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Moon of Jupiter From Wikipedia, the free encyclopedia
Chaldene /kælˈdiːniː/, also known as Jupiter XXI, 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 10.[6][1][7]
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 XXI |
Pronunciation | /kælˈdiːniː/ |
Named after | Χαλδηνή Chaldēnē |
S/2000 J 10 | |
Adjectives | Chaldenean /kældɪˈniːən/ |
Orbital characteristics [2] | |
Epoch 27 April 2019 (JD 2458600.5) | |
Observation arc | 17.46 yr (6,376 days) |
0.1604721 AU (24,006,280 km) | |
Eccentricity | 0.1500864 |
–759.88 d | |
159.35152° | |
0° 28m 25.54s / day | |
Inclination | 164.25379° (to ecliptic) |
215.26817° | |
340.66981° | |
Satellite of | Jupiter |
Group | Carme group |
Physical characteristics[3] | |
4 km | |
Albedo | 0.04 (assumed) |
Spectral type | B–V = 0.82 ± 0.05, V–R = 0.50 ± 0.05[4] |
22.5[5] | |
16.0[2] | |
Chaldene is about 3.8 kilometres in diameter, and orbits Jupiter at an average distance of 22,713,000 km in 759.88 days, at an inclination of 167° to the ecliptic (169° to Jupiter's equator), in a retrograde direction and with an eccentricity of 0.2916.
It was named in October 2002 after Chaldene, the mother of Solymos by Zeus in Greek mythology.[8]
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°.
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