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Chwichiya 002 C3.00 Ung #54 - 2,1 g

Chwichiya 002 C3.00 Ung #54 – 2,1 g

658,72 $

Chwichiya 002 is an ordinary carbonaceous chondrite of the C3.00 ungrouped type; it is the most primitive type ever found to date, having undergone no hydration or heating prior to its ejection from the parent body.
This meteorite may be one of the most scientifically significant meteorites of all time; there is no doubt that our understanding of the solar system will advance thanks to it.
It was discovered in Western Sahara.
A must-have for any collection!
https://www.futura-sciences.com/sciences/actualites/astronomie-tresor-cosmique-france-cette-meteorite-contient-grains-plus-anciens-soleil-w2t8-130194/

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Trinitite #52 - 2,1 g

Trinitite #52 – 2,1 g

107,64 $

Trinitite is a type of glass formed during the first nuclear test, known as Trinity, which took place in Alamogordo, New Mexico, on July 16, 1945.

Trinitite is formed by the vitrification of desert sand mixed with various components of the structure on which the bomb rested, as well as the bomb itself. Recently, researchers discovered that a piece of red trinitite had taken the form of a quasicrystal.

First discovered in the laboratory in the 1980s, quasicrystals also occur in nature, particularly in meteorites.

It should be noted that trinitite is not harmful to health.

 

 

 

 

 

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Trinitite #51 - 1,8 g

Trinitite #51 – 1,8 g

92,42 $

Trinitite is a type of glass formed during the first nuclear test, known as Trinity, which took place in Alamogordo, New Mexico, on July 16, 1945.

Trinitite is formed by the vitrification of desert sand mixed with various components of the structure on which the bomb rested, as well as the bomb itself. Recently, researchers discovered that a piece of red trinitrite had taken on the form of a quasicrystal.

First discovered in the laboratory in the 1980s, quasicrystals also occur in nature, particularly in meteorites.

It should be noted that trinitite is not harmful to health.

 

 

 

 

 

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Trinitite #50 - 2,8 g

Trinitite #50 – 2,8 g

143,92 $

Trinitite is a type of glass formed during the first nuclear test, known as Trinity, which took place in Alamogordo, New Mexico, on July 16, 1945.

Trinitite is formed by the vitrification of desert sand mixed with various components of the structure on which the bomb rested, as well as the bomb itself. Recently, researchers discovered that a piece of red trinitrite had taken on the form of a quasicrystal.

First discovered in the laboratory in the 1980s, quasicrystals also occur in nature, particularly in meteorites.

It should be noted that trinitite is not harmful to health.

 

 

 

 

 

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Trinitite #49 - 1,7 g

Trinitite #49 – 1,7 g

87,76 $

Trinitite is a type of glass formed during the first nuclear test, known as Trinity, which took place in Alamogordo, New Mexico, on July 16, 1945.

Trinitite is formed by the vitrification of desert sand mixed with various components of the structure on which the bomb rested, as well as the bomb itself. Recently, researchers discovered that a piece of red trinitite had taken the form of a quasicrystal.

First discovered in the laboratory in the 1980s, quasicrystals also occur in nature, particularly in meteorites.

It should be noted that trinitite is not harmful to health.

 

 

 

 

 

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Trinitite #48 - 3 g

Trinitite #48 – 3 g

154,44 $

Trinitite is a type of glass formed during the first nuclear test, known as Trinity, which took place in Alamogordo, New Mexico, on July 16, 1945.

Trinitite is formed by the vitrification of desert sand mixed with various components of the structure on which the bomb rested, as well as the bomb itself. Recently, researchers discovered that a piece of red trinitrite had taken on the form of a quasicrystal.

First discovered in the laboratory in the 1980s, quasicrystals also occur in nature, particularly in meteorites.

It should be noted that trinitite is not harmful to health.

 

 

 

 

 

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Trinitite #47 - 1,3 g

Trinitite #47 – 1,3 g

66,70 $

Trinitite is a type of glass formed during the first nuclear test, known as Trinity, which took place in Alamogordo, New Mexico, on July 16, 1945.

