Rasteroids

Rasteroids are a type of asteroid that are characterized by their irregular, often jagged shapes, and their composition primarily of rocky materials. They are remnants from the early solar system and are believed to be the source of many meteorites that fall to Earth. Rasteroids are typically found in the asteroid belt between Mars and Jupiter, but they can also be found in other regions of the solar system, including near-Earth space.

The term "rasteroid" is not officially recognized by the International Astronomical Union, but it is commonly used in the scientific community to describe these types of asteroids. Rasteroids are distinguished from other types of asteroids, such as carbonaceous chondrites and stony-iron meteorites, by their composition and structure.

Rasteroids are of particular interest to scientists because they provide valuable insights into the early history of the solar system. By studying the composition and structure of rasteroids, scientists can learn more about the processes that shaped the solar system billions of years ago. Additionally, rasteroids are potential targets for future space missions, as they may contain valuable resources such as water and minerals.

In summary, rasteroids are a type of asteroid characterized by their irregular shapes and rocky composition. They are remnants from the early solar system and are of particular interest to scientists due to their potential to provide insights into the early history of the solar system and as potential targets for future space missions.