Asteroid belt

Helping orphans the way you would do it

The "Asteroid Belt" is a region of the solar system falling roughly between the planets Mars and Jupiter where the greatest concentration of asteroid orbits can be found. The term asteroid belt can also generally describe a region of concentrated asteroids with similar orbits.

Origin

It is believed that, during the first million years of the solar system history, planets formed by accretion of planetesimals. Repeated collisions led to the familiar rocky planets and to the gas giants cores.

However, in this zone of the system the strong gravity of Jupiter inhibited the final stages, and the planetesimals could not form a single planet. The planetesimals instead continued to orbit the Sun as before. In this sense the asteroid belt can be considered a relic of the primitive Solar System, but many observations point to an active evolution of the physical conditions so the asteroids themselves are not particularly pristine. Instead, the objects in the outer Kuiper belt are believed to have had little change since the solar system's formation.

Asteroid belt environment

Despite this, tens of thousands of asteroids are currently known, and estimates of the total number are in millions range. About 220 of them are larger than 100 km. The biggest asteroid belt member is Ceres, which is about 1000 km across. The total mass of the Asteroid belt is estimated to be 2.3×10²¹ kilograms (of which more than a third is accounted for by Ceres), which is less than that of Pluto.

The high population makes for a very active environment, where collisions between asteroids occur very often (in astronomical terms). A collision may fragment an asteroid in numerous small pieces (leading to the formation of a new asteroid family), or may glue two asteroids together if it occurs at low relative speeds. After five billion years, the current Asteroid belt population bears little resemblance to the original one.

Asteroid belts are a staple of science fiction stories, since they are always portrayed as being so dense that adventurous measures must be taken to avoid an impact. In reality, the asteroids are spread over such a high volume that it would be highly improbable to even pass close to a random asteroid. For example, the numerous space probes sent to the outer solar system, just across the main asteroid belt, never had any problems, and asteroid rendezvous missions have elaborate targeting procedures.

See also: Asteroid, Asteroid family, Centaur

The Solar System

(For other objects and regions, see: List of solar system objects, Astronomical objects)