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・ Callisthenes of Laconia
・ Callisthenia
・ Callisthenia angusta
・ Callisthenia costilobata
・ Callisthenia lacteata
・ Callisthenia plicata
・ Callisthenia ruberrima
・ Callisthenia ruficollis
・ Callisthenia schadei
・ Callisthenia truncata
・ Callisthenia variegata
・ Callisti
・ Callisto
・ Callisto (band)
・ Callisto (comics)
Callisto (moon)
・ Callisto (moth)
・ Callisto (mythology)
・ Callisto albicinctella
・ Callisto basistrigella
・ Callisto Cliffs
・ Callisto coffeella
・ Callisto Corporation
・ Callisto Cosulich
・ Callisto denticulella
・ Callisto elegantella
・ Callisto insperatella
・ Callisto pfaffenzelleri
・ Callisto Piazza
・ Callisto series


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Callisto (moon) : ウィキペディア英語版
Callisto (moon)

.〕
| rotation = synchronous
| axial_tilt = zero〔
| albedo = 0.22 (geometric)〔
| magnitude = 5.65 (opposition)〔(【引用サイトリンク】url=http://www.oarval.org/ClasSaten.htm )
| temperatures=yes
| temp_name1 = K〔
| max_temp_1 =
| mean_temp_1 =
| min_temp_1 =
| atmosphere = yes
| surface_pressure = 〔
| atmosphere_composition = ≈  carbon dioxide;〔
up to molecular oxygen(O2)〔
}}
Callisto 〔, or as (ギリシア語:''Καλλιστώ'')〕 (Jupiter IV) is one of the 67 moons of Jupiter.
It was discovered in 1610 by Galileo Galilei. It is the third-largest moon in the Solar System and the second largest in the Jovian system, after Ganymede, and the largest object in the Solar System not to be properly differentiated. At in diameter, Callisto has about 99% the diameter of the planet Mercury but only about a third of its mass. It is the fourth Galilean moon of Jupiter by distance, with an orbital radius of about .〔 It is not part of the orbital resonance that affects three inner Galilean satellites—Io, Europa and Ganymede—and thus does not experience appreciable tidal heating.〔 Callisto's rotation is tidally locked to its orbit around Jupiter, so that the same hemisphere always faces inward; Jupiter appears to stand nearly still in Callisto's sky. It is less affected by Jupiter's magnetosphere than the other inner satellites because of its more remote orbit, located just outside Jupiter's main radiation belt.〔〔(Space Today Online - Exploring Jupiter - The Cratered Moon Callisto )〕
Callisto is composed of approximately equal amounts of rock and ices, with a mean density of about , the lowest density and surface gravity of Jupiter's major moons. Compounds detected spectroscopically on the surface include water ice, carbon dioxide, silicates, and organic compounds. Investigation by the ''Galileo'' spacecraft revealed that Callisto may have a small silicate core and possibly a subsurface ocean of liquid water〔 at depths greater than .〔〔
The surface of Callisto is the oldest and most heavily cratered in the Solar System.〔(Callisto: Overview - Solar System Exploration - NASA )〕 It does not show any signatures of subsurface processes such as plate tectonics or volcanism, with no signs that geological activity in general has ever occurred, and is thought to have evolved predominantly under the influence of impacts.〔 Prominent surface features include multi-ring structures, variously shaped impact craters, and chains of craters (''catenae'') and associated scarps, ridges and deposits.〔 At a small scale, the surface is varied and made up of small, sparkly frost deposits at the tips of high spots, surrounded by a low-lying, smooth blanket of dark material.〔 This is thought to result from the sublimation-driven degradation of small landforms, which is supported by the general deficit of small impact craters and the presence of numerous small knobs, considered to be their remnants.〔 The absolute ages of the landforms are not known.
Callisto is surrounded by an extremely thin atmosphere composed of carbon dioxide〔 and probably molecular oxygen,〔 as well as by a rather intense ionosphere.〔 Callisto is thought to have formed by slow accretion from the disk of the gas and dust that surrounded Jupiter after its formation.〔 Callisto's gradual accretion and the lack of tidal heating meant that not enough heat was available for rapid differentiation. The slow convection in the interior of Callisto, which commenced soon after formation, led to partial differentiation and possibly to the formation of a subsurface ocean at a depth of 100–150 km and a small, rocky core.〔
The likely presence of an ocean within Callisto leaves open the possibility that it could harbor life. However, conditions are thought to be less favorable than on nearby Europa.〔 Various space probes from ''Pioneers 10'' and ''11'' to ''Galileo'' and ''Cassini'' have studied Callisto. Because of its low radiation levels, Callisto has long been considered the most suitable place for a human base for future exploration of the Jovian system.〔
==History==


抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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