Discovery [1] | |
---|---|
Discovered by | Seth B. Nicholson |
Discovery site | Mt. Wilson Observatory |
Discovery date | 6 July 1938 |
Designations | |
Designation | Jupiter X |
Pronunciation | /laɪˈsɪθiə/[2][3] |
Named after | Λυσιθέα Lysithea |
Adjectives | Lysithean /laɪˈsɪθiən/[4] |
Orbital characteristics [5] | |
Epoch 27 April 2019 (JD 2458600.5) | |
Observation arc | 79.87 yr (29,171 days) |
0.0782144 AU (11,700,710 km) | |
Eccentricity | 0.1478734 |
+258.57 d | |
27.18992° | |
1° 23m 32.227s / day | |
Inclination | 26.29254° (to ecliptic) |
343.46495° | |
94.80010° | |
Satellite of | Jupiter |
Group | Himalia group |
Physical characteristics | |
42.2±0.7 km (WISE)[6] 42.2±3 km (occultation)[7]: 6 | |
12.78±0.10 h[8] | |
Albedo | 0.036±0.006[6] |
Spectral type | C/P[6] |
18.2[9] | |
11.2[5] | |
Lysithea /laɪˈsɪθiə/ is a prograde irregular satellite of Jupiter. It was discovered by Seth Barnes Nicholson in 1938 at Mount Wilson Observatory[1] and is named after the mythological Lysithea, daughter of Oceanus and one of Zeus' lovers.[10]
Lysithea did not receive its present name until 1975; before then, it was simply known as Jupiter X. It was sometimes called "Demeter"[11] from 1955 to 1975.
It belongs to the Himalia group, moons orbiting between 11 and 13 Gm from Jupiter at an inclination of about 28.3°.[12] Its orbital elements are as of January 2000. They are continuously changing due to solar and planetary perturbations. It is gray in color (B−V=0.72, V−R=0.36, V−I=0.74) and intermediate between C-type and P-type asteroids.[13][6]
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