4.90" Etched Odessa Iron Meteorite Slice (106.3 g) - Texas

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.

About The Odessa Iron Meteorite

The Odessa iron meteorite is an iron octahedrite (IAB-MG) meteorite collected in 1922 within Ector County, Texas. A total of approximately 1.6 tons of meteorite fragments were collected in and around the Odessa Crater in Texas, which was the second recognized impact crater in the United States. This crater is estimated to be about 63,500 years old and was found by a rancher who stumbled upon it while looking for a lost calf.

It is believed that the meteor broke into two significant fragments. The larger would be responsible for the main crater, and the smaller for the eastern part of the crater. Data suggests that these pieces had a near simultaneous impact, which would create the strange shape of the crater. According to extensive geological research by A&M Graduate Charles Edward Stanford, the original crater was approximately 394 Ft. in diameter, and approximately 115 Ft. in depth.

Meteoritical Bulletin: Entry for Odessa (Iron)

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.