Keolests

Keolests are a group of small, stony meteorites that are believed to have originated from the asteroid belt between Mars and Jupiter. They are named after the Keota meteorite, which fell in Iowa, USA, in 1879. Keolests are characterized by their low iron content, typically ranging from 5% to 10%, and their high abundance of silicate minerals. They are further classified into two main types: H and L, based on their chemical composition. H-type keolests are rich in iron and magnesium, while L-type keolests are rich in iron and calcium. Keolests are of particular interest to scientists because they provide valuable insights into the early solar system and the processes that shaped it. They are also sought after by collectors due to their unique composition and aesthetic appeal. Despite their relatively small size, keolests have a significant impact on our understanding of the universe and its origins.