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Io (/ˈaɪ.oʊ/), or Jupiter I, is the innermost and third-largest of the four Galilean moons of the planet Jupiter. It is the fourth-largest moon in the Solar System, has the highest density of all of them, and has the lowest amount of water (by atomic ratio) of any known astronomical object in the Solar System. It was discovered in 1610 by Galileo Galilei and was named after the mythological character Io, a priestess of Hera who became one of Zeus's lovers.

INTO JAPANESE

イオ(/ˈaɪ.oʊ/)、または木星Iは、惑星木星の4つのガリラヤ衛星の中で最も内側と3番目に大きい。太陽系で4番目に大きい月で、その中で最も密度が高く、太陽系の既知の天体の中で最も低い水量(原子比)を持っています。それはガリレによって1610年に発見されました

BACK INTO ENGLISH

Io (/ˈaɪ.oʊ/), or Jupiter I, is the innermost and third largest of the planet Jupiter's four Galilee moons. It is the fourth largest moon in the solar system, the densest of which has the lowest amount of water (atomic ratio) of any known celestial body in the solar system. It was discovered in 1610 by Galilee

INTO JAPANESE

イオ(/ˈaɪ.oʊ/)、または木星Iは、木星の4つのガリラヤ衛星の中で最も内側と3番目に大きい。太陽系で4番目に大きい月で、太陽系内の既知の天体の中で最も密度の高い水量(原子比)を持っています。それはガリラヤによって1610年に発見されました

BACK INTO ENGLISH

Io (/ˈaɪ.oʊ/), or Jupiter I, is the innermost and third largest of Jupiter's four Galilee moons. It is the fourth largest moon in the solar system and has the densest amount of water (atomic ratio) of any known celestial body in the solar system. It was discovered in 1610 by Galilee

INTO JAPANESE

イオ(/ˈaɪ.oʊ/)、または木星Iは、木星の4つのガリラヤ衛星の中で最も内側と3番目に大きい。太陽系で4番目に大きい月で、太陽系の既知の天体の中で最も密度の高い量の水(原子比)を持っています。それはガリラヤによって1610年に発見されました

BACK INTO ENGLISH

Io (/ˈaɪ.oʊ/), or Jupiter I, is the innermost and third largest of Jupiter's four Galilee moons. It is the fourth largest moon in the solar system and has the densest amount of water (atomic ratio) of any known celestial body in the solar system. It was discovered in 1610 by Galilee