There are a large number of asteroids found in the solar system. Most of them circle the sun in the same manner as planets do. Some of them may circulate around the nearest planet, too. The asteroids are rock-like in appearance and contain different minerals. They are believed to be created by the Big Bang that occurred when the stars and planets came into being. The origin of asteroids is believed to have occurred almost 13.7 billion years ago. There are at least 1,113,527 asteroids in the solar system today. Vesta is the largest of them with a diameter of 530 kilometres, while the smallest measures less than 10 metres across. The combined mass of all known asteroids today is far less than that of earth’s satellite, i.e. the moon. The asteroids are rich in minerals and space missions like ISRO and NASA are contemplating mining them to retrieve large amounts of nickel, iron, and other elements/metals.
The first few asteroids were discovered in the 19th century. William Herschel first used the term. The scientists began to refer to asteroids as “minor planets” by 1802. The practice of attributing names to different asteroids was discontinued in 1851 with the newly discovered rocks designated a number instead of names. This particular rock is now known both as an asteroid and a dwarf planet. It is the “International Astronomical Union (IAU)” that deals with the naming of celestial bodies including stars, planets, and asteroids. The body has become less strict about the naming process at present. Collectively known as “star rocks,” there are many asteroids named after fictional characters, musicians, and the crew of the doomed Space Shuttle Columbia. The IAU has discontinued the practice of naming asteroids after pets.
Asteroids are primarily found in the asteroid belt seen between Mars and Jupiter. Three of the biggest asteroids are sphere-like in shape, however, with their composition differing greatly. They form three distinct groups based on the chemicals inside.
Asteroid | Meteor |
A small planet like structure | Falling Stars or meteorites |
Orbits the sun in an elliptical path | It follows an elliptical path around the sun but may be distracted by the gravitational pull of other heavier bodies |
It is a remnant of the early planet created with the solar system | It consists of dust-like particles created by the collision of heavenly bodies |
The shape is jagged and irregular | It is made of dust-like particles with the shape not being evident |
There is no atmosphere | There is no atmosphere causing the meteors to burn while falling on earth |
It is 1 to 100 kilometres in diameter | It measures less than 10 metres in diameter |
Asteroids are heavenly bodies found in different areas of the solar system. They have a mass much less than that of a planet. Termed as minor planets, they differ sharply from planets, comets, and meteorites. They are believed to have formed billions of years ago with the creation of the Universe. Each asteroid is different, with some of them circling the closest planet instead of the sun. There are more than 1,113,527 in the solar system at present. Many are found in the asteroid belt located between Mars and Jupiter. They contain a rich deposit of various metals and minerals.