词条 | Compositional data for selected solar system objects |
释义 | Compositional data for selected solar system objects Table Compositional data for selected solar system objects object distance from Sun (AU)* mean density (g/cm3) general composition Sun -- 1.4 hydrogen, helium Mercury 0.4 5.4 iron, nickel, silicates Venus 0.7 5.2 silicates, iron, nickel Earth 1 5.5 silicates, iron, nickel Moon 1 3.3 silicates Mars 1.5 3.9 silicates, iron, sulfur asteroids (asteroid) 2-4.5 (main and outer belts) typically 2-4 silicates, iron, nickel Jupiter 5.2 1.3 hydrogen, helium Io 5.2 3.6 silicates, sulfur Europa 5.2 3.0 silicates, water ice (crust) Ganymede 5.2 1.9 water ice, silicates Callisto 5.2 1.8 water ice, silicates Saturn 9.5 0.7 hydrogen, helium Tethys 9.5 1.0 water ice Titan 9.5 1.9 water ice, silicates, organics Centaur objects (Centaur object) 5-30 (mainly between orbits of Jupiter and Neptune) possibly less than 1 presumed similar to that of comets: water ice, other ices, traces of silicates Uranus 19.2 1.3 ices, silicates, hydrogen, helium Neptune 30.1 1.6 ices, silicates, hydrogen, helium Triton 30.1 2.0 water ice, silicates, organics Pluto 39.5 2.0 water ice, silicates, organics Kuiper belt objects 30-50 (main concentration) possibly less than 1 presumed similar to that of comets: water ice, other ices, traces of silicates, organics Oort cloud objects 20,000-100,000 possibly less than 1 presumed similar to that of comets: water ice, other ices, traces of silicates, organics *One astronomical unit (AU) is the mean distance of Earth from the Sun, about 150 million km. See as table: ![]() |
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