Meteorites News

Meteorites are solid pieces of debris from objects such as asteroids or comets that originate in outer space and survive their passage through the Earth’s atmosphere to reach the ground. These extraterrestrial materials provide invaluable information about the early solar system’s conditions and the processes that led to the formation of planetary bodies. Meteorites are classified into three main types: stony meteorites, which are made up of minerals rich in silicon and oxygen; iron meteorites, which consist largely of metallic iron-nickel; and stony-iron meteorites, which contain both metallic and rocky materials. Scientists study meteorites to gain insights into the composition of other planets and the history of collisions and material exchange in the solar system. Additionally, certain meteorites have shown to contain organic compounds, offering clues about the potential pathways for the development of life on Earth.