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Prospero (moon)

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Prospero
Discovery image of Prospero, taken by the CFHT in July 1999
Discovery
Discovered by
Discovery date18 July 1999
Designations
Designation
Uranus XVIII
Pronunciation/ˈprɒspɛroʊ/[1]
AdjectivesProsperonian /prɒspɛˈroʊniən/,[2] Prosperian /prɒˈspɪəriən/[3]
Orbital characteristics
Mean orbit radius
16,256,000 km[4][5]
Eccentricity0.4448[5]
1978.29 d
Inclination152°[4] (to the ecliptic)[4]
Satellite ofUranus
Physical characteristics
50 km[6]
  • 14.29±0.183 h (double-peak)[7]
  • 7.145±0.092 h (single-peak)[8]
Albedo0.04 (Assumed)
23.2
10.6

Prospero, also known as Uranus XVIII and previously as S/1999 U 3, is a irregular moon of Uranus. It was discovered on 18 July 1999 by Matthew Holman and his team and it was named after the sorcerer Prospero in William Shakespeare's play The Tempest. Prospero orbits Uranus at an average distance of 16.2 million km (10.1 million mi) and takes about 1978 Earth days (5.4 Earth years) to complete one orbit. Prospero is estimated to be about 50 km (31 mi)[6] in diameter and although many of its physical properties are still unknown, telescope observations suggest that it has an elongated shape and a rotation period of either 7 or 14 hours.[8][7]

Animation of discovery images to show Prospero's motion among background stars

Discovery and naming

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Prospero was discovered on 18 July 1999, together with Setebos and Stephano, by Matthew Holman and his team.

When the discovery of Prospero was announced, it was given the temporary provisional designation S/1999 U 3 by the Minor Planet Center. It was later named and given the Roman numeral designation Uranus XVIII by the International Astronomical Union's Working Group for Planetary System Nomenclature on 21 August 2000. The moon was named after the sorcerer Prospero in William Shakespeare's play The Tempest.

Orbit

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Prospero orbits Uranus at a mean distance of approximately 16,256,000 km and completes one revolution in about 1978 days. Its orbit is highly inclined, with an inclination of approximately 152° to the ecliptic, is retrograde, and has a high orbital eccentricity of 0.445. Its orbital elements are subject to continuous variations caused by solar and planetary perturbations.

Prospero is not known to be part of a collisional family or group.

The similar orbital characteristics and colors of Prospero and Setebos suggest that they may share a common origin.[9] However, further observations are needed to confirm this hypothesis.

Physical characteristics

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Very little is known about its physical properties. Assuming Prospero has a low albedo of 0.04 like other Uranian irregular moons, its brightness suggests a diameter of about 50 km (31 mi).[6]

The satellite appears neutral (grey) in visible light (colour indices B−V=0.80, R−V=0.39)[10] similar to Setebos.

Prospero's brightness varies periodically as it rotates, which indicates it has an elongated shape.[8] Kepler observations in 2017 measured a brightness variation of 0.41 magnitudes,[8] implying an equatorial semi-axis ratio (a/b) not less than 1.4. The rotation period of Prospero is ambiguous, as it depends on whether its light curve is single-peaked or double-peaked. If Propsero's light curve is single-peaked, its rotation period would be 7.145±0.092 hours.[8] If its light curve is double-peaked, then its rotation period would be 14.29±0.183 hours, twice the single-peak period.[7]

Origin

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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.[9] However, Sycorax is considerably redder than the other moons, which are predominantly gray.

Exploration

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Prospero has not been imaged up close by a space probe. All Uranian irregular moons including Prospero are planned to be distant observation targets for the proposed Uranus Orbiter and Probe (UOP), which will measure the Uranian irregular moons' rotation periods and shapes by watching their brightness change over time.[7] The UOP may not be able to do a close flyby of Prospero because the moon does not orbit near the ecliptic plane.[7]

See also

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References

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  1. ↑ Benjamin Smith (1903), The Century Dictionary and Cyclopedia
  2. ↑ Emenyonu, Ernest (2003), Emerging perspectives on Chinua Achebe, v. 1.
  3. ↑ in scare quotes in Bate (1997) The genius of Shakespeare
  4. 1 2 3 Sheppard, Jewitt & Kleyna 2005, p. 523, Table 3.
  5. 1 2 Yeomans, Donald K. (28 June 2007). "Planetary Satellite Mean Orbital Parameters". JPL/NASA. Retrieved 19 January 2008.
  6. 1 2 3 Sheppard, Scott S.; Jewitt, David; Kleyna, Jan (January 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.
  7. 1 2 3 4 5 Verbiscer, Anne J.; Denk, Tilmann; Mottola, Stefano; Porter, Simon B. (July 2023). Observing the Irregular Moons of Uranus by a Uranus Flagship Mission (PDF). Uranus Flagship: Investigations and Instruments for Cross-Discipline Science Workshop (poster). Bibcode:2023LPICo2808.8187V. 8187. Archived from the original (PDF) on 2024-02-29.
  8. 1 2 3 4 5 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.
  9. 1 2 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
  10. ↑ Grav, Holman & Fraser 2004.
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