Deep Space Meteorite

Although they are not the most abundant meteorites that have been found on Earth, many people are most familiar with iron meteorites. This is largely due to the fact that even a casual observer may readily identify them as meteorites due to their metallic content and their considerable weight. Also, since they weather slowly they are often bigger than other types of meteorites. Iron meteorites are believed to have formed in deep space from supernovas or the cores of planets or asteroids. In addition to iron, these meteorites contain a certain amount of nickel, and the two metals combined are exceptionally hard, a characteristic that appears to greatly facilitate their survival in deep space.


© 1995-2022 by Michael W. Davidson and The Florida State University. All Rights Reserved. No images, graphics, software, scripts, or applets may be reproduced or used in any manner without permission from the copyright holders. Use of this website means you agree to all of the Legal Terms and Conditions set forth by the owners.
This website is maintained by our
Graphics & Web Programming Team
in collaboration with Optical Microscopy at the
National High Magnetic Field Laboratory.
Last modification: Tuesday, Jan 06, 2004 at 11:02 AM
Access Count Since September 19, 1995: 29165
Microscopes provided by:
Visit the Nikon website. Visit the Olympus Microscopy Resource Center website.