) Sycorax ( ) is the largest retrograde irregular satellite of Uranus. Sycorax was discovered on 6 September 1997 by Brett J. Gladman, Philip D. Nicholson, Joseph A. Burns, and John J. Kavelaars using the 200-inch Hale telescope, together with Caliban, and given the temporary designation S/1997 U 2. Officially confirmed as Uranus XVII, it was named after Sycorax, Caliban's mother in William Shakespeare's play ""The Tempest"". Sycorax follows a distant orbit,"
"Portia (moon) Portia ( ) is an inner satellite of Uranus. It was discovered from the images taken by ""Voyager 2"" on 3 January 1986, and was given the temporary designation S/1986 U 1. The moon is named after Portia, the heroine of William Shakespeare's play ""The Merchant of Venice"". It is also designated Uranus XII. Portia is the second-largest inner satellite of Uranus after Puck. The Portian orbit, which lies inside Uranus' synchronous orbital radius, is slowly decaying due to tidal deceleration. The moon will one day either break up into a planetary ring or hit Uranus. It heads"
"Portia. Explanatory notes Citations Portia (moon) Portia ( ) is an inner satellite of Uranus. It was discovered from the images taken by ""Voyager 2"" on 3 January 1986, and was given the temporary designation S/1986 U 1. The moon is named after Portia, the heroine of William Shakespeare's play ""The Merchant of Venice"". It is also designated Uranus XII. Portia is the second-largest inner satellite of Uranus after Puck. The Portian orbit, which lies inside Uranus' synchronous orbital radius, is slowly decaying due to tidal deceleration. The moon will one day either break up into a planetary ring or"
"Mab (moon) Mab ( ), or Uranus XXVI (26), is an inner satellite of Uranus. It was discovered by Mark R. Showalter and Jack J. Lissauer in 2003 using the Hubble Space Telescope. It was named after Queen Mab, a fairy queen from English folklore who is mentioned in William Shakespeare's play ""Romeo and Juliet"". Because the moon is small and dark, it was not seen in the heavily scrutinized images taken by ""Voyager 2"" during its Uranus flyby in 1986. However, it is brighter than another moon, Perdita, which was discovered from Voyager's photos in 1997. This led scientists"
"by William Lassell on 24 October 1851. Although William Herschel, who discovered Uranus's two largest moons Titania and Oberon in 1787, claimed to have observed four additional moons, this was never confirmed and those four objects are now thought to be spurious. All of Uranus's moons are named after characters from the works of William Shakespeare or Alexander Pope's ""The Rape of the Lock"". The names of all four satellites of Uranus then known were suggested by John Herschel in 1852 at the request of Lassell. Ariel is named after the leading sylph in ""The Rape of the Lock"". It"
"Tempest"", because the four previously discovered moons of Uranus, Ariel, Umbriel, Titania and Oberon, had all been named after characters of Shakespeare or Alexander Pope. However, the previous moons had been named specifically after fairies, whereas Miranda was a human. Subsequently, discovered satellites of Uranus were named after characters from Shakespeare and Pope, whether fairies or not. The moon is also designated Uranus V. Of Uranus's five round satellites, Miranda orbits closest to it, at roughly 129,000 km from the surface; about a quarter again as far as its most distant ring. Its orbital period is 34 hours, and, like"
"Sycorax (moon) Sycorax ( ) is the largest retrograde irregular satellite of Uranus. Sycorax was discovered on 6 September 1997 by Brett J. Gladman, Philip D. Nicholson, Joseph A. Burns, and John J. Kavelaars using the 200-inch Hale telescope, together with Caliban, and given the temporary designation S/1997 U 2. Officially confirmed as Uranus XVII, it was named after Sycorax, Caliban's mother in William Shakespeare's play ""The Tempest"". Sycorax follows a distant orbit, more than 20 times further from Uranus than the furthest regular moon, Oberon. Its orbit is retrograde, moderately inclined and eccentric. The orbital parameters suggest that it"
"Juliet (moon) Juliet ( , ) is an inner satellite of Uranus. It was discovered from the images taken by ""Voyager 2"" on 3 January 1986, and was given the temporary designation S/1986 U 2. It is named after the heroine of William Shakespeare's play ""Romeo and Juliet"". It is also designated Uranus XI. Juliet belongs to Portia Group of satellites, which also includes Bianca, Cressida, Desdemona, Portia, Rosalind, Cupid, Belinda and Perdita. These satellites have similar orbits and photometric properties. Unfortunately, other than its orbit, radius of 53 km and geometric albedo of 0.08 virtually nothing is known about"
