Asteroids, also called minor planets or planetoids, are a class of astronomical objects. The term asteroid is generally used to indicate a diverse group of small celestial bodies in the solar system that orbit around the Sun. "Asteroid", Greek for "star-like", is the most commonly used word in the English literature for minor planets, which is the term preferred by the International Astronomical Union, while other languages prefer planetoid, Greek for "planet-like", because it more or less describes what they are. In late August 2006, the IAU introduced a new class "small solar system bodies" (SSSB), to include most objects thus far classified as minor planets and comets. At the same time, the term "dwarf planet" was created for classifying the largest of the minor planets.
The first asteroid to be discovered, Ceres, is the largest asteroid known to date and is now classified as a dwarf planet. All others are currently classified as small solar system bodies. The vast majority of asteroids are found within the main asteroid belt, with elliptical orbits between those of Mars and Jupiter. It is thought that these asteroids are remnants of the protoplanetary disc, and in this region the accretion of planetesimals into a larger planet or planets during the formative period of the solar system was prevented by large gravitational perturbations by Jupiter. Some asteroids have moons or are found in co-orbiting pairs known as binary systems.
Celina Erika · Sun Mar 09, 2008 @ 02:38am · 0 Comments |