Trinitite is formed by the vitrification of desert sand mixed with various components of the structure on which the bomb rested, as well as the bomb itself. Recently, researchers discovered that a piece of red trinitite had taken the form of a quasicrystal.

First discovered in the laboratory in the 1980s, quasicrystals also occur in nature, particularly in meteorites.

It should be noted that trinitite is not harmful to health.

 

 

 

 

 

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Trinitite #46 - 3,9 g

Trinitite #46 – 3,9 g

201,24 $

Trinitite is a type of glass formed during the first nuclear test, known as Trinity, which took place in Alamogordo, New Mexico, on July 16, 1945.

Trinitite is formed by the vitrification of desert sand mixed with various components of the structure on which the bomb rested, as well as the bomb itself. Recently, researchers discovered that a piece of red trinitrite had taken on the form of a quasicrystal.

First discovered in the laboratory in the 1980s, quasicrystals also occur in nature, particularly in meteorites.

It should be noted that trinitite is not harmful to health.

 

 

 

 

 

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Chwichiya 002 C3.00 Ung #53 - 2,8 gOut of stock

Chwichiya 002 C3.00 Ung #53 – 2,8 g

877,50 $

Chwichiya 002 is an ordinary carbonaceous chondrite of the C3.00 ungrouped type; it is the most primitive type ever found to date, having undergone no hydration or heating prior to its ejection from the parent body.
This meteorite may be one of the most scientifically significant meteorites of all time; there is no doubt that our understanding of the solar system will advance thanks to it.
It was discovered in Western Sahara.
A must-have for any collection!
https://www.futura-sciences.com/sciences/actualites/astronomie-tresor-cosmique-france-cette-meteorite-contient-grains-plus-anciens-soleil-w2t8-130194/

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Chwichiya 002 C3.00 Ung #52 - 4,5 g

Chwichiya 002 C3.00 Ung #52 – 4,5 g

1.316,26 $

Chwichiya 002 is an ordinary carbonaceous chondrite of the C3.00 ungrouped type; it is the most primitive type ever found to date, having undergone no hydration or heating prior to its ejection from the parent body.
This meteorite may be one of the most scientifically significant meteorites of all time; there is no doubt that our understanding of the solar system will advance thanks to it.
It was discovered in Western Sahara.
A must-have for any collection!
https://www.futura-sciences.com/sciences/actualites/astronomie-tresor-cosmique-france-cette-meteorite-contient-grains-plus-anciens-soleil-w2t8-130194/

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Chwichiya 002 C3.00 Ung #51 - 3,7 g

Chwichiya 002 C3.00 Ung #51 – 3,7 g

1.082,24 $

Chwichiya 002 is an ordinary carbonaceous chondrite of the C3.00 ungrouped type; it is the most primitive type ever found to date, having undergone no hydration or heating prior to its ejection from the parent body.
This meteorite may be one of the most scientifically significant meteorites of all time; there is no doubt that our understanding of the solar system will advance thanks to it.
It was discovered in Western Sahara.
A must-have for any collection!
https://www.futura-sciences.com/sciences/actualites/astronomie-tresor-cosmique-france-cette-meteorite-contient-grains-plus-anciens-soleil-w2t8-130194/

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Chwichiya 002 C3.00 Ung #50 - 3,6 g

Chwichiya 002 C3.00 Ung #50 – 3,6 g

1.053,00 $

Chwichiya 002 is an ordinary carbonaceous chondrite of the C3.00 ungrouped type; it is the most primitive type ever found to date, having undergone no hydration or heating prior to its ejection from the parent body.
This meteorite may be one of the most scientifically significant meteorites of all time; there is no doubt that our understanding of the solar system will advance thanks to it.
It was discovered in Western Sahara.
A must-have for any collection!
https://www.futura-sciences.com/sciences/actualites/astronomie-tresor-cosmique-france-cette-meteorite-contient-grains-plus-anciens-soleil-w2t8-130194/

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Chwichiya 002 C3.00 Ung #49 - 7,9 gOut of stock