"Juliet. At the Voyager 2 images Juliet appears as an elongated object, the major axis pointing towards Uranus. The ratio of axes of Juliet's prolate spheroid is 0.5 ± 0.3, which is rather an extreme value. Its surface is grey in color. Juliet may collide with Desdemona within the next 100 million years. Explanatory notes Citations Juliet (moon) Juliet ( , ) is an inner satellite of Uranus. It was discovered from the images taken by ""Voyager 2"" on 3 January 1986, and was given the temporary designation S/1986 U 2. It is named after the heroine of William Shakespeare's"
"for which the mass has been directly measured. Cressida may collide with Desdemona within the next 100 million years. Explanatory notes Citations Cressida (moon) Cressida ( , ) is an inner satellite of Uranus. It was discovered from the images taken by ""Voyager 2"" on 9 January 1986, and was given the temporary designation S/1986 U 3. It was named after Cressida, the Trojan daughter of Calchas, a tragic heroine who appears in William Shakespeare's play ""Troilus and Cressida"" (as well as in tales by Geoffrey Chaucer and others). It is also designated Uranus IX. Cressida belongs to the Portia"
"Rosalind (moon) Rosalind ( ) is an inner satellite of Uranus. It was discovered from the images taken by ""Voyager 2"" on 13 January 1986, and was given the temporary designation S/1986 U 4. It was named after the daughter of the banished Duke in William Shakespeare's play ""As You Like It"". It is also designated Uranus XIII. Rosalind belongs to Portia group of satellites, which also includes Bianca, Cressida, Desdemona, Portia, Juliet, Cupid, Belinda and Perdita. These satellites have similar orbits and photometric properties. Other than its orbit, radius of 36 km and geometric albedo of 0.08 virtually nothing"
"Bianca (moon) Bianca ( ) is an inner satellite of Uranus. It was discovered from the images taken by ""Voyager 2"" on January 23, 1986, and was given the temporary designation S/1986 U 9. It was named after the sister of Katherine in Shakespeare's play ""The Taming of the Shrew"". It is also designated Uranus VIII. Bianca belongs to Portia Group of satellites, which also includes Cressida, Desdemona, Juliet, Portia, Rosalind, Cupid, Belinda and Perdita. These satellites have similar orbits and photometric properties. Other than its orbit, radius of 27 km, and geometric albedo of 0.08 virtually nothing is known"
"is known about Rosalind. In the Voyager 2 images Rosalind appears as an almost spherical object. The ratio of axes of Rosalind's prolate spheroid is 0.8-1.0. Its surface is grey in color. Rosalind is very close to a 3:5 orbital resonance with Cordelia. Explanatory notes Citations Rosalind (moon) Rosalind ( ) is an inner satellite of Uranus. It was discovered from the images taken by ""Voyager 2"" on 13 January 1986, and was given the temporary designation S/1986 U 4. It was named after the daughter of the banished Duke in William Shakespeare's play ""As You Like It"". It is"
"Cordelia (moon) Cordelia ( ) is the innermost known moon of Uranus. It was discovered from the images taken by ""Voyager 2"" on January 20, 1986, and was given the temporary designation S/1986 U 7. It was not detected again until the Hubble Space Telescope observed it in 1997. Cordelia takes its name from the youngest daughter of Lear in William Shakespeare's ""King Lear."" It is also designated Uranus VI. Other than its orbit, radius of 20 km and geometric albedo of 0.08 virtually nothing is known about it. In the Voyager 2 images Cordelia appears as an elongated object"
"Cressida (moon) Cressida ( , ) is an inner satellite of Uranus. It was discovered from the images taken by ""Voyager 2"" on 9 January 1986, and was given the temporary designation S/1986 U 3. It was named after Cressida, the Trojan daughter of Calchas, a tragic heroine who appears in William Shakespeare's play ""Troilus and Cressida"" (as well as in tales by Geoffrey Chaucer and others). It is also designated Uranus IX. Cressida belongs to the Portia Group of satellites, which includes Bianca, Desdemona, Juliet, Portia, Rosalind, Cupid, Belinda and Perdita. These satellites have similar orbits and photometric properties."
