Short description: Moon of Uranus
- There is also an asteroid called 548 Kressida.
Cressida Enhanced Voyager 2 image of Cressida |
| Discovery |
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| Discovered by | Stephen P. Synnott / Voyager 2 |
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| Discovery date | January 9, 1986 |
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| Designations |
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Designation | Uranus IX |
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| Pronunciation | [1] |
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| Named after | Χρησίδα |
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| Adjectives | Cressidian [2] |
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| Orbital characteristics |
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| Mean orbit radius | 61,766.730 ± 0.046 km[3] |
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| Eccentricity | 0.00036 ± 0.00011[3] |
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| Orbital period | 0.463569601 ± 0.000000013 d[3] |
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| Inclination | 0.006 ± 0.040° (to Uranus' equator)[3] |
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| Satellite of | Uranus |
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| Physical characteristics |
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| Dimensions | 92 × 74 × 74 km[4] |
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| Mean radius | 39.8 ± 2 km[4][5][6] |
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| Surface area | ~20,000 km2[lower-alpha 1] |
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| Volume | ~260,000 km3[lower-alpha 1] |
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| Mass | 2.5±0.4×1017 kg[7] |
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| Mean density | 0.86±0.16 g/cm3[7] |
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surface gravity | ~0.013 m/s2[lower-alpha 1] |
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escape velocity | ~0.034 km/s[lower-alpha 1] |
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| Rotation period | synchronous[4] |
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| Axial tilt | zero[4] |
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| Physics | ~64 K[lower-alpha 1] |
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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.[8] 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.[9]
Cressida belongs to the Portia group of satellites, which includes Bianca, Desdemona, Juliet, Portia, Rosalind, Cupid, Belinda and Perdita.[10] These satellites have similar orbits and photometric properties.[10] Other than its orbit,[3] radius of 41 km[4] and geometric albedo of 0.08,[10] virtually nothing is known about it.
In the Voyager 2 images Cressida appears as an elongated object, its major axis pointing towards Uranus. The ratio of axes of Cressida's prolate spheroid is 0.8 ± 0.3.[4] Its surface is grey in color.[4]
Cressida orbits close to a 3:2 resonance with the η ring, one of the rings of Uranus. Perturbations of the ring's shape provide a way to measure the mass of Cressida, which was found to be 2.5±0.4×1017 kg. Cressida is the only small satellite of Uranus for which the mass has been directly measured.[7]
Cressida may collide with Desdemona within the next 100 million years.[11]
See also
References
Explanatory notes
- ↑ 1.0 1.1 1.2 1.3 1.4 Calculated on the basis of other parameters.
Citations
- ↑ Benjamin Smith (1903) The Century Dictionary and Cyclopedia
- ↑ Kellog (1995) Boccaccio's and Chaucer's Cressida
- ↑ 3.0 3.1 3.2 3.3 3.4
Jacobson, R. A. (1998). "The Orbits of the Inner Uranian Satellites From Hubble Space Telescope and Voyager 2 Observations". The Astronomical Journal 115 (3): 1195–1199. doi:10.1086/300263. Bibcode: 1998AJ....115.1195J.
- ↑ 4.0 4.1 4.2 4.3 4.4 4.5 4.6
Karkoschka, Erich (2001). "Voyager's Eleventh Discovery of a Satellite of Uranus and Photometry and the First Size Measurements of Nine Satellites". Icarus 151 (1): 69–77. doi:10.1006/icar.2001.6597. Bibcode: 2001Icar..151...69K.
- ↑
"Planetary Satellite Physical Parameters". JPL (Solar System Dynamics). 24 October 2008. http://ssd.jpl.nasa.gov/?sat_phys_par.
- ↑
Williams, Dr. David R. (23 November 2007). "Uranian Satellite Fact Sheet". NASA (National Space Science Data Center). http://nssdc.gsfc.nasa.gov/planetary/factsheet/uraniansatfact.html.
- ↑ 7.0 7.1 7.2
Chancia, Robert. A.; Hedman, Matthew M.; French, Richard G. (28 August 2017). "Weighing Uranus' moon Cressida with the η ring". The Astronomical Journal 154 (4): 153. doi:10.3847/1538-3881/aa880e. Bibcode: 2017AJ....154..153C.
- ↑
Smith, B. A. (January 16, 1986). "Satellites of Uranus". IAU Circular 4164. http://www.cbat.eps.harvard.edu/iauc/04100/04164.html#Item1. Retrieved 29 October 2011.
- ↑
"Planet and Satellite Names and Discoverers". Gazetteer of Planetary Nomenclature. USGS Astrogeology. July 21, 2006. http://planetarynames.wr.usgs.gov/Page/Planets.
- ↑ 10.0 10.1 10.2
Karkoschka, Erich (2001). "Comprehensive Photometry of the Rings and 16 Satellites of Uranus with the Hubble Space Telescope". Icarus 151 (1): 51–68. doi:10.1006/icar.2001.6596. Bibcode: 2001Icar..151...51K.
- ↑
Duncan, Martin J.; Lissauer, Jack J. (1997). "Orbital Stability of the Uranian Satellite System". Icarus 125 (1): 1–12. doi:10.1006/icar.1996.5568. Bibcode: 1997Icar..125....1D.
External links
- Cressida Profile by NASA's Solar System Exploration
- Uranus' Known Satellites (by Scott S. Sheppard)
Uranus (Outline of Uranus |
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| Geography |
- Atmosphere
- Climate
- Dark Spot
- Magnetosphere
- Rings
| |
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| Moons |
- Ariel
- Miranda
- Oberon
- Puck
- Titania
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|
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| Astronomy | | Discovery |
- William Herschel
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| General |
- 15 Orionis
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| Exploration | | Past | |
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| Proposals |
- MUSE
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- NASA Uranus orbiter and probe
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|
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|
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| Related | |
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Moons of Uranus |
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- Generally listed in increasing distance from Uranus
|
| Inner |
- Rings of Uranus
- Cordelia
- Ophelia
- Bianca
- Cressida
- Desdemona
- Juliet
- Portia
- Rosalind
- Cupid
- Belinda
- Perdita
- Puck
- Mab
|
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| Major (spheroid) |
- Miranda
- Ariel
- Umbriel
- Titania
- Oberon
|
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| Outer (irregular) |
- Francisco
- Caliban
- Stephano
- Trinculo
- Sycorax
- Margaret
- Prospero
- Setebos
- Ferdinand
|
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| Geological features |
- Arielian
- Mirandian
- Oberonian
- Puckian
- Titanian
- Gertrude
- Messina Chasmata
- Ursula
- Rousillon Rupes
- Umbrielian
|
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Natural satellites of the Solar System |
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Planetary satellites |
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- 2003 AZ84
- Gǃkúnǁʼhòmdímà–Gǃòʼé ǃHú
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