Atmospheric entry refers to the journey that a celestial object takes as it penetrates the Earth's atmosphere. This process subjects the object to great thermal stress due to friction with air molecules, which causes the object's surface to heat up dramatically.
As a meteor enters the atmosphere, the rapid increase in temperature often causes it to combust. The bright light produced from this combustion is what we see when we look up at a shooting star. Most meteors completely disintegrate before reaching the surface. However, larger fragments might survive the atmosphere, becoming meteorites.
- The speed and angle of entry are critical in determining whether a meteor becomes a meteorite.
- Larger size and higher velocity increase the likelihood of surviving atmospheric entry.