Elara near the glare of bright Jupiter |
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| Discovery | |
|---|---|
| Discovered by | C. D. Perrine |
| Discovery date | January 2, 1905[1][2] |
| Orbital characteristics | |
| Mean orbit radius | 11,740,000 km (0.07810 AU)[3] |
| Eccentricity | 0.22[3] |
| Orbital period | 259.64 d (0.708 a)[3] |
| Average orbital speed | 3.27 km/s[3] |
| Inclination | 26.63° (to the ecliptic) 30.66° (to Jupiter's equator)[3] |
| Satellite of | Jupiter |
| Physical characteristics | |
| Mean radius | 43 km[4] |
| Surface area | ~23,200 km2 |
| Volume | ~333,000 km3 |
| Mass | 8.7×1017 kg |
| Mean density | 2.6 g/cm3 (assumed)[4] |
| Equatorial surface gravity | ~0.031 m/s2 (0.003 g) |
| Escape velocity | ~0.052 km/s |
| Sidereal rotation period | ~0.5 d (12 h) |
| Albedo | 0.04 (assumed)[4] |
| Temperature | ~124 K |
| Apparent magnitude | 16.3[4] |
Elara (pron.: /ˈɛlərə/ EL-ər-ə; Greek: Ελάρα) is a prograde irregular satellite of Jupiter. It was discovered by Charles Dillon Perrine at Lick Observatory in 1905.[1][2] It is the eighth largest moon of Jupiter and is named after Elara, one of Zeus's lovers and the mother of the giant Tityos.[5]
Elara did not receive its present name until 1975; before then, it was simply known as Jupiter VII. It was sometimes called "Hera"[6] between 1955 and 1975.
Elara belongs to the Himalia group, five moons orbiting between 11 and 13 Gm from Jupiter at an inclination of about 27.5°.[3] Its orbital elements are as of January 2000. They are continuously changing due to solar and planetary perturbations.
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In February and March 2007, the New Horizons spacecraft to Pluto captured Elara in several LORRI images from a distance of five million miles.
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