"about it. At the Voyager 2 images Bianca appears as an elongated object, the major axis pointing towards Uranus. The ratio of axes of the Bianca's prolate spheroid is 0.7 ± 0.2. Its surface is grey in color. Explanatory notes Citations Bianca (moon) Bianca ( ) is an inner satellite of Uranus. It was discovered from the images taken by ""Voyager 2"" on January 23, 1986, and was given the temporary designation S/1986 U 9. It was named after the sister of Katherine in Shakespeare's play ""The Taming of the Shrew"". It is also designated Uranus VIII. Bianca belongs to"
"Ursula (crater) Ursula is a large crater on Uranus's moon Titania. It is about 135 km across, and is cut by Belmont Chasma. It is named after Hero's attendant in William Shakespeare's comedy Much Ado About Nothing. Ursula has a central pit with diameter of about 20 km. It is probably one of the youngest large impact craters on Titania. The crater is surrounded by smooth plains, which have the lowest impact crater density of all geological units on the moon, although they are cut by Belmont Chasma. The plains may be impact deposits (ejecta) associated with Ursula or they"
"may be cryovolcanic in origin. Explanatory notes Citations Sources Ursula (crater) Ursula is a large crater on Uranus's moon Titania. It is about 135 km across, and is cut by Belmont Chasma. It is named after Hero's attendant in William Shakespeare's comedy Much Ado About Nothing. Ursula has a central pit with diameter of about 20 km. It is probably one of the youngest large impact craters on Titania. The crater is surrounded by smooth plains, which have the lowest impact crater density of all geological units on the moon, although they are cut by Belmont Chasma. The plains may"
"numerals, and since then Titania has been designated '. Shakespeare's character's name is pronounced , but the moon is often pronounced , by analogy with the familiar chemical element titanium. The adjectival form, ""Titanian"", is homonymous with that of Saturn's moon Titan. The name ""Titania"" is ancient Greek in origin, meaning ""Daughter of the Titans"". Titania orbits Uranus at the distance of about , being the second farthest from the planet among its five major moons. Titania's orbit has a small eccentricity and is inclined very little relative to the equator of Uranus. Its orbital period is around 8.7 days,"
"Desdemona (moon) Desdemona ( ) is an inner satellite of Uranus. It was discovered from the images taken by ""Voyager 2"" on 13 January 1986, and was given the temporary designation S/1986 U 6. Desdemona is named after the wife of Othello in William Shakespeare's play ""Othello"". It is also designated Uranus X. Desdemona belongs to Portia Group of satellites, which also includes Bianca, Cressida, Juliet, Portia, Rosalind, Cupid, Belinda and Perdita. These satellites have similar orbits and photometric properties. Other than its orbit, radius of 32 km and geometric albedo of 0.08 virtually nothing is known about Desdemona. At"
"10199 Chariklo 10199 Chariklo ( or ; ; provisional designation ) is the largest confirmed centaur (minor planet of the outer Solar System). It orbits the Sun between Saturn and Uranus, grazing the orbit of Uranus. On 26 March 2014, astronomers announced the discovery of two rings (nicknamed Oiapoque and Chuí) around Chariklo by observing a stellar occultation, making it the first minor planet known to have rings. Chariklo was discovered by James V. Scotti of the Spacewatch program on February 15, 1997. Chariklo is named after the nymph Chariclo (""""), the wife of Chiron and the daughter of Apollo."
"Ariel (moon) Ariel is the fourth-largest of the 27 known moons of Uranus. Ariel orbits and rotates in the equatorial plane of Uranus, which is almost perpendicular to the orbit of Uranus and so has an extreme seasonal cycle. It was discovered in October 1851 by William Lassell and named for a character in two different pieces of literature. As of 2017, much of the detailed knowledge of Ariel derives from a single flyby of Uranus performed by the spacecraft ""Voyager 2"" in 1986, which managed to image around 35% of the moon's surface. There are no active plans at"
"sky, where ""'midst the stars [it] inscribes Belinda's name"", contributed to the eventual naming of three of the moons of Uranus after characters from ""The Rape of the Lock"": Umbriel, Ariel, and Belinda. The first two are major bodies and were named in 1852 by John Herschel, a year after their discovery. The inner satellite Belinda was not discovered until 1986 and is the only other of the planet's 27 moons taken from Pope's poem rather than Shakespeare's works. Modern adaptations of ""The Rape of the Lock"" include Deborah Mason's opera-ballet, on which the composer worked since 2002. It had"