Meteorites

Meteorites are solid fragments of meteoroids that survive their passage through the Earth's atmosphere and land on the Earth's surface. They originate from asteroids, comets, or even planets, breaking off from these celestial bodies and traveling through space. When a meteoroid enters the atmosphere and produces a visible streak of light, it is called a meteor. If it survives the intense heat and pressure during this process and reaches the ground, it is classified as a meteorite. Meteorites come in various types, including stony, metallic, and stony-iron, reflecting their diverse chemical compositions. They provide valuable scientific insights into the early solar system, the formation of planets, and the history of celestial bodies. Meteorites can vary greatly in size, from tiny grains to large masses weighing hundreds of kilograms. Collecting and studying meteorites is of great interest to both scientists and enthusiasts, as they can reveal clues about the universe's origins and the processes that shaped it.