Discovery[1] | |
---|---|
Discovered by | Scott S. Sheppard David C. Jewitt Yanga R. Fernandez Eugene A. Magnier |
Discovery site | Mauna Kea Observatory |
Discovery date | 23 November 2000 |
Designations | |
Designation | Jupiter XXIII |
Pronunciation | /ˈkæləkiː/[a] |
Named after | Καλύκη Kalykē |
S/2000 J 2 | |
Adjectives | Kalykean /kæləˈkiːən/ |
Orbital characteristics[2] | |
Epoch 27 April 2019 (JD 2458600.5) | |
Observation arc | 16.34 yr (5,967 days) |
0.1614179 AU (24,147,770 km) | |
Eccentricity | 0.3028225 |
−766.61 d | |
63.16063° | |
0° 28m 10.57s / day | |
Inclination | 165.93730° (to ecliptic) |
132.43876° | |
323.78885° | |
Satellite of | Jupiter |
Group | Carme group |
Physical characteristics | |
6.9±1.3 km[3] | |
Albedo | 0.029±0.014[3] |
21.8[4] | |
15.4[2] | |
Kalyke /ˈkæləkiː/, 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.[5][1]
From infrared thermal measurements by the WISE spacecraft, Kalyke's albedo is measured at 2.9%, corresponding to a diameter of 6.9 kilometres.[3] 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.[6]
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.[7]
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