Chwichiya 002 C3.00 Ung #49 – 7,9 g

1.848,60 $

Chwichiya 002 is an ordinary carbonaceous chondrite of the C3.00 ungrouped type; it is the most primitive type ever found to date, having undergone no hydration or heating prior to its ejection from the parent body.
This meteorite may be one of the most scientifically significant meteorites of all time; there is no doubt that our understanding of the solar system will advance thanks to it.
It was discovered in Western Sahara.
A must-have for any collection!
https://www.futura-sciences.com/sciences/actualites/astronomie-tresor-cosmique-france-cette-meteorite-contient-grains-plus-anciens-soleil-w2t8-130194/

Details
Amgala 001 Mars Shergottite (olivine-phyric) #53 - 0,4 g

Amgala 001 Mars Shergottite (olivine-phyric) #53 – 0,4 g

51,48 $

Amgala is a rare meteorite from Mars, classified as Shergottite (olivine-phyric).

It was discovered in the Western Sahara in 2022

A meteorite offering exceptional value for money !

Amgala 001 26.014°N, 11.020°W

Saguia el Hamra, Western Sahara

Purchased: 2022 Dec

Classification: Martian meteorite (Shergottite)

History: Multiple stones were found together in December 2022 near Meharrize. Said Muftah Bachir and Ziyao Wang bought 12 kg together from the finders, including the largest 5200 g individual; Mark Lyon acquired 19165 g from two different dealers; Aziz Habibi obtained 3500 g from another dealer.

Physical characteristics: Weathered exterior surfaces of the stones are brown with a distinctive knobby appearance. Fresh interiors are greenish-gray with darker olivine phenocrysts visible.

Petrography: (A. Irving, UWS, and P. Carpenter, WUSL) Zoned olivine phenocrysts (up to 2 mm in length) are set in a groundmass with variable grainsize composed predominantly of prismatic, zoned clinopyroxene and lath-like maskelynite, together with accessory alkali feldspar, pyrrhotite, ulvöspinel, chromite (with variable Ti content), ilmenite, baddeleyite and chlorapatite. Thin opaque shock veins crosscut the specimen as well as secondary calcite veinlets. Olivine phenocrysts contain small patches of alteration products (red-brown in thin section).

Geochemistry: Olivine (Fa31.7-56.6, FeO/MnO = 52-55, N = 5), pigeonite (Fs27.7-48.4Wo10.4-9.8, FeO/MnO = 29-35, N = 3), subcalcic augite (Fs20.7-30.4Wo32.5-34.6, FeO/MnO = 28-32, N = 2), maskelynite (An47.4-50.5Or2.2-1.7, N = 2), alkali feldspar (Ab49.4Or34.0An16.7).

Classification: Shergottite (olivine-phyric).

Specimens: 68.3 g including one polished thin section at UWB; remainder with Mr. S. Bachir/WangZ (12 kg), Mr. M. Lyon (19165 g) and Mr. A. Habibi (3500 g).

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Amgala 001 Mars Shergottite (olivine-phyric) #52 - 0,4 gOut of stock

Amgala 001 Mars Shergottite (olivine-phyric) #52 – 0,4 g

51,48 $

Amgala is a rare meteorite from Mars, classified as Shergottite (olivine-phyric).

It was discovered in the Western Sahara in 2022

A meteorite offering exceptional value for money !

Amgala 001 26.014°N, 11.020°W

Saguia el Hamra, Western Sahara

Purchased: 2022 Dec

Classification: Martian meteorite (Shergottite)

History: Multiple stones were found together in December 2022 near Meharrize. Said Muftah Bachir and Ziyao Wang bought 12 kg together from the finders, including the largest 5200 g individual; Mark Lyon acquired 19165 g from two different dealers; Aziz Habibi obtained 3500 g from another dealer.

Physical characteristics: Weathered exterior surfaces of the stones are brown with a distinctive knobby appearance. Fresh interiors are greenish-gray with darker olivine phenocrysts visible.

