HAMMADAH AL HAMRA 346 Type L6 Meteorite - 60 g






Over 20 years collecting meteorites; former museum curator and experienced restorer.
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Hammadah al Hamra 346, an L6 meteorite from Libya, fell in April 2018 and weighs 60 g.
Description from the seller
Fantastic complete L5-type meteorite due to its low iron content
Known previously as Ghadamis, this meteorite is presumed to have fallen in April 2018 and it has not been until now that it has finally been officially classified.
In this wonderful meteorite, one can observe a multitude of meteorite features, such as regmaglypts, fusion crust, and flight lines.
Regmaglypts are produced by the air as it shapes the hot surface of the meteorite.
Also visible is the fusion crust originated by the very high temperatures reached during entry into the atmosphere, temperatures that approach 7000°C, and this is the reason why spacecraft are fitted with a protective heat shield.
The flight lines are produced by the material orienting itself in the direction of the fall.
The contraction crust forms when the meteorite cools rapidly, and the fusion crust cracks, leaving this rare pattern to be seen.
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 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 previously as Ghadamis, this meteorite is presumed to have fallen in April 2018 and it has not been until now that it has finally been officially classified.
In this wonderful meteorite, one can observe a multitude of meteorite features, such as regmaglypts, fusion crust, and flight lines.
Regmaglypts are produced by the air as it shapes the hot surface of the meteorite.
Also visible is the fusion crust originated by the very high temperatures reached during entry into the atmosphere, temperatures that approach 7000°C, and this is the reason why spacecraft are fitted with a protective heat shield.
The flight lines are produced by the material orienting itself in the direction of the fall.
The contraction crust forms when the meteorite cools rapidly, and the fusion crust cracks, leaving this rare pattern to be seen.
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 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.
