Cressida (moon)
| Discovery | |
|---|---|
| Discovered by | Stephen P. Synnott / Voyager 2 |
| Discovery date | January 9, 1986 |
| Orbital characteristics | |
Mean orbit radius | 61,766.730 ± 0.046 km[1] |
| Eccentricity | 0.00036 ± 0.00011[1] |
| 0.463569601 ± 0.000000013 d[1] | |
| Inclination | 0.006 ± 0.040° (to Uranus' equator)[1] |
| Satellite of | Uranus |
| Physical characteristics | |
| Dimensions | 92 × 74 × 74 km[2] |
Mean radius | 41 ± 2 km[2] |
| ~20,000 km²[3] | |
| Volume | ~260,000 km³[3] |
| Mass | ~3.4×1017 kg[3] |
Mean density | ~1.3 g/cm³ (assumed) |
| ~0.013 m/s2[3] | |
| ~0.034 km/s[3] | |
| synchronous[2] | |
| zero[2] | |
| Albedo | 0.08 ± 0.01[4] |
| Temperature | ~64 K[3] |
Cressida is a closer moon to Uranus. It was found from the images taken by Voyager 2 on 1986-01-09, and was given the designation S/1986 U 3.[5] It was named after 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.[6]
Cressida belongs to Portia Group of moons, which also includes Bianca, Desdemona, Juliet, Portia, Rosalind, Cupid, Belinda and Perdita.[4] These moons have similar orbits and photometric properties.[4] Other than its orbit,[1] radius of 41 km[2] and geometric albedo of 0.08[4] almost nothing is known about it.
At the Voyager 2 images Cressida appears as a stretched object, the major axis pointing towards Uranus. The ratio of axes of Cressida's prolate spheroid is 0.8 ± 0.3.[2] Its surface is grey in color.[2]
References
[change | change source]- ↑ 1.0 1.1 1.2 1.3 1.4 Jacobson, R.A. (1998). "The Orbits of the Inner Uranian Satellites From Hubble Space Telescope and Voyager2 Observations". The Astronomical Journal. 115 (3): 1195–1199. Bibcode:1998AJ....115.1195J. doi:10.1086/300263. S2CID 118616209.
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 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. Bibcode:2001Icar..151...69K. doi:10.1006/icar.2001.6597.
- ↑ 3.0 3.1 3.2 3.3 3.4 3.5 Calculated on the basis of other parameters
- ↑ 4.0 4.1 4.2 4.3 Karkoschka, Erich (2001). "Comprehensive Photometry of the Rings and 16 Satellites of Uranus with the Hubble Space Telescope". Icarus. 151 (1): 51–68. Bibcode:2001Icar..151...51K. doi:10.1006/icar.2001.6596.
- ↑ Smith, B. A. (January 16, 1986). "IAU Circular No. 4164". Retrieved 2006-08-06.
- ↑ "Planet and Satellite Names and Discoverers". Gazetteer of Planetary Nomenclature. USGS Astrogeology. July 21, 2006. Retrieved 2006-08-06.
Other websites
[change | change source]- Cressida Profile Archived 2007-06-08 at the Wayback Machine by NASA's Solar System Exploration
| Moons | Ariel · Belinda · Bianca · Caliban · Cordelia · Cressida · Cupid · Desdemona · Ferdinand · Francisco · Juliet · Mab · Margaret · Miranda · Oberon · Ophelia · Perdita · Portia · Prospero · Puck · Rosalind · Setebos · Stephano · Sycorax · Titania · Trinculo · Umbriel Other: Arieal features · Miranda features · Puck Craters · Umbriel craters Miranda's Verona Rupes · Umbriel Crater Wunda |  |
|---|---|---|
| Characteristics | ||
| Discovery | ||
| Exploration | ||
| Other | ||