M-type asteroids are known as metallic asteroids and are composed primarily of iron and nickel.

C-type asteroids are the most common type, accounting for approximately 75% of known asteroids.

D-type asteroids are known as icy asteroids and are rich in water ice and other volatile compounds.

S-type asteroids are composed primarily of silicate minerals, such as olivine and pyroxene.

V-type asteroids are believed to be fragments of a larger body that broke apart due to a collision.

C-type asteroids are composed primarily of carbon-rich compounds, such as graphite and organic molecules.

S-type asteroids have a high albedo, meaning they reflect a significant amount of sunlight.

M-type asteroids are composed primarily of metal, such as iron and nickel.

D-type asteroids are commonly found in the Trojan group, which are asteroids that share Jupiter's orbit.

V-type asteroids are composed primarily of basaltic material, which is a type of igneous rock.

C-type asteroids have a low albedo, meaning they absorb a significant amount of sunlight.

D-type asteroids are composed primarily of water ice and other volatile compounds.

C-type asteroids are commonly found in the Hilda group, which are asteroids that share Jupiter's orbit but are located further away from the Sun.

A-type asteroids are composed primarily of silicate minerals, similar to S-type asteroids, but with a higher abundance of pyroxene.

S-type asteroids have distinct spectral features that allow astronomers to identify them.