Callisto (moon)

{{Infobox planet
| name = Callisto
| alt_names = Jupiter IV
| adjectives = Callistoan, Callistonian
| image = Callisto - July 8 1979 (38926064465).jpg
| bgcolour = #a0ffa0
| discoverer = Galileo Galilei
| discovered = 7 January 1610
| apoapsis = 
| period = 
| avg_speed = 
| inclination = 2.017° (to the ecliptic)0.192° (to local Laplace planes)
| satellite_of = Jupiter
| mean_radius =  (0.378 Earths)>
| surface_area =  (0.143 Earths)
| volume =  (0.0541 Earths)
| mass =  (0.018 Earths)
| density = 
| surface_grav =  (0.126 *g*)
| moment_of_inertia_factor =  (estimate)
| escape_velocity = 2.440&nbsp;km/s
| rotation = synchronous
| axial_tilt = zero
| albedo = 0.22 (geometric)
| magnitude = 5.65 (opposition)
| temp_name1 = K
| max_temp_1 = 
| mean_temp_1 = 
| min_temp_1 = 
| atmosphere = yes
| surface_pressure =  (, )
| atmosphere_composition = ≈&thinsp; carbon dioxide;up to  molecular oxygen(O2)
}}

**Callisto** is a moon of the planet Jupiter. It was discovered in 1610 by Galileo Galilei and named after Kallisto. It is the second largest moon orbiting Jupiter, after Ganymede, and the third largest moon in the Solar System. 

Callisto is almost the same size as the planet Mercury, being 99% the diameter of the planet, but is much less massive. Of the four Galilean moons of Jupiter, Callisto is the farthest out, with an orbital radius of about 1,880,000&nbsp;kilometres. It does not form part of the orbital resonance that affects three inner Galilean satellites, Io, Europa and Ganymede. Like the Earth's Moon, Callisto rotates synchronously with its orbital period. This means that one side is always turned toward Jupiter, while the other side never sees the face of the planet. Callisto's surface is less affected by Jupiter's magnetosphere than the seven moons nearer the planet.

Callisto has about equal amounts of rock and ices, with an average density of about 1.83&nbsp;g/cm³. Chemical compounds on the surface include water ice, carbon dioxide, silicates, and organics. The Galileo spacecraft made investigations of the moon, and revealed that Callisto may have a small silicate core and possibly a subsurface ocean of liquid water more than 100&nbsp;kilometers deep.

The surface of Callisto is heavily cratered and extremely old. The surface does not show any sign of processes occurring below the surface such as plate tectonics, earthquakes or volcanoes, and is thought to have evolved mainly under the influence of meteorite impacts. Notable surface features include multi-ring structures, impact craters in different shapes, and chains of craters (known as catenae) and associated scarps, ridges and deposits. The absolute ages of the landforms are not known.

Callisto is surrounded by an extremely thin atmosphere made out of carbon dioxide and probably oxygen molecules. There is also a rather intense ionosphere. An ocean is thought to exist within Callisto. This may mean that life might exist. However, this is less likely than on nearby Europa. 

Various space probes from Pioneers 10–11 to Galileo and Cassini−Huygens have studied the moon. Callisto is considered the most suitable place for humans to settle for future exploration of the Jovian system.

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