Prospero (moon)
Discovery image of Prospero, taken by the CFHT in July 1999 | |
| Discovery | |
|---|---|
| Discovered by |
|
| Discovery date | 18 July 1999 |
| Designations | |
Designation | Uranus XVIII |
| Pronunciation | /ˈprɒspɛroʊ/[1] |
| Adjectives | Prosperonian /prɒspɛˈroʊniən/,[2] Prosperian /prɒˈspɪəriən/[3] |
| Orbital characteristics | |
Mean orbit radius | 16,256,000 km[4][5] |
| Eccentricity | 0.4448[5] |
| 1978.29 d | |
| Inclination | 152°[4] (to the ecliptic)[4] |
| Satellite of | Uranus |
| Physical characteristics | |
| 50 km <50 km[6] | |
| 7.145±0.092 h[6] | |
| Albedo | 0.04 (Assumed) >0,03 [6] |
| 23,2 | |
| 10,6 | |
Prospero, also known as Uranus XVIII, is one of the largest retrograde irregular satellites of Uranus.
Discovery and Naming
Prospero was discovered on 18 July 1999 by the astrophysicist Matthew Holman and his team, and given the provisional designation S/1999 U 3.
Confirmed as Uranus XVIII, it was named after the sorcerer Prospero in William Shakespeare's play The Tempest.
Orbit
Prospero orbits Uranus at an average distance of 16,256,000 km, in 1978 days, at an inclination of about 152° to the ecliptic, in a retrograde direction and with a high eccentricity of 0.445. The orbital elements are continuously changing due to solar and planetary perturbations.
Physical characteristics
Prospero's estimated diameter is 50 kilometers, assuming an albedo of 4%.
The satellite appears neutral (grey) in visible light (colour indices B−V=0.80, R−V=0.39),[7] similar to Setebos.
Measurements of Prospero's light curve by the Kepler Space Telescope indicate that its rotation period is about 7 hours and 8.76 min,[6] which makes it one of the fastest-rotating moons in the Solar System.
Origin
Prospero probably did not form near Uranus but was captured by Uranus later. Its orbital parameters suggest that it may belong to the same dynamic cluster as Sycorax and Setebos, suggesting a common origin.[8] However, Sycorax has a much redder color than the other moons, which tend to be grey in color.
See also
References
- ^ Benjamin Smith (1903), The Century Dictionary and Cyclopedia
- ^ Emenyonu, Ernest (2003), Emerging perspectives on Chinua Achebe, v. 1.
- ^ in scare quotes in Bate (1997) The genius of Shakespeare
- ^ a b c Sheppard, Jewitt & Kleyna 2005, p. 523, Table 3.
- ^ a b Yeomans, Donald K. (28 June 2007). "Planetary Satellite Mean Orbital Parameters". JPL/NASA. Retrieved 19 January 2008.
- ^ a b c d Farkas-Takács, A.; Kiss, Cs.; Pál, A.; Molnár, L.; Szabó, Gy. M.; Hanyecz, O.; et al. (September 2017). "Properties of the Irregular Satellite System around Uranus Inferred from K2, Herschel, and Spitzer Observations". The Astronomical Journal. 154 (3): 13. arXiv:1706.06837. Bibcode:2017AJ....154..119F. doi:10.3847/1538-3881/aa8365. S2CID 118869078. 119.
- ^ Grav, Holman & Fraser 2004.
- ^ Grav, Tommy; Holman, Matthew J.; Gladman, Brett J.; Aksnes, Kaare Photometric survey of the irregular satellites, Icarus, 166, (2003), pp. 33–45. arXiv:astro-ph/0301016
- Grav, Tommy; Holman, Matthew J.; Fraser, Wesley C. (20 September 2004). "Photometry of Irregular Satellites of Uranus and Neptune". The Astrophysical Journal. 613 (1): L77–L80. arXiv:astro-ph/0405605. Bibcode:2004ApJ...613L..77G. doi:10.1086/424997. S2CID 15706906.
- Sheppard, S. S.; Jewitt, D.; Kleyna, J. (2005). "An Ultradeep Survey for Irregular Satellites of Uranus: Limits to Completeness". The Astronomical Journal. 129 (1): 518–525. arXiv:astro-ph/0410059. Bibcode:2005AJ....129..518S. doi:10.1086/426329. S2CID 18688556.