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Tarkint 001 Mars Shergottite #32 - 0,7 g

Tarkint 001 Mars Shergottite #32 – 0,7 g

122,86 $

Tarkint 001 is a rare meteorite from Mars, classified as Shergottite (olivine-phyric).

It was discovered in Gao, Mali, in 2025.

Its surface reveals numerous brown-green olivine phenocrystals measuring a few millimeters, embedded in a fine-grained, light beige matrix.

The unique feature of this meteorite is that it is unlike any other Martian meteorite.

The total known weight of this meteorite is only 2 kg, so there won’t be enough for everyone !

Tarkint 001 17.4959263, 0.6428554

Gao, Mali

Find: 2025

Classification: Martian meteorite (Shergottite)

History: In 2025, fragments of a meteorite were discovered in a desert area 60 km east of the village of Tarkint and approximately 150 km northeast of the city of Gao, Mali. The discovery occurred by chance during a local field survey, where the distinctive surface features of the stones drew the attention of the field researchers. Purchased by Ali Muftah in 2025.

Physical characteristics: The total collected mass was approximately 2 kg. The deposit samples display an exterior partially covered with dark, slightly abraded fusion crust. Sawcut surface reveals many distinctive mm-sized brown-green olivine phenocrysts set in light tan-colored, fine-grained groundmass.

Petrography: (C. Agee, UNM) Electron microprobe analysis of a polished mount shows this meteorite to be an olivine-phyric shergottite. Olivine phenocrysts display core-rim igneous zoning. Plagioclase has been converted to maskelynite. Fine-grained pigeonite and maskelynite make up the groundmass. Minor amounts of chromite, Ti-magnetite, and troilite are ubiquitous.

Geochemistry: (T. Shisseh, UNM) Olivine Fa32.6±12.1, Fe/Mn=53±4, n=13; pigeonite Fs23.3±3.2Wo4.9±2.2, Fe/Mn=30±1, n=17; maskelynite An54.9±3.5Ab44.7±3.5, n=4.

Classification: Martian, olivine-phyric shergottite. Visually, the macroscopic texture of this meteorite is reminiscent of NWA 10416, however they are not paired. This meteorite lacks augite and altered olivine, it also has maskelynite-only, with no remnant plagioclase present. This meteorite has olivine that is significantly more forsteritic than NWA 10416.

Specimens: 48 g on deposit at UNM, Ali Muftah holds the main mass, Eric Twelker holds a 410.7 g piece.

Tarkint 001 Mars Shergottite #31 - 0,7 g

Tarkint 001 Mars Shergottite #31 – 0,7 g

122,86 $

Tarkint 001 is a rare meteorite from Mars, classified as Shergottite (olivine-phyric).

It was discovered in Gao, Mali, in 2025.

Its surface reveals numerous brown-green olivine phenocrystals measuring a few millimeters, embedded in a fine-grained, light beige matrix.

The unique feature of this meteorite is that it is unlike any other Martian meteorite.

The total known weight of this meteorite is only 2 kg, so there won’t be enough for everyone !

Tarkint 001 17.4959263, 0.6428554

Gao, Mali

Find: 2025

Classification: Martian meteorite (Shergottite)

History: In 2025, fragments of a meteorite were discovered in a desert area 60 km east of the village of Tarkint and approximately 150 km northeast of the city of Gao, Mali. The discovery occurred by chance during a local field survey, where the distinctive surface features of the stones drew the attention of the field researchers. Purchased by Ali Muftah in 2025.

Physical characteristics: The total collected mass was approximately 2 kg. The deposit samples display an exterior partially covered with dark, slightly abraded fusion crust. Sawcut surface reveals many distinctive mm-sized brown-green olivine phenocrysts set in light tan-colored, fine-grained groundmass.

Petrography: (C. Agee, UNM) Electron microprobe analysis of a polished mount shows this meteorite to be an olivine-phyric shergottite. Olivine phenocrysts display core-rim igneous zoning. Plagioclase has been converted to maskelynite. Fine-grained pigeonite and maskelynite make up the groundmass. Minor amounts of chromite, Ti-magnetite, and troilite are ubiquitous.

Geochemistry: (T. Shisseh, UNM) Olivine Fa32.6±12.1, Fe/Mn=53±4, n=13; pigeonite Fs23.3±3.2Wo4.9±2.2, Fe/Mn=30±1, n=17; maskelynite An54.9±3.5Ab44.7±3.5, n=4.

