Generally, a band of asteroids which encircles a star, often where a planet would normally have formed. It may form the main "world" in a stellar system, as in the Barnard Belt, or it may simply be a region between planets where no planet coalesced, as in the Sol Belt.
Asteroids belts have a number of possible origins. Generally, a planet failed to coalesce during the formation of its star system, usually because of gravitational forces from a nearby gas giant, or because of the disruptive influence of multiple stars (Belts are for this reason far more common in systems with multiple suns than in one star systems).
Much more rarely, a planet has been torn apart by tidal forces, leaving a path of scattered debris. There are also a few instances when "planet-buster" weapons were used, such as Muno Gamma, destroyed by Geminga Orthodoxy during the Second Empires War.
Asteroid belts usually include several thousand asteroids, along with billions of smaller fragments, some as tiny as grains of dust, which are often the result of collisions between asteroids. Because of the ease of extracting resources, asteroid belts are highly sought after by developers.
Belter - Text by M. Alan Kazlev  A person who practices the profession of asteroid prospector and miner (belt mining), usually working alone or with a small number of partners.  Any resident of an asteroid belt, including citizens of civilised belts such as the Barnard Belt, Sol Main Belt, the Mirthsen-Simoris Spinward Marches, or any of the other innumerable belts in known space. Many belters have never been in a spaceship, let alone set foot on a planet or large orbital.
Kuiper Belt - Text by M. Alan Kazlev In the Solar System, the region beyond Neptune. It includes more than 70,000 small objects, a number up to asteroidal size. It is located from 30 to 50 A.U.'s and was discovered in 1992. The Kuiper belt may be the source of the short-period comets (like Halley's comet). The Kuiper belt was named for the Dutch-American astronomer Gerard P. Kuiper, who predicted its existence in 1951. In general, any belt beyond the outermost large planet of a solar system, consisting of mainly icy objects (ice dwarfs and ice planetisimals).