Iron Meteorites

Iron Meteorites

Iron meteorites, composed primarily of iron and nickel, are fascinating remnants of the early solar system, originating from the cores of ancient asteroids. Unlike their rocky counterparts, these meteorites have a distinct metallic luster and often exhibit intricate Widmanstätten patterns—crystalline structures that form during the slow cooling of molten metal over millions of years. Their dense, heavy composition makes them stand out among meteorite types, and their rarity adds to their scientific and aesthetic appeal. Often found in arid or polar regions where they are less weathered, iron meteorites offer valuable insights into the processes that shaped our solar system’s formation.