The asteroid belt is a zone in space between the orbits of Mars and Jupiter in which most of the asteroids in the Solar System, probably millions of them and of different sizes, are rotating in orbit around the sun. It is also known by the name of main belt in order to make a correct distinction between it and the smaller bodies that are in the solar system. We also find inside the belt, the dwarf planet called Ceres.
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The asteroid belt is an area in the outer space between Mars and Jupiter where thousands of asteroids are located, varying in size and shape, and where we also find the dwarf planet Ceres.
During the 18th century, astronomers created a pattern in several planets’ orbits that gave rise to the Titius-Bode law, which said how much space existed between the planets. In addition to this observation, they realized that there were large and small objects orbiting between Mars and Jupiter, and from here, was born the term asteroid, after they realized the large number of them, the term asteroid belt was born.
The current theory about the origin of the asteroid belt has been proposed by researchers at the University of Bordeaux. It suggests that, at an earlier point in history, the belt was overpopulated and that, through Jupiter’s gravitational pull, it threw approximately 99% of its material out of the solar system. They suggest that, then, the belt emerged from an empty space that then gradually filled with material that had been thrown from other planets. So, we can say that the asteroids reached the belt as it was created.
The belt is located between the orbits of Mars and Jupiter where we find thousands of asteroids occupying a strip located at distances between 2 and 4 AU from the sun, this means between 300 and 600 kilometers. It is important to mention that 1 AU is an astronomical unit that marks the average distance between the sun and the earth and is equal to 149,597,871 km.
Some of its main features are:
The only planet we find in the asteroid belt has the name of Ceres and has been classified as a dwarf planet because its gravity has shaped it spherically. Towards 2006, it was considered to be the largest asteroid, but the theory changed from that year on. It has a magnitude of 3.32 more than any other body inside the belt and is formed by a silicate nucleus and a water layer as ice.
Briceño V., Gabriela. (2019). Asteroid belt. Recovered on 24 February, 2024, de Euston96: https://www.euston96.com/en/asteroid-belt/