Meteoriteista

Meteoriteista is a celestial body that has survived its passage through Earth's atmosphere and landed on the surface. They are remnants from the formation of the solar system, offering valuable clues about its early history. Meteoriteista originate from various sources, primarily asteroids, but also from the Moon and Mars.

These space rocks can vary greatly in size, from microscopic grains to massive boulders weighing many tons. Their composition is also diverse, broadly categorized into stony, iron, and stony-iron types. Stony meteorites are the most common, resembling terrestrial rocks but often containing distinctive minerals like olivine and pyroxene, and sometimes chondrules – small, spherical grains that are evidence of early solar system processes. Iron meteorites are composed primarily of metallic iron and nickel, and stony-iron meteorites are a mixture of both rock and metal.

When a meteorite enters Earth's atmosphere, it experiences intense friction, causing it to heat up and create a bright streak of light known as a meteor or "shooting star." If a fragment survives and reaches the ground, it becomes a meteorite. The impact of larger meteoriteista can create craters, some of which are prominent geological features on Earth. Studying meteoriteista helps scientists understand the composition of other celestial bodies, the processes that shaped our solar system, and the potential for extraterrestrial life. They are a direct link to the cosmos, brought to us for examination.