Al Haggounia 001 is a meteorite of type chondrite enstatite, more precisely EL chondrite impact melt rock.
To date only 23 meteorites of this type have been classified.
This meteorite was discovered in Morocco in the Western Sahara.
Al Haggounia 001 is a meteorite of type chondrite enstatite, more precisely EL chondrite impact melt rock.
To date only 23 meteorites of this type have been classified.
This meteorite was discovered in Morocco in the Western Sahara.
Sueilila 003 is a meteorite of type CV3, oxidized subgroup, it was discovered by Mbark Ben Amar and Amar Azerwal in 2016 in the Western Sahara.
This meteorite has the particularity to have large chondrules of brown color and smaller chondrules of gray color.
No explanation has been found so far by science.
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.
Sueilila 003 is a meteorite of type CV3, oxidized subgroup, it was discovered by Mbark Ben Amar and Amar Azerwal in 2016 in the Western Sahara.
This meteorite has the particularity to have large chondrules of brown color and smaller chondrules of gray color.
No explanation has been found so far by science.
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.
Sueilila 003 is a meteorite of type CV3, oxidized subgroup, it was discovered by Mbark Ben Amar and Amar Azerwal in 2016 in the Western Sahara.
This meteorite has the particularity to have large chondrules of brown color and smaller chondrules of gray color.
No explanation has been found so far by science.
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.
Sueilila 003 is a meteorite of type CV3, oxidized subgroup, it was discovered by Mbark Ben Amar and Amar Azerwal in 2016 in the Western Sahara.
This meteorite has the particularity to have large chondrules of brown color and smaller chondrules of gray color.
No explanation has been found so far by science.
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.
Sueilila 003 is a meteorite of type CV3, oxidized subgroup, it was discovered by Mbark Ben Amar and Amar Azerwal in 2016 in the Western Sahara.
This meteorite has the particularity to have large chondrules of brown color and smaller chondrules of gray color.
No explanation has been found so far by science.
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.
Sueilila 003 is a meteorite of type CV3, oxidized subgroup, it was discovered by Mbark Ben Amar and Amar Azerwal in 2016 in the Western Sahara.
This meteorite has the particularity to have large chondrules of brown color and smaller chondrules of gray color.
No explanation has been found so far by science.
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.
Sueilila 003 is a meteorite of type CV3, oxidized subgroup, it was discovered by Mbark Ben Amar and Amar Azerwal in 2016 in the Western Sahara.
This meteorite has the particularity to have large chondrules of brown color and smaller chondrules of gray color.
No explanation has been found so far by science.
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.
Sueilila 003 is a meteorite of type CV3, oxidized subgroup, it was discovered by Mbark Ben Amar and Amar Azerwal in 2016 in the Western Sahara.
This meteorite has the particularity to have large chondrules of brown color and smaller chondrules of gray color.
No explanation has been found so far by science.
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 15971 is a pallasite meteorite.
Pallasites are meteorites composed of olivine crystals embedded in an iron-nickel matrix.
Pallasites are among the most aesthetic meteorites.
NWA 15971 is a pallasite meteorite.
Pallasites are meteorites composed of olivine crystals embedded in an iron-nickel matrix.
Pallasites are among the most aesthetic meteorites.
Out of stock
NWA 15971 is a pallasite meteorite.
Pallasites are meteorites composed of olivine crystals embedded in an iron-nickel matrix.
Pallasites are among the most aesthetic meteorites.
NWA 15971 is a pallasite meteorite.
Pallasites are meteorites composed of olivine crystals embedded in an iron-nickel matrix.
Pallasites are among the most aesthetic meteorites.
NWA 15971 is a pallasite meteorite.
Pallasites are meteorites composed of olivine crystals embedded in an iron-nickel matrix.
Pallasites are among the most aesthetic meteorites.
NWA 15971 is a pallasite meteorite.
Pallasites are meteorites composed of olivine crystals embedded in an iron-nickel matrix.
Pallasites are among the most aesthetic meteorites.
NWA 15971 is a pallasite meteorite.
Pallasites are meteorites composed of olivine crystals embedded in an iron-nickel matrix.
Pallasites are among the most aesthetic meteorites.
Out of stock
NWA 15971 is a pallasite meteorite.
Pallasites are meteorites composed of olivine crystals embedded in an iron-nickel matrix.
Pallasites are among the most aesthetic meteorites.