Petrography: (A. Irving, UWS, and P. Carpenter, WUSL) Zoned olivine phenocrysts (up to 2 mm in length) are set in a groundmass with variable grainsize composed predominantly of prismatic, zoned clinopyroxene and lath-like maskelynite, together with accessory alkali feldspar, pyrrhotite, ulvöspinel, chromite (with variable Ti content), ilmenite, baddeleyite and chlorapatite. Thin opaque shock veins crosscut the specimen as well as secondary calcite veinlets. Olivine phenocrysts contain small patches of alteration products (red-brown in thin section).

Geochemistry: Olivine (Fa31.7-56.6, FeO/MnO = 52-55, N = 5), pigeonite (Fs27.7-48.4Wo10.4-9.8, FeO/MnO = 29-35, N = 3), subcalcic augite (Fs20.7-30.4Wo32.5-34.6, FeO/MnO = 28-32, N = 2), maskelynite (An47.4-50.5Or2.2-1.7, N = 2), alkali feldspar (Ab49.4Or34.0An16.7).

Classification: Shergottite (olivine-phyric).

Specimens: 68.3 g including one polished thin section at UWB; remainder with Mr. S. Bachir/WangZ (12 kg), Mr. M. Lyon (19165 g) and Mr. A. Habibi (3500 g).

Details
Amgala 001 Mars Shergottite (olivine-phyric) #51 - 1,4 g

Amgala 001 Mars Shergottite (olivine-phyric) #51 – 1,4 g

180,18 $

Amgala is a rare meteorite from Mars, classified as Shergottite (olivine-phyric).

It was discovered in the Western Sahara in 2022

A meteorite offering exceptional value for money !

Amgala 001 26.014°N, 11.020°W

Saguia el Hamra, Western Sahara

Purchased: 2022 Dec

Classification: Martian meteorite (Shergottite)

History: Multiple stones were found together in December 2022 near Meharrize. Said Muftah Bachir and Ziyao Wang bought 12 kg together from the finders, including the largest 5200 g individual; Mark Lyon acquired 19165 g from two different dealers; Aziz Habibi obtained 3500 g from another dealer.

Physical characteristics: Weathered exterior surfaces of the stones are brown with a distinctive knobby appearance. Fresh interiors are greenish-gray with darker olivine phenocrysts visible.

Petrography: (A. Irving, UWS, and P. Carpenter, WUSL) Zoned olivine phenocrysts (up to 2 mm in length) are set in a groundmass with variable grainsize composed predominantly of prismatic, zoned clinopyroxene and lath-like maskelynite, together with accessory alkali feldspar, pyrrhotite, ulvöspinel, chromite (with variable Ti content), ilmenite, baddeleyite and chlorapatite. Thin opaque shock veins crosscut the specimen as well as secondary calcite veinlets. Olivine phenocrysts contain small patches of alteration products (red-brown in thin section).

Geochemistry: Olivine (Fa31.7-56.6, FeO/MnO = 52-55, N = 5), pigeonite (Fs27.7-48.4Wo10.4-9.8, FeO/MnO = 29-35, N = 3), subcalcic augite (Fs20.7-30.4Wo32.5-34.6, FeO/MnO = 28-32, N = 2), maskelynite (An47.4-50.5Or2.2-1.7, N = 2), alkali feldspar (Ab49.4Or34.0An16.7).

Classification: Shergottite (olivine-phyric).

Specimens: 68.3 g including one polished thin section at UWB; remainder with Mr. S. Bachir/WangZ (12 kg), Mr. M. Lyon (19165 g) and Mr. A. Habibi (3500 g).

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Amgala 001 Mars Shergottite (olivine-phyric) #50 - 1 g

Amgala 001 Mars Shergottite (olivine-phyric) #50 – 1 g

128,70 $

Amgala is a rare meteorite from Mars, classified as Shergottite (olivine-phyric).

It was discovered in the Western Sahara in 2022

A meteorite offering exceptional value for money !

