Linked from

The 26 pages that link to Asteroid belt, each with the reason it gives.

• AsteroidBroader topic: It is the main region where asteroids are found.

• Late Heavy BombardmentRelated: Changes to its population have been proposed as one source of early inner-planet impactors.

• Solar System formationRelated: Its surviving planetesimals preserve evidence of incomplete accretion and Jupiter’s influence.

• CeresNarrower topic: Ceres is the belt’s largest resident, but its size sets it apart from typical asteroids.

• Planetary ringsCompared with: Both contain orbiting solids, but the asteroid belt is heliocentric and much more dispersed.

• Grand Tack hypothesisRelated: Jupiter’s migration can scatter material into the belt from distinct source regions.

• Zodiacal lightRelated: Collisions among asteroids supply some of the interplanetary dust.

• Impact eventRelated: Collisions among its asteroids produce fragments that can eventually cross Earth's orbit.

• Kirkwood gapNarrower topic: Kirkwood gaps are depleted zones within this population.

• Pioneer 10Related: Pioneer 10’s safe crossing helped show that spacecraft could traverse this region.

• VestaNarrower topic: Vesta orbits within this population of rocky bodies.

• Poynting–Robertson effectRelated: The effect can transport small collision fragments from the belt toward the Sun.

• Minor planetBroader topic: Its asteroids form the most familiar and numerous minor-planet population.

• Planetary accretionRelated: Its surviving bodies retain clues to accretion disrupted by Jupiter's gravitational influence.

• Asteroid familyNarrower topic: Most known asteroid families occupy this population.

• Trojan asteroidNarrower topic: The main belt is a distinct population from asteroids trapped in a planet’s co-orbital regions.

• Asteroid collisionNarrower topic: Its large population makes repeated collisions possible over Solar System history.

• 4 VestaNarrower topic: Vesta orbits within this region, where its early history unfolded.

• FomalhautCompared with: Fomalhaut’s dusty ring is often compared with a much larger, extrasolar analogue of the Solar System’s belt.

• Titius–Bode lawBroader topic: Its location near the predicted missing-planet orbit became the law’s strongest apparent success.

• 2 PallasNarrower topic: Pallas follows an unusually inclined orbit through this population of rocky bodies.

• 243 IdaNarrower topic: Ida follows a main-belt orbit within this population.

• Interplanetary mediumRelated: Collisions and surface impacts among its bodies release dust into interplanetary space.

• 10 HygieaNarrower topic: Hygiea orbits within this broad population of rocky and metallic bodies.

• Heinrich Wilhelm Matthias OlbersNarrower topic: Pallas and Vesta belong to the population Olbers helped establish as a distinct group of solar-system objects.

• Minor-planet moonNarrower topic: Surveying this population helps establish how frequently main-belt asteroids have moons.