Megaclite facts for kids
Megaclite imaged by the Canada-France-Hawaii Telescope in December 2001
|
|
| Discovery | |
|---|---|
| Discovered by | Scott S. Sheppard David C. Jewitt Yanga R. Fernandez Eugene A. Magnier |
| Discovery site | Mauna Kea Observatory |
| Discovery date | 25 November 2000 |
| Designations | |
| MPC designation | Jupiter XIX |
| Pronunciation | /mɛɡəˈklaɪtiː/ |
|
Named after
|
Μεγακλειτή Megaclītē |
| S/2000 J 8 | |
| Adjectives | Megaclitean /ˌmɛɡəklɪˈtiːən/ |
| Orbital characteristics | |
| Epoch 27 April 2019 (JD 2458600.5) | |
| Observation arc | 16.26 yr (5,938 days) |
| 0.1586666 AU (23,736,190 km) | |
| Eccentricity | 0.4102170 |
| –747.09 d | |
| 269.64681° | |
|
Mean motion
|
0° 28m 54.732s / day |
| Inclination | 143.20224° (to ecliptic) |
| 356.52408° | |
| 8.71854° | |
| Satellite of | Jupiter |
| Physical characteristics | |
|
Mean diameter
|
≈ 6 km |
| Albedo | 0.04 (assumed) |
| 21.7 | |
| 15.0 | |
Megaclite /mɛɡəˈklaɪtiː/, also known as Jupiter XIX, is a natural 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 8.
Megaclite is about 6 kilometres in diameter, and orbits Jupiter at an average distance of 24,687,000 kilometers in 747.09 days, at an inclination of 150° to the ecliptic (148° to Jupiter's equator), in a retrograde direction and with an eccentricity of 0.308.
It was named in October 2002 after Megaclite, mother by Zeus (Jupiter) of Thebe and Locrus in Greek mythology.
It belongs to the Pasiphae group, irregular retrograde moons orbiting Jupiter at distances ranging between 22.8 and 24.7 Gm, and with inclinations ranging between 144.5° and 158.3°. However, while Pasiphae is gray (B−V=0.74, V−R=0.38, V−I=0.74) in color, Megaclite is light red (B−V=0.94, V−R=0.41, V−I=1.05) and come similar to Callirrhoe.
See also
In Spanish: Megaclite (satélite) para niños
