SOLAR SYSTEM
The solar system is the collection of planets, satellites, asteroids, comets, and cosmic dust particles that are mostly in elliptical, coplanar orbits around the Sun. The total mass of the solar system is around 450 times the mass of the Earth and about 1/750 of the mass of the Sun. About three-quarters of that mass is concentrated in the gaseous giant planet Jupiter. Cosmogony, the study of the origin of planets, indicates that the cloud of gas and dust that condensed to form the solar system must have had a mass a few hundred times greater than that of the present system. The planets formed about 4.6 billion years ago and in the early days suffered a great deal from bombardment by asteroids. The rate of these collisions has decreased by about 2,000 times since then. The surface temperature of the planets decreases roughly as the inverse square root of their distance from the Sun. The inner planets, Mercury, Venus, Earth, and Mars have a rock and metal composition, low relative mass, and few satellites. The Moon is unusual in as much as it has a mass of 1/81 of that of Earth. Only Charon, Pluto's satellite, compared to Pluto's mass, has a larger ratio. Phobos and Deimos, the two small satellites of Mars, are thought to be captured asteroids. The outer planets, Jupiter, Saturn, Uranus, and Neptune, have rock-metal cores of ten to twenty or so times the mass of the Earth and are surrounded by huge atmospheres of hydrogen and helium gas. These planets have large collections of orbiting satellites and all have ring systems, although the rings of Saturn are by far the most elaborate. Pluto, the outermost planet, has a mass of only one-quarter that of the Moon and is probably an escaped satellite. There was relatively little matter in the preplanetary nebula in the region of Pluto and it would have taken a long time for a planet to form at that distance from the Sun, so it is probable that there are no major planets beyond Neptune. However, many astronomers believe that a large spherical shell of comets, the Oort-Opik Cloud, surrounds the planetary system and extends almost one-third of the way to the nearest stars. Therefore the planetary system probably has a radius of only about forty times that of the Earth's orbit, whereas the distance to the nearest stars is some 270,000 times the radius of the Earth's orbit.