TURPAN 003 #3 Iron - silicate inclusion 2.4 g 1 × 118,91 $
Zagora 003 Eucrite #4 - 23,9 g 1 × 307,96 $
NWA 15169 Lunaire #26 - 2,1 g 1 × 206,89 $
Clay layer K-T Bidart France #11 – 2 g 1 × 25,76 $
Oued El Kechbi #25 L4 - 0,3 g 1 × 10,70 $
VINALES L6 #5 - 8 g 1 × 114,14 $Subtotal: 784,37 $
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.
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.
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.
NWA 16738 is a CK3 carbonaceous meteorite.
To date, only 88 of these have been classified.
The reference fall is the Karoonda meteorite that fell in 1930 in Australia.
CK meteorites have inclusions called CAI’s, (calcium and aluminum rich mineral inclusions), formed 4,567 to 4,571 million years ago, they are the oldest materials in the Solar System.
Out of stock
NWA 16172 is a carbonaceous meteorite of a new carbonaceous class called CL.
CL-type meteorites are characterized by a large number of chondrules with little matrix and unusual metal grains for a carbonaceous meteorite.
This is a rare classification, with few items available for sale.
NWA 16172 is a carbonaceous meteorite of a new carbonaceous class called CL.
CL-type meteorites are characterized by a large number of chondrules with little matrix and unusual metal grains for a carbonaceous meteorite.
This is a rare classification, with few items available for sale.
NWA 16172 is a carbonaceous meteorite of a new carbonaceous class called CL.
CL-type meteorites are characterized by a large number of chondrules with little matrix and unusual metal grains for a carbonaceous meteorite.
This is a rare classification, with few items available for sale.
Out of stock
NWA 16172 is a carbonaceous meteorite of a new carbonaceous class called CL.
CL-type meteorites are characterized by a large number of chondrules with little matrix and unusual metal grains for a carbonaceous meteorite.
This is a rare classification, with few items available for sale.
Out of stock
NWA 16172 is a carbonaceous meteorite of a new carbonaceous class called CL.
CL-type meteorites are characterized by a large number of chondrules with little matrix and unusual metal grains for a carbonaceous meteorite.
This is a rare classification, with few items available for sale.
NWA 15523 is a CM2-type meteorite weighing just 780 grams, discovered in 2022.
This meteorite is of the same type as the famous Murchison meteorite.
CM2 meteorites are becoming increasingly difficult to find on the market.
NWA 15523 is a CM2-type meteorite weighing just 780 grams, discovered in 2022.
This meteorite is of the same type as the famous Murchison meteorite.
CM2 meteorites are becoming increasingly difficult to find on the market.
NWA 15523 is a CM2-type meteorite weighing just 780 grams, discovered in 2022.
This meteorite is of the same type as the famous Murchison meteorite.
CM2 meteorites are becoming increasingly difficult to find on the market.
NWA 15523 is a CM2-type meteorite weighing just 780 grams, discovered in 2022.
This meteorite is of the same type as the famous Murchison meteorite.
CM2 meteorites are becoming increasingly difficult to find on the market.
NWA 15523 is a CM2-type meteorite weighing just 780 grams, discovered in 2022.
This meteorite is of the same type as the famous Murchison meteorite.
CM2 meteorites are becoming increasingly difficult to find on the market.
NWA 15523 is a CM2-type meteorite weighing just 780 grams, discovered in 2022.
This meteorite is of the same type as the famous Murchison meteorite.
CM2 meteorites are becoming increasingly difficult to find on the market.
NWA 15523 is a CM2-type meteorite weighing just 780 grams, discovered in 2022.
This meteorite is of the same type as the famous Murchison meteorite.
CM2 meteorites are becoming increasingly difficult to find on the market.