Origin of Meteors

The origin of meteors has its own shelf in the astronimcal library.   Astronomers believe that an estimated 1,000 tons of meteoric dust and rock enter the Earths atmosphere every day from deep space.  The dust and rock could have come from supernovas(exploding star), collision of meteors, chips off asteroids, and just pieces still floating around from formations of planets and moons.  Another way that meteors form are from comets.  When comets get closer to the sun, the suns heat waves melt the comets ice that was holding the meteoric dust and rock, letting the debris fall.   Some astronomers believe that some comets have held their debris for nearly five million years. 

Streaking Meteor
Image: Night Sky
Image Credit: Summer Stargazing, Terence Dickonson
Meteorite next to coin
Image: Meteorites
Image Credit: Arachnauts Meteorite Gallery
Between Mars and Jupiter, there is a belt of meteoric rock that just orbits between the planets.  Sometimes pieces chip off and randomly fall to the Earth, and these are called sporadics. 
Astronomy Home
Click here to go back.

Created by ThinkQuest Team 23830
Last Updated August 28, 1998.
All images, unless otherwise credited, are credit of M. Mathis, 1998.