1.8" Canyon Diablo Iron Meteorite (52.7 g) - Arizona

Iron Meteorite Care - Important!

Iron meteorites can be susceptible to rusting and deterioration due to moisture in the atmosphere; proper care includes avoiding handling them with your bare hands, as the oils form your skin can affect the metal, and especially keeping them in moisture-free environments. This is particularly important in areas with high humidity, such as Florida. All iron meteorite material we sell has been stabilized in some way, which will help with this issue, but care still needs to be taken to keep your treasure in good condition. Keep iron meteorites stored in a moisture-free environment, preferably with a corrosion inhibitor such as an enclosed display case with a dehumidifier or desiccants.

It's suggested that you inspect your specimen at least once a month, looking specifically for spots that appear discolored (brown or yellow in hue). If a rust spot develops, immediate attention is required to prevent it from spreading. It can be treated by gently rubbing the spot with a cotton swab dipped in CLR (Calcium, Lime, and Rust remover). Repeat this process until the rust color is removed. The meteorite should then be rinsed with alcohol (100% pure is best).

Following this process, it is safe to bake the meteorite for about an hour at 200˚ F (150˚ F for stony-iron meteorites like pallasites) to remove any remaining moisture. Be careful when removing it from the oven as the metal will be hot. A bath in ATF (automatic transmission fluid) or high quality, light oil is suggested while the meteorite is still hot. Once cooled, remove any excess fluid and place it back in its moisture free environment.

The Canyon Diablo Meteorite

About 50,000 years ago, the giant Canyon Diablo meteor hit the dry Arizona desert at an incredible speed, almost 48,280 kilometers per hour. The resulting blast created an impact crater about 3/4 of a mile wide and about 600 feet deep. Most of the meteor was vaporized, but some fragments survived: the largest found is about 639 kilograms. The meteor itself likely weighed up to 63,000 tons, about 30 tons of which have been recovered.



Assays of the recovered meteorite fragments yielded about 7% nickel and 1/3 oz per ton platinum. In some specimens, tiny black nanodiamonds called "carbonados" were discovered inside graphite and troilite nodules. These carbonados were probably formed by the shock wave of the meteor's collision with earth.

About Iron Meteorites

Iron type meteorites are composed primarily of iron and nickel, and are the remnants of differential cores torn apart at the beginning of the solar system. These metallic meteorites are often the easiest to identify after millions of years post-impact because they are quite different from terrestrial material, especially when it comes to their mass-to-surface area ratio. They are exceptionally heavy for their size since iron is a high-density metal: this is also why the Earth's core is nickel-iron. As planets form, the densest metals form gravitational centers, bringing more and more material into their gravitational pull. In the solar system's rocky planets, these dense materials are most often nickel and iron.

Most iron meteorites have distinctive, geometric patterns called Widmanstätten patterns, which become visible when the meteorite is cut and acid etched. These patterns are criss-crossing bands of the iron-nickel alloys kamacite and taenite that slowly crystalized as the core of the meteorites' parent bodies slowly cooled. Such large alloy crystallizations for mover millions of years and do not occur naturally on Earth, further proving that iron meteorites come from extraterrestrial bodies.