Meteorite

A meteorite is a solid piece of debris from outer space that originates from a variety of sources, including comets, asteroids, and meteoroids, that survives its passage through the Earth's atmosphere and impacts the surface. Meteorites are often categorized into three primary groups: stony meteorites (the most common type, made of silicate minerals), iron meteorites (composed largely of metallic iron-nickel), and stony-iron meteorites (a mix of stone and metal). The term "meteorite" is derived from the Greek word meteōros, meaning "suspended in the air," and lithos, meaning "stone." In Hebrew, the term is מִטְעוֹרִיט (mite'orit), while in other languages, it is known as Meteorit in German, Météorite in French, and Meteorito in Spanish and Italian. Meteorites provide valuable insights into the composition and history of the solar system, as they often contain ancient materials that predate the formation of Earth. The study of meteorites, known as meteoritics, is a vital branch of planetary science.