Classification: Martian, olivine-phyric shergottite. Visually, the macroscopic texture of this meteorite is reminiscent of NWA 10416, however they are not paired. This meteorite lacks augite and altered olivine, it also has maskelynite-only, with no remnant plagioclase present. This meteorite has olivine that is significantly more forsteritic than NWA 10416.

Specimens: 48 g on deposit at UNM, Ali Muftah holds the main mass, Eric Twelker holds a 410.7 g piece.

Tarkint 001 Mars Shergottite #30 - 1,8 g

Tarkint 001 Mars Shergottite #30 – 1,8 g

257,40 $

Tarkint 001 is a rare meteorite from Mars, classified as Shergottite (olivine-phyric).

It was discovered in Gao, Mali, in 2025.

Its surface reveals numerous brown-green olivine phenocrystals measuring a few millimeters, embedded in a fine-grained, light beige matrix.

The unique feature of this meteorite is that it is unlike any other Martian meteorite.

The total known weight of this meteorite is only 2 kg, so there won’t be enough for everyone !

Tarkint 001 17.4959263, 0.6428554

Gao, Mali

Find: 2025

Classification: Martian meteorite (Shergottite)

History: In 2025, fragments of a meteorite were discovered in a desert area 60 km east of the village of Tarkint and approximately 150 km northeast of the city of Gao, Mali. The discovery occurred by chance during a local field survey, where the distinctive surface features of the stones drew the attention of the field researchers. Purchased by Ali Muftah in 2025.

Physical characteristics: The total collected mass was approximately 2 kg. The deposit samples display an exterior partially covered with dark, slightly abraded fusion crust. Sawcut surface reveals many distinctive mm-sized brown-green olivine phenocrysts set in light tan-colored, fine-grained groundmass.

Petrography: (C. Agee, UNM) Electron microprobe analysis of a polished mount shows this meteorite to be an olivine-phyric shergottite. Olivine phenocrysts display core-rim igneous zoning. Plagioclase has been converted to maskelynite. Fine-grained pigeonite and maskelynite make up the groundmass. Minor amounts of chromite, Ti-magnetite, and troilite are ubiquitous.

Geochemistry: (T. Shisseh, UNM) Olivine Fa32.6±12.1, Fe/Mn=53±4, n=13; pigeonite Fs23.3±3.2Wo4.9±2.2, Fe/Mn=30±1, n=17; maskelynite An54.9±3.5Ab44.7±3.5, n=4.

Classification: Martian, olivine-phyric shergottite. Visually, the macroscopic texture of this meteorite is reminiscent of NWA 10416, however they are not paired. This meteorite lacks augite and altered olivine, it also has maskelynite-only, with no remnant plagioclase present. This meteorite has olivine that is significantly more forsteritic than NWA 10416.

Specimens: 48 g on deposit at UNM, Ali Muftah holds the main mass, Eric Twelker holds a 410.7 g piece.

Tarkint 001 Mars Shergottite #29 - 2 g

Tarkint 001 Mars Shergottite #29 – 2 g

292,50 $

Tarkint 001 is a rare meteorite from Mars, classified as Shergottite (olivine-phyric).

It was discovered in Gao, Mali, in 2025.

Its surface reveals numerous brown-green olivine phenocrystals measuring a few millimeters, embedded in a fine-grained, light beige matrix.

The unique feature of this meteorite is that it is unlike any other Martian meteorite.

The total known weight of this meteorite is only 2 kg, so there won’t be enough for everyone !

Tarkint 001 17.4959263, 0.6428554

Gao, Mali

Find: 2025

Classification: Martian meteorite (Shergottite)

History: In 2025, fragments of a meteorite were discovered in a desert area 60 km east of the village of Tarkint and approximately 150 km northeast of the city of Gao, Mali. The discovery occurred by chance during a local field survey, where the distinctive surface features of the stones drew the attention of the field researchers. Purchased by Ali Muftah in 2025.

Physical characteristics: The total collected mass was approximately 2 kg. The deposit samples display an exterior partially covered with dark, slightly abraded fusion crust. Sawcut surface reveals many distinctive mm-sized brown-green olivine phenocrysts set in light tan-colored, fine-grained groundmass.

Petrography: (C. Agee, UNM) Electron microprobe analysis of a polished mount shows this meteorite to be an olivine-phyric shergottite. Olivine phenocrysts display core-rim igneous zoning. Plagioclase has been converted to maskelynite. Fine-grained pigeonite and maskelynite make up the groundmass. Minor amounts of chromite, Ti-magnetite, and troilite are ubiquitous.

