![]() Click image for description | |
Discovery | |
---|---|
Discovered by | G. Galilei S. Marius |
Discovery date | January 11, 1610 |
Orbital characteristics | |
Periapsis | 1,069,200 km (0.007147 AU) |
Apoapsis | 1,071,600 km (0.007163 AU) |
Mean orbit radius | 1,070,400 km (0.007155 AU) |
Eccentricity | 0.002[1] |
7.15455296 d (0.019588 a) | |
Average orbital speed | 10.880 km/s |
Inclination | 2.21° (to the ecliptic) 0.20° (to Jupiter's equator) |
Satellite of | Jupiter |
Physical characteristics | |
Mean radius | 2631.2 km (0.413 Earths) |
87.0 million km² (0.171 Earths) [2] | |
Volume | 7.6×1010 km³ (0.0704 Earths) |
Mass | 1.4819×1023 kg (0.025 Earths) |
Mean density | 1.942 g/cm³ |
1.428 m/s2 (0.146 g) | |
2.741 km/s (6,130 mph) | |
synchronous | |
zero | |
Albedo | 0.43 ± 0.02[3] |
Temperature | ~109 K (−172 °C) |
4.61 (opposition) [3] | |
Atmosphere | |
Surface pressure | trace |
Composition by volume | oxygen |
Ganymede[p] is the largest of the 95 known moons of the planet Jupiter. It is also the largest moon in the Solar System. Ganymede is larger in diameter than the planet Mercury, but has only about half of its mass as Ganymede is much less dense. Ganymede is part of a group called the Galilean Satellites. These also include Io, Europa and Callisto.
Galileo Galilei discovered this moon in 1610.[4] Simon Marius suggested the name "Ganymede" soon after. In Greek mythology, Ganymede was Zeus' cup-bearer.[5] This name and the names of the other Galilean satellites were not favoured for a long time, and were not put into common use until the mid-20th century. Instead, it is simply referred to by its Roman numeral designation (a system that was introduced by Galileo) as "Jupiter III" or as the "third satellite of Jupiter".[6] Ganymede is the only Galilean moon of Jupiter named after a male figure.