Carbonaceous chondrites are a type of stony meteorite that contain a high abundance of carbon compounds, including organic molecules, amino acids, and even water. They are thought to be some of the most primitive and least processed meteorites, dating back to the early stages of the solar system's formation. Studying carbonaceous chondrites can provide valuable insights into the origins of life on Earth and the potential for life elsewhere in the universe. Researchers analyze the chemical composition, mineralogy, and isotopic signatures of carbonaceous chondrites to learn more about the conditions in the early solar system and the processes that led to the formation of planets and other celestial bodies.