The Asteroid Belt
Scattered in orbits around the sun are bits and pieces of rock left over from the dawn of the solar system. Most of these asteroids orbit between Mars and Jupiter in a grouping known as the Main Asteroid Belt. Check out our big gallery of asteroid pictures, or read below to learn about this belt and how it formed.
Origin & Location
Early in the life of the solar system, dust and rock circling the sun were pulled together by gravity into planets. But Jupiter, the largest planet, kept a number of the pieces from coalescing into another planet. Instead, its gravity disrupted the formation process, leaving an array of unattached asteroids.
The Main Asteroid Belt lies more than two-and-a-half times as far as Earth does from the sun. It contains billions — maybe even trillions — of asteroids. Most of these are relatively small, from the size of boulders to a few thousand feet in diameter. But some are significantly larger. Vesta, Pallas, and Hygiea are others than 250 miles (400 kilometers) long and bigger. The region also contains the dwarf planet Ceres. At 590 miles (950 km) in diameter, or about a quarter of the size of our moon, Ceres is round yet is considered too small to be a full-fledged planet. However, it makes up approximately a third of the mass of the asteroid belt.
The Main Belt once contained enough material to form a planet nearly four times as large as Earth. Jupiter's gravity not only stopped the creation of such a planet, it also swept most of the material clear, leaving far too little behind for a planet of any size to form. Indeed, if the entire mass of the Main Belt could somehow create a single body, it would weigh in at less than half of the mass of the moon.
Other solar systems are thought to contain their own asteroid belts.
Most of the asteroids in the Main Belt are made of rock and stone, but a small portion of them contain iron and nickel metals. The remaining asteroids are made up of a mix of these, along with carbon-rich materials. Some of the more distant asteroids tend to contain more ices. Although they aren't large enough to maintain an atmosphere, but there is evidence that some asteroids contain water.
Some asteroids are large, solid bodies—there are more than 16 in the belt with a diameter greater than 150 miles (240 km). Others are piles of rubble held together by gravity. Most asteroids aren't quite massive enough to have achieved a spherical shape and instead are irregular, often resembling a lumpy potato. The asteroid 216 Kleopatra resembles a dog bone.
In 2007, NASA launched a mission, Dawn, to visit two of the largest bodies in the Main Asteroid Belt, Ceres and Vesta. Dawn reached Vesta in 2011 and remained there for over a year. It should reach Ceres in 2015. [Asteroid Vesta and NASA's Dawn Spacecraft]
Discovery of the Asteroid Belt
The 18th century astronomer Johann Titius noted a mathematical pattern in the layout of the planets and used it to predict the existence of one between Mars and Jupiter. Astronomers scoured the heavens in search of this missing body. In 1800, 25 astronomers formed a group known as the Celestial Police, each searching 15 degrees of the zodiac for the missing planet. But the discovery of the first body in this region came from a nonmember, Italian astronomer Giuseppe Piazzi: he named it Ceres. A second body, Pallas, was found a little over a year later.
For some time, both of these objects were referred to as planets. But the discovery rate of these objects increased, and by the beginning of the 19th century, over a hundred had been found. Scientists quickly realized that these were too small to be considered planets, and they began to be known as asteroids.
—Nola Taylor Redd