HAMMADAH AL HAMRA 346 Type L6 Meteorite - 52 g






Over 20 years collecting meteorites; former museum curator and experienced restorer.
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Hammadah al Hamra 346 L6 meteorite from Libya, a complete specimen that fell in April 2018, weighing 52 g.
Description from the seller
Fantastic complete L5-type meteorite due to its low iron content.
Known formerly as Ghadamis, this meteorite is thought to have fallen in April 2018 and it has only now finally been officially classified.
In this superb meteorite, you can observe a multitude of meteorite features, such as regmaglypts, fusion crust, and flight lines.
Regmaglyphs are produced when the air shapes the hot surface of the meteorite.
You can also observe the fusion crust created by the high temperatures reached during entry into the atmosphere, temperatures that approach 7000°C and that is the reason why spacecraft are fitted with a protective thermal shield.
The flight lines are produced as the material aligns in the direction of the fall.
The contraction crust originates when the meteorite cools rapidly, and the fusion crust cracks, leaving this rare pattern to behold.
At Expometeoritos, we specialize in divulgation, talks, workshops, analyses, classification, and exhibitions of meteorites.
We are members of:
.- IMCA (International Meteorite Collectors Association) #8187
.- Meteoritical Society
.- American Meteor Society
All of our pieces are certified and, in addition, we provide the chemical composition analysis if the piece’s value exceeds €300, performed at our facilities by X-ray spectroscopy.
Seller's Story
Fantastic complete L5-type meteorite due to its low iron content.
Known formerly as Ghadamis, this meteorite is thought to have fallen in April 2018 and it has only now finally been officially classified.
In this superb meteorite, you can observe a multitude of meteorite features, such as regmaglypts, fusion crust, and flight lines.
Regmaglyphs are produced when the air shapes the hot surface of the meteorite.
You can also observe the fusion crust created by the high temperatures reached during entry into the atmosphere, temperatures that approach 7000°C and that is the reason why spacecraft are fitted with a protective thermal shield.
The flight lines are produced as the material aligns in the direction of the fall.
The contraction crust originates when the meteorite cools rapidly, and the fusion crust cracks, leaving this rare pattern to behold.
At Expometeoritos, we specialize in divulgation, talks, workshops, analyses, classification, and exhibitions of meteorites.
We are members of:
.- IMCA (International Meteorite Collectors Association) #8187
.- Meteoritical Society
.- American Meteor Society
All of our pieces are certified and, in addition, we provide the chemical composition analysis if the piece’s value exceeds €300, performed at our facilities by X-ray spectroscopy.
