Perdita (moon)

Perdita /ˈpɜːrdɪtə/ is an inner satellite of Uranus. Perdita's discovery was complicated. The first photographs of Perdita were taken by the Voyager 2 spacecraft in 1986, but it was not recognized from the photographs for more than a decade. In 1999, the moon was noticed by Erich Karkoschka and reported.[3][5] But because no further pictures could be taken to confirm its existence, it was officially demoted in 2001.[6] However, in 2003, pictures taken by the Hubble Space Telescope managed to pick up an object where Perdita was supposed to be, finally confirming its existence.[7][8]

Perdita
Discovery
Discovered byErich Karkoschka / Voyager 2
Discovery dateMay 18, 1999 (in images dating back to January 18, 1986)
Designations
Designation
Uranus XXV
Pronunciation/ˈpɜːrdɪtə/[1]
AdjectivesPerditean /pɜːrdɪˈtiːən/[2]
Orbital characteristics
Mean orbit radius
76,417 ± 1 km[3]
Eccentricity0.0012 ± 0.0005[3]
0.638021 ± 0.000013 d[3]
Inclination0.0 ± 0.3° (to Uranus' equator)[3]
Satellite ofUranus
Physical characteristics
Dimensions30 × 30 × 30 km[3]
Mean radius
15 ± 3 km[3]
~2,800 km² [lower-alpha 1]
Volume~14,000 km³ [lower-alpha 1]
Mass~0.18×1017 kg[lower-alpha 1]
Mean density
~1.3 g/cm³ (assumed)
~0.0047 m/s² [lower-alpha 1]
~0.011 km/s[lower-alpha 1]
synchronous[3]
zero[3]
Albedo0.08 ± 0.01[4]
Temperature~64 K[lower-alpha 1]

    Following its discovery in 1999, it was given the temporary designation of S/1986 U 10.[5] It was named Perdita (Latin for 'lost') after the daughter of Leontes and Hermione in William Shakespeare's play The Winter's Tale. The moon is also designated Uranus XXV.[9]

    The moon orbits between Belinda and Puck. The above-mentioned Hubble measurements prove that Perdita does not follow a direct Keplerian motion around Uranus. Instead, it is clearly caught in a 43:44 orbital resonance with the nearby moon Belinda. It is also close to an 8:7 resonance with Rosalind.[3][7]

    Perdita belongs to the Portia group of satellites, which also includes Bianca, Cressida, Desdemona, Portia, Juliet, Cupid, Rosalind and Belinda.[4] These satellites have similar orbits and photometric properties.[4] Little is known about Perdita apart from its orbit,[3][7] radius of 15 km[3] and geometric albedo of 0.08.[4]

    See also

    References

    Explanatory notes

    1. Calculated on the basis of other parameters.

    Citations

    1. Benjamin Smith (1903) The Century Dictionary and Cyclopedia
    2. Byrne (2008) Perdita: the literary, theatrical, scandalous life of Mary Robinson
    3. Karkoschka, Voyager 2001.
    4. Karkoschka, Hubble 2001.
    5. IAUC 7171.
    6. Foust 2001.
    7. Showalter & Lissauer 2006.
    8. IAUC 8194.
    9. USGS: Planet and Satellite Names and Discoverers.

    Sources

    • 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.
    • 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.
    • Green, Daniel W. E. (May 18, 1999). "S/1986 U 10". IAU Circular. 7171. ISSN 0081-0304. Retrieved 2012-01-26.
    • Foust, Jeff (December 31, 2001). "Moon of Uranus is demoted". Spaceflight Now. Retrieved 2012-01-26.CS1 maint: ref=harv (link)
    • Showalter, Mark R.; Lissauer, Jack J. (2006-02-17). "The Second Ring-Moon System of Uranus: Discovery and Dynamics". Science. 311 (5763): 973–977. Bibcode:2006Sci...311..973S. doi:10.1126/science.1122882. PMID 16373533.CS1 maint: ref=harv (link)
    • Green, Daniel W. E. (September 3, 2003). "Satellites of Uranus". IAU Circular. 8194. ISSN 0081-0304. Retrieved 2012-01-26.
    • USGS/IAU (July 21, 2006). "Planet and Satellite Names and Discoverers". Gazetteer of Planetary Nomenclature. USGS Astrogeology. Retrieved 2012-01-26.
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