Out of stock
Oued Awlitis 003 is a brecciated LL6 meteorite of 1141 grams. It was discovered in 2011 near the village of Lemluia in the Western Sahara. Other meteorites have been found in the same area, a lunar meteorite Oued Awlitis 001 and a carbonaceous type CV3 meteorite Oued Awlitis 002. This is a very rich area where other meteorites will be found.
Out of stock
Oued Awlitis 003 is a brecciated LL6 meteorite of 1141 grams. It was discovered in 2011 near the village of Lemluia in the Western Sahara. Other meteorites have been found in the same area, a lunar meteorite Oued Awlitis 001 and a carbonaceous type CV3 meteorite Oued Awlitis 002. This is a very rich area where other meteorites will be found.
Oued Awlitis 003 is a brecciated LL6 meteorite of 1141 grams. It was discovered in 2011 near the village of Lemluia in the Western Sahara. Other meteorites have been found in the same area, a lunar meteorite Oued Awlitis 001 and a carbonaceous type CV3 meteorite Oued Awlitis 002. This is a very rich area where other meteorites will be found.
Out of stock
Oued Awlitis 003 is a brecciated LL6 meteorite of 1141 grams. It was discovered in 2011 near the village of Lemluia in the Western Sahara. Other meteorites have been found in the same area, a lunar meteorite Oued Awlitis 001 and a carbonaceous type CV3 meteorite Oued Awlitis 002. This is a very rich area where other meteorites will be found.
Out of stock
Fezzou 001 is a rare meteorite of type chondrite rumuruti R4. This meteorite of only 154 grams was discovered in Morocco by Rjdali Hmou and Mohamed Taouch on August 1, 2018. This rumuruti has the particularity to be a little magnetic and not brecciated.
Out of stock
Fezzou 001 is a rare meteorite of type chondrite rumuruti R4. This meteorite of only 154 grams was discovered in Morocco by Rjdali Hmou and Mohamed Taouch on August 1, 2018. This rumuruti has the particularity to be a little magnetic and not brecciated.
Fezzou 001 is a rare meteorite of type chondrite rumuruti R4. This meteorite of only 154 grams was discovered in Morocco by Rjdali Hmou and Mohamed Taouch on August 1, 2018. This rumuruti has the particularity to be a little magnetic and not brecciated.
Fezzou 001 is a rare meteorite of type chondrite rumuruti R4. This meteorite of only 154 grams was discovered in Morocco by Rjdali Hmou and Mohamed Taouch on August 1, 2018. This rumuruti has the particularity to be a little magnetic and not brecciated.
Fezzou 001 is a rare meteorite of type chondrite rumuruti R4. This meteorite of only 154 grams was discovered in Morocco by Rjdali Hmou and Mohamed Taouch on August 1, 2018. This rumuruti has the particularity to be a little magnetic and not brecciated.
Fezzou 001 is a rare meteorite of type chondrite rumuruti R4. This meteorite of only 154 grams was discovered in Morocco by Rjdali Hmou and Mohamed Taouch on August 1, 2018. This rumuruti has the particularity to be a little magnetic and not brecciated.
Out of stock
NWA 15170 is a lodranite meteorite of only 89 grams.
The lodranites are a type of meteorites forming a group within the primitive achondrites.
The reference fall is the Lodran meteorite that fell in 1868 in Pakistan..
These rare meteorites are composed for a large part of orthopyroxene (45 to 55 %), of magnesian olivine (40 %), of Fe-Ni alloy, of troilite, of clinopyroxene, of daubreelite, schreibersite, chromite and, accessorily, feldspars plagioclase and orthoclase, alabandite, graphite and apatite.
NWA 15170 is a lodranite meteorite of only 89 grams.
The lodranites are a type of meteorites forming a group within the primitive achondrites.
The reference fall is the Lodran meteorite that fell in 1868 in Pakistan..
These rare meteorites are composed for a large part of orthopyroxene (45 to 55 %), of magnesian olivine (40 %), of Fe-Ni alloy, of troilite, of clinopyroxene, of daubreelite, schreibersite, chromite and, accessorily, feldspars plagioclase and orthoclase, alabandite, graphite and apatite.
Out of stock
NWA 15170 is a lodranite meteorite of only 89 grams.
The lodranites are a type of meteorites forming a group within the primitive achondrites.
The reference fall is the Lodran meteorite that fell in 1868 in Pakistan..
These rare meteorites are composed for a large part of orthopyroxene (45 to 55 %), of magnesian olivine (40 %), of Fe-Ni alloy, of troilite, of clinopyroxene, of daubreelite, schreibersite, chromite and, accessorily, feldspars plagioclase and orthoclase, alabandite, graphite and apatite.
Out of stock
NWA 15170 is a lodranite meteorite of only 89 grams.
The lodranites are a type of meteorites forming a group within the primitive achondrites.
The reference fall is the Lodran meteorite that fell in 1868 in Pakistan..
These rare meteorites are composed for a large part of orthopyroxene (45 to 55 %), of magnesian olivine (40 %), of Fe-Ni alloy, of troilite, of clinopyroxene, of daubreelite, schreibersite, chromite and, accessorily, feldspars plagioclase and orthoclase, alabandite, graphite and apatite.
Out of stock
NWA 13881 is a CV3 type meteorite with very large chondrules.
CV3 chondrites are characterized by the presence of large chondrules, abundant pre-solar isotopes and white inclusions called CAI’s.
CAI’s are mineral inclusions rich in calcium and aluminum, formed 4,567 to 4,571 million years ago they are the oldest materials in the Solar System.
Out of stock
NWA 13881 is a CV3 type meteorite with very large chondrules.
CV3 chondrites are characterized by the presence of large chondrules, abundant pre-solar isotopes and white inclusions called CAI’s.
CAI’s are mineral inclusions rich in calcium and aluminum, formed 4,567 to 4,571 million years ago they are the oldest materials in the Solar System.
NWA 13881 is a CV3 type meteorite with very large chondrules.
CV3 chondrites are characterized by the presence of large chondrules, abundant pre-solar isotopes and white inclusions called CAI’s.
CAI’s are mineral inclusions rich in calcium and aluminum, formed 4,567 to 4,571 million years ago they are the oldest materials in the Solar System.
The Atacamaites were discovered in the Atacama desert in Chile.
They are black and glassy objects of about 1 cm, they were formed following an impact about 7.8 million years ago.
Their small size, heterogeneity, state of oxidation and level of contamination distinguish them from tektites, which is why a study conducted by J. Gattacceca, Bertrand Devouard, Jean-Alix J-A Barrat, Pierre Rochette, M.L. Balestrieri, G. Bigazzi, G. Ménard, F. Moustard, E. dos Santos, R. Scorzelli, proposes to name them “tektoids”.
The impactor was an iron meteorite, most probably of the IIAB group.
