Libya Crystal Tektite, with cristobalite. - 1.96 kg






Over 20 years collecting meteorites; former museum curator and experienced restorer.
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Cristal de Libia is a tectite meteorite with cristobalite, originating from Libia and Egypt, weighing 1.955 kg and featuring gas bubbles.
Description from the seller
Libyan Crystal is pure silica, formed in the Sahara desert, between Libya and Egypt by the impact of a large meteorite 28 million years ago.
The Libyan Crystal has been used as tools and jewelry in antiquity, with Pharaoh Tutankhamun's scarab brooch being the most famous piece.
Tectites are the result of the melting and crystallization of terrestrial material due to the high temperatures and pressures sometimes generated by the impact of a large meteorite on the Earth's surface.
Bubbles can be observed inside, which enclose gas, very useful scientifically to analyze and understand how tectites form. Additionally, we can observe traces of non-crystallized sediments.
They are increasingly scarce, particularly those of a considerable size like the one offered in this lot. If it is already difficult to find a meteorite, a tectite is much more difficult to find because this phenomenon does not always occur.
At Expometeoritos, we handle dissemination, 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, in addition, we provide the chemical composition analysis if the piece's value exceeds €300, performed at our facilities by X-ray Spectrometry.
Seller's Story
Libyan Crystal is pure silica, formed in the Sahara desert, between Libya and Egypt by the impact of a large meteorite 28 million years ago.
The Libyan Crystal has been used as tools and jewelry in antiquity, with Pharaoh Tutankhamun's scarab brooch being the most famous piece.
Tectites are the result of the melting and crystallization of terrestrial material due to the high temperatures and pressures sometimes generated by the impact of a large meteorite on the Earth's surface.
Bubbles can be observed inside, which enclose gas, very useful scientifically to analyze and understand how tectites form. Additionally, we can observe traces of non-crystallized sediments.
They are increasingly scarce, particularly those of a considerable size like the one offered in this lot. If it is already difficult to find a meteorite, a tectite is much more difficult to find because this phenomenon does not always occur.
At Expometeoritos, we handle dissemination, 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, in addition, we provide the chemical composition analysis if the piece's value exceeds €300, performed at our facilities by X-ray Spectrometry.
