Erg Chech 002 is an achondrite type meteorite found in Algeria in 2020.
The particularity of this meteorite is that it does not resemble any meteorite known to date and that we know nothing of the parent body from which it came.
This meteorite is dated 4.565 billion years (older than our Earth), it was formed at the beginning of the solar system.
It is the oldest magmatic rock in the solar system known to date !
This meteorite also has the particularity to have large green crystals of pyroxene.
Erg Chech 002 is an achondrite type meteorite found in Algeria in 2020.
The particularity of this meteorite is that it does not resemble any meteorite known to date and that we know nothing of the parent body from which it came.
This meteorite is dated 4.565 billion years (older than our Earth), it was formed at the beginning of the solar system.
It is the oldest magmatic rock in the solar system known to date !
This meteorite also has the particularity to have large green crystals of pyroxene.
Erg Chech 002 is an achondrite type meteorite found in Algeria in 2020.
The particularity of this meteorite is that it does not resemble any meteorite known to date and that we know nothing of the parent body from which it came.
This meteorite is dated 4.565 billion years (older than our Earth), it was formed at the beginning of the solar system.
It is the oldest magmatic rock in the solar system known to date !
This meteorite also has the particularity to have large green crystals of pyroxene.
Erg Chech 002 is an achondrite type meteorite found in Algeria in 2020.
The particularity of this meteorite is that it does not resemble any meteorite known to date and that we know nothing of the parent body from which it came.
This meteorite is dated 4.565 billion years (older than our Earth), it was formed at the beginning of the solar system.
It is the oldest magmatic rock in the solar system known to date !
This meteorite also has the particularity to have large green crystals of pyroxene.
Erg Chech 002 is an achondrite type meteorite found in Algeria in 2020.
The particularity of this meteorite is that it does not resemble any meteorite known to date and that we know nothing of the parent body from which it came.
This meteorite is dated 4.565 billion years (older than our Earth), it was formed at the beginning of the solar system.
It is the oldest magmatic rock in the solar system known to date !
This meteorite also has the particularity to have large green crystals of pyroxene.
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.
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.
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.
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