Amgala 001 26.014°N, 11.020°W

Saguia el Hamra, Western Sahara

Purchased: 2022 Dec

Classification: Martian meteorite (Shergottite)

History: Multiple stones were found together in December 2022 near Meharrize. Said Muftah Bachir and Ziyao Wang bought 12 kg together from the finders, including the largest 5200 g individual; Mark Lyon acquired 19165 g from two different dealers; Aziz Habibi obtained 3500 g from another dealer.

Physical characteristics: Weathered exterior surfaces of the stones are brown with a distinctive knobby appearance. Fresh interiors are greenish-gray with darker olivine phenocrysts visible.

Petrography: (A. Irving, UWS, and P. Carpenter, WUSL) Zoned olivine phenocrysts (up to 2 mm in length) are set in a groundmass with variable grainsize composed predominantly of prismatic, zoned clinopyroxene and lath-like maskelynite, together with accessory alkali feldspar, pyrrhotite, ulvöspinel, chromite (with variable Ti content), ilmenite, baddeleyite and chlorapatite. Thin opaque shock veins crosscut the specimen as well as secondary calcite veinlets. Olivine phenocrysts contain small patches of alteration products (red-brown in thin section).

Geochemistry: Olivine (Fa31.7-56.6, FeO/MnO = 52-55, N = 5), pigeonite (Fs27.7-48.4Wo10.4-9.8, FeO/MnO = 29-35, N = 3), subcalcic augite (Fs20.7-30.4Wo32.5-34.6, FeO/MnO = 28-32, N = 2), maskelynite (An47.4-50.5Or2.2-1.7, N = 2), alkali feldspar (Ab49.4Or34.0An16.7).

Classification: Shergottite (olivine-phyric).

Specimens: 68.3 g including one polished thin section at UWB; remainder with Mr. S. Bachir/WangZ (12 kg), Mr. M. Lyon (19165 g) and Mr. A. Habibi (3500 g).

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Amgala 001 Mars Shergottite (olivine-phyric) #49 - 2 g

Amgala 001 Mars Shergottite (olivine-phyric) #49 – 2 g

257,40 $

Amgala is a rare meteorite from Mars, classified as Shergottite (olivine-phyric).

It was discovered in the Western Sahara in 2022

A meteorite offering exceptional value for money !

Amgala 001 26.014°N, 11.020°W

Saguia el Hamra, Western Sahara

Purchased: 2022 Dec

Classification: Martian meteorite (Shergottite)

History: Multiple stones were found together in December 2022 near Meharrize. Said Muftah Bachir and Ziyao Wang bought 12 kg together from the finders, including the largest 5200 g individual; Mark Lyon acquired 19165 g from two different dealers; Aziz Habibi obtained 3500 g from another dealer.

Physical characteristics: Weathered exterior surfaces of the stones are brown with a distinctive knobby appearance. Fresh interiors are greenish-gray with darker olivine phenocrysts visible.

Petrography: (A. Irving, UWS, and P. Carpenter, WUSL) Zoned olivine phenocrysts (up to 2 mm in length) are set in a groundmass with variable grainsize composed predominantly of prismatic, zoned clinopyroxene and lath-like maskelynite, together with accessory alkali feldspar, pyrrhotite, ulvöspinel, chromite (with variable Ti content), ilmenite, baddeleyite and chlorapatite. Thin opaque shock veins crosscut the specimen as well as secondary calcite veinlets. Olivine phenocrysts contain small patches of alteration products (red-brown in thin section).

Geochemistry: Olivine (Fa31.7-56.6, FeO/MnO = 52-55, N = 5), pigeonite (Fs27.7-48.4Wo10.4-9.8, FeO/MnO = 29-35, N = 3), subcalcic augite (Fs20.7-30.4Wo32.5-34.6, FeO/MnO = 28-32, N = 2), maskelynite (An47.4-50.5Or2.2-1.7, N = 2), alkali feldspar (Ab49.4Or34.0An16.7).

Classification: Shergottite (olivine-phyric).

Specimens: 68.3 g including one polished thin section at UWB; remainder with Mr. S. Bachir/WangZ (12 kg), Mr. M. Lyon (19165 g) and Mr. A. Habibi (3500 g).

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