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Sycorax (moon)

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For other uses, see Sycorax (disambiguation).
Sycorax
Animation of discovery images taken by the Hale Telescope in September 1997
Discovery[1]
Discovered by
Discovery siteHale Telescope at Palomar Obs.
Discovery date6 September 1997
Designations
Designation
Uranus XVII
Pronunciation/ˈsɪkɒræks/[2][3]
Named after
Sycorax
S/1997 U 2
AdjectivesSycoraxian /sɪkɒˈræksiən/[4]
Orbital characteristics[5]
Epoch 31 July 2016 (JD 2457600.5)
Observation arc32.37 yr (11,815 d)
Earliest precovery date2 June 1984
12,193,230 km (0.0815067 AU)
Eccentricity0.4841889
3.52 yr (1,286.28 d)
160.58731°
0° 16m 47.56s / day
Inclination153.22796° (to the ecliptic)
159.403° (to local Laplace plane)[6]
258.56478°
16.29680°
Satellite ofUranus
Physical characteristics
157+23
−15 km[7]
165+36
−42 km[8]
Mass~2.5×1018 kg (estimate)[6]
Mean density
~1.3 g/cm3 (assumed)[6]
6.9162±0.0013 hr (double-peaked)[7]
3.6 hr (single-peaked)[9]
Albedo0.065+0.015
−0.011[7]
0.049+0.038
−0.017[8]
Temperature~65 K (mean estimate)
20.8 (V)[10]
7.5±0.04[7]
7.83±0.06[8]

Sycorax /ˈsɪkɒræks/ is the largest retrograde irregular satellite of Uranus. Sycorax was discovered on 6 September 1997 by Brett J. Gladman, Philip D. Nicholson, Joseph A. Burns, and John J. Kavelaars using the 200-inch Hale telescope, together with Caliban, and given the temporary designation S/1997 U 2.[1]

Retrograde irregular satellites of Uranus

Officially confirmed as Uranus XVII, it was named after Sycorax, Caliban's mother in William Shakespeare's play The Tempest.

Orbit

Animation of Sycorax's orbit around Uranus.
   Uranus  ·    Sycorax ·    Francisco  ·    Caliban  ·    Stephano  ·    Trinculo

Sycorax follows a distant orbit, more than 20 times further from Uranus than the furthest regular moon, Oberon.[1] Its orbit is retrograde, moderately inclined and eccentric. The orbital parameters suggest that it may belong, together with Setebos and Prospero, to the same dynamic cluster, suggesting common origin.[11]

The diagram illustrates the orbital parameters of the retrograde irregular satellites of Uranus (in polar co-ordinates) with the eccentricity of the orbits represented by the segments extending from the pericentre to the apocentre.

Physical characteristics

Full discovery image of Sycorax, located at the top-right of the image

The diameter of Sycorax is estimated at 165 km based on the thermal emission data from Spitzer and Herschel Space telescopes[8] making it the largest irregular satellite of Uranus, comparable in size with Puck and with Himalia, the biggest irregular satellite of Jupiter.

The satellite appears light-red in the visible spectrum (colour indices B–V = 0.87 V–R = 0.44,[12] B–V = 0.78 ± 0.02 V–R = 0.62 ± 0.01,[11] B–V = 0.839 ± 0.014 V–R = 0.531 ± 0.005[9]), redder than Himalia but still less red than most Kuiper belt objects. However, in the near infrared, the spectrum turns blue between 0.8 and 1.25 μm[clarification needed] and finally becomes neutral at the longer wavelengths.[10]

The rotation period of Sycorax is estimated at about 6.9 hours.[7] Rotation causes periodical variations of the visible magnitude with the amplitude of 0.12.[7] The rotation axis of Sycorax is unknown, though measurements of its light curve suggest it is being viewed at an near equator-on configuration. In this case, Sycorax may have a north pole right ascension around 356° and a north pole declination around 45°.[7]

Origin

It is hypothesized that Sycorax is a captured object; it did not form in the accretion disk which existed around Uranus just after its formation. No exact capture mechanism is known, but capturing a moon requires the dissipation of energy. Possible capture processes include gas drag in the protoplanetary disk and many-body interactions and capture during the fast growth of Uranus's mass (so-called pull-down).[13][9]

See also

References

  1. ^ a b c Gladman Nicholson et al. 1998.
  2. ^ Shakespeare Recording Society (1995) The Tempest (audio CD)
  3. ^ Benjamin Smith (1903) The Century Dictionary and Cyclopedia
  4. ^ Goldberg (2004) Tempest in the Caribbean
  5. ^ "M.P.C. 102109" (PDF). Minor Planet Circular. Minor Planet Center. 14 November 2016.
  6. ^ a b c Jacobson, R.A. (2003) URA067 (2007-06-28). "Planetary Satellite Mean Orbital Parameters". JPL/NASA. Retrieved 2008-01-23.{{cite web}}: CS1 maint: numeric names: authors list (link)
  7. ^ a b c d e f g 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.{{cite journal}}: CS1 maint: unflagged free DOI (link)
  8. ^ a b c d Lellouch, E.; Santos-Sanz, P.; Lacerda, P.; Mommert, M.; Duffard, R.; Ortiz, J. L.; Müller, T. G.; Fornasier, S.; Stansberry, J.; Kiss, Cs.; Vilenius, E.; Mueller, M.; Peixinho, N.; Moreno, R.; Groussin, O.; Delsanti, A.; Harris, A. W. (September 2013). ""TNOs are Cool": A survey of the trans-Neptunian region. IX. Thermal properties of Kuiper belt objects and Centaurs from combined Herschel and Spitzer observations" (PDF). Astronomy & Astrophysics. 557: A60. arXiv:1202.3657. Bibcode:2013A&A...557A..60L. doi:10.1051/0004-6361/201322047. Retrieved 7 November 2014.
  9. ^ a b c Maris, Michele; Carraro, Giovanni; Parisi, M.G. (2007). "Light curves and colours of the faint Uranian irregular satellites Sycorax, Prospero, Stephano, Setebos, and Trinculo". Astronomy & Astrophysics. 472 (1): 311–319. arXiv:0704.2187. Bibcode:2007A&A...472..311M. doi:10.1051/0004-6361:20066927. S2CID 12362256.
  10. ^ a b Romon, J.; de Bergh, C.; et al. (2001). "Photometric and spectroscopic observations of Sycorax, satellite of Uranus". Astronomy & Astrophysics. 376 (1): 310–315. Bibcode:2001A&A...376..310R. doi:10.1051/0004-6361:20010934.
  11. ^ a b Grav, Holman & Fraser 2004.
  12. ^ Rettig, Walsh & Consolmagno 2001.
  13. ^ Sheppard, Jewitt & Kleyna 2005.
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