Odessa - Metallic Meteorite - 360 g - (1)






Over 20 years collecting meteorites; former museum curator and experienced restorer.
€80 | ||
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€75 |
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ODESSA metallic meteorite from Texas, United States (IAB-MG) weighing 360 g.
Description from the seller
A complete piece of great beauty, with a multitude of shapes.
As the meteorite disintegrated upon impact, it is very difficult to find pieces for sale, since only a few specimens from this Odessa fall have been collected.
A metallic meteorite is composed, primarily, of iron and nickel.
In reality, it is a piece of the asteroid's core. In the differentiation process, when the asteroid is a ball of magma during its formation, iron and nickel settle at the center of the asteroid, as they are the heaviest elements. After cooling, the asteroid's metallic core is formed. Through catastrophic collisions, the asteroid and its core break apart and those fragments remain in space until some piece falls to our planet. It is estimated that they represent 5.7% of falls.
The crater was identified by Daniel Barringuer, the same person who recognized the famous METEOR CRATER in Arizona, in the late 1920s, and the first Odessa meteorite was described in 1922.
The main crater measures 160 meters in diameter and 2 meters in depth.
At Expometeoritos, we handle outreach, talks, workshops, analyses, classification, and exhibitions of meteorites.
We are members of:
.- IMCA (International Meteorite Collectors Association) #8187
.- Meteoritical Society
.- American Meteor Society
All our pieces are certified and, furthermore, we provide the analysis of the chemical composition if the piece's value exceeds €300, performed at our facilities by X-ray spectroscopy.
Seller's Story
A complete piece of great beauty, with a multitude of shapes.
As the meteorite disintegrated upon impact, it is very difficult to find pieces for sale, since only a few specimens from this Odessa fall have been collected.
A metallic meteorite is composed, primarily, of iron and nickel.
In reality, it is a piece of the asteroid's core. In the differentiation process, when the asteroid is a ball of magma during its formation, iron and nickel settle at the center of the asteroid, as they are the heaviest elements. After cooling, the asteroid's metallic core is formed. Through catastrophic collisions, the asteroid and its core break apart and those fragments remain in space until some piece falls to our planet. It is estimated that they represent 5.7% of falls.
The crater was identified by Daniel Barringuer, the same person who recognized the famous METEOR CRATER in Arizona, in the late 1920s, and the first Odessa meteorite was described in 1922.
The main crater measures 160 meters in diameter and 2 meters in depth.
At Expometeoritos, we handle outreach, talks, workshops, analyses, classification, and exhibitions of meteorites.
We are members of:
.- IMCA (International Meteorite Collectors Association) #8187
.- Meteoritical Society
.- American Meteor Society
All our pieces are certified and, furthermore, we provide the analysis of the chemical composition if the piece's value exceeds €300, performed at our facilities by X-ray spectroscopy.