Geochemistry: (T. Shisseh, UNM) Olivine Fa32.6±12.1, Fe/Mn=53±4, n=13; pigeonite Fs23.3±3.2Wo4.9±2.2, Fe/Mn=30±1, n=17; maskelynite An54.9±3.5Ab44.7±3.5, n=4.

Classification: Martian, olivine-phyric shergottite. Visually, the macroscopic texture of this meteorite is reminiscent of NWA 10416, however they are not paired. This meteorite lacks augite and altered olivine, it also has maskelynite-only, with no remnant plagioclase present. This meteorite has olivine that is significantly more forsteritic than NWA 10416.

Specimens: 48 g on deposit at UNM, Ali Muftah holds the main mass, Eric Twelker holds a 410.7 g piece.

Tarkint 001 Mars Shergottite #28 - 0,9 g

Tarkint 001 Mars Shergottite #28 – 0,9 g

147,42 $

Tarkint 001 is a rare meteorite from Mars, classified as Shergottite (olivine-phyric).

It was discovered in Gao, Mali, in 2025.

Its surface reveals numerous brown-green olivine phenocrystals measuring a few millimeters, embedded in a fine-grained, light beige matrix.

The unique feature of this meteorite is that it is unlike any other Martian meteorite.

The total known weight of this meteorite is only 2 kg, so there won’t be enough for everyone !

Tarkint 001 17.4959263, 0.6428554

Gao, Mali

Find: 2025

Classification: Martian meteorite (Shergottite)

History: In 2025, fragments of a meteorite were discovered in a desert area 60 km east of the village of Tarkint and approximately 150 km northeast of the city of Gao, Mali. The discovery occurred by chance during a local field survey, where the distinctive surface features of the stones drew the attention of the field researchers. Purchased by Ali Muftah in 2025.

Physical characteristics: The total collected mass was approximately 2 kg. The deposit samples display an exterior partially covered with dark, slightly abraded fusion crust. Sawcut surface reveals many distinctive mm-sized brown-green olivine phenocrysts set in light tan-colored, fine-grained groundmass.

Petrography: (C. Agee, UNM) Electron microprobe analysis of a polished mount shows this meteorite to be an olivine-phyric shergottite. Olivine phenocrysts display core-rim igneous zoning. Plagioclase has been converted to maskelynite. Fine-grained pigeonite and maskelynite make up the groundmass. Minor amounts of chromite, Ti-magnetite, and troilite are ubiquitous.

Geochemistry: (T. Shisseh, UNM) Olivine Fa32.6±12.1, Fe/Mn=53±4, n=13; pigeonite Fs23.3±3.2Wo4.9±2.2, Fe/Mn=30±1, n=17; maskelynite An54.9±3.5Ab44.7±3.5, n=4.

Classification: Martian, olivine-phyric shergottite. Visually, the macroscopic texture of this meteorite is reminiscent of NWA 10416, however they are not paired. This meteorite lacks augite and altered olivine, it also has maskelynite-only, with no remnant plagioclase present. This meteorite has olivine that is significantly more forsteritic than NWA 10416.

Specimens: 48 g on deposit at UNM, Ali Muftah holds the main mass, Eric Twelker holds a 410.7 g piece.

Tarkint 001 Mars Shergottite #27 - 2,3 g

Tarkint 001 Mars Shergottite #27 – 2,3 g

322,92 $

Tarkint 001 is a rare meteorite from Mars, classified as Shergottite (olivine-phyric).

It was discovered in Gao, Mali, in 2025.

Its surface reveals numerous brown-green olivine phenocrystals measuring a few millimeters, embedded in a fine-grained, light beige matrix.

The unique feature of this meteorite is that it is unlike any other Martian meteorite.

The total known weight of this meteorite is only 2 kg, so there won’t be enough for everyone !

Tarkint 001 17.4959263, 0.6428554

Gao, Mali

Find: 2025

Classification: Martian meteorite (Shergottite)

History: In 2025, fragments of a meteorite were discovered in a desert area 60 km east of the village of Tarkint and approximately 150 km northeast of the city of Gao, Mali. The discovery occurred by chance during a local field survey, where the distinctive surface features of the stones drew the attention of the field researchers. Purchased by Ali Muftah in 2025.

Physical characteristics: The total collected mass was approximately 2 kg. The deposit samples display an exterior partially covered with dark, slightly abraded fusion crust. Sawcut surface reveals many distinctive mm-sized brown-green olivine phenocrysts set in light tan-colored, fine-grained groundmass.

Petrography: (C. Agee, UNM) Electron microprobe analysis of