Kalyke

Kalyke /ˈkælək/, also known as Jupiter XXIII, is a retrograde irregular satellite of Jupiter. It was discovered by a team of astronomers from the University of Hawaii led by Scott S. Sheppard in 2000, and given the temporary designation S/2000 J 2.

Kalyke
Kalyke imaged by the Canada-France-Hawaii Telescope in December 2001
Discovery
Discovered byScott S. Sheppard
David C. Jewitt
Yanga R. Fernandez
Eugene A. Magnier
Discovery siteMauna Kea Observatory
Discovery date23 November 2000
Designations
Designation
Jupiter XXIII
Pronunciation/ˈkælək/
Named after
Καλύκη Kalykē
Alternative names
S/2000 J 2
AdjectivesKalykean /kæləˈkən/
Orbital characteristics
Epoch 27 April 2019 (JD 2458600.5)
Observation arc16.34 yr (5,967 days)
Semi-major axis
0.1614179 AU (24,147,770 km)
Eccentricity0.3028225
Orbital period (sidereal)
−766.61 d
Mean anomaly
63.16063°
Mean motion
0° 28m 10.57s / day
Inclination165.93730° (to ecliptic)
Longitude of ascending node
132.43876°
323.78885°
Satellite ofJupiter
GroupCarme group
Physical characteristics
Mean diameter
6.9±1.3 km
Albedo0.029±0.014
21.8
15.4

    From infrared thermal measurements by the WISE spacecraft, Kalyke's albedo is measured at 2.9%, corresponding to a diameter of 6.9 kilometres. It orbits Jupiter at an average distance of 23,181,000 km in 766.61 days, at an inclination of 166° to the ecliptic (165° to Jupiter's equator), in a retrograde direction and with an eccentricity of 0.2140.

    It was named in October 2002 after the Greek mythological figure Kalyke or Calyce.

    It belongs to the Carme group, made up of irregular retrograde moons orbiting Jupiter at a distance ranging between 23 and 24 Gm and at an inclination of about 165°. Kalyke is redder in color (B−V=0.94, V−R=0.70) than other moons of the Carme group, suggesting that it is a captured centaur or TNO, or a remnant of such an object that collided with the Carme group progenitor.

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