|Discovery site||Hale Telescope at Palomar Obs.|
|Discovery date||6 September 1997|
|S/1997 U 2|
|Epoch 31 July 2016 (JD 2457600.5)|
|Observation arc||32.37 yr (11,815 d)|
|Earliest precovery date||2 June 1984|
|12,193,230 km (0.0815067 AU)|
|3.52 yr (1,286.28 d)|
|0° 16m 47.56s / day|
|Inclination||153.22796° (to the ecliptic)|
159.403° (to local Laplace plane)
|Mass||~2.5×1018 kg (estimate)|
|~1.3 g/cm³ (assumed)|
|6.9162±0.0013 hr (double-peaked)|
3.6 hr (single-peaked)
|Temperature||~65 K (mean estimate)|
Sycorax // 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.
Sycorax follows a distant orbit, more than 20 times further from Uranus than the furthest regular moon, Oberon. 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.
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.
The diameter of Sycorax is estimated at 165 km based on the thermal emission data from Spitzer and Herschel Space telescopes 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, B–V = 0.78 ± 0.02 V–R = 0.62 ± 0.01, B–V = 0.839 ± 0.014 V–R = 0.531 ± 0.005), 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.
The rotation period of Sycorax is estimated at about 6.9 hours. Rotation causes periodical variations of the visible magnitude with the amplitude of 0.12. 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°.
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).
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