The most common meteorites that hit Earth are stony meteorites, primarily composed of silicate minerals and rock-forming elements like oxygen, silicon, magnesium, and iron. Among these, chondrites are the most prevalent type, containing small spherical inclusions called chondrules. Iron meteorites, which are composed mainly of metallic iron and nickel, are less common but also significant. Overall, these meteorites provide valuable insights into the early solar system and the formation of planetary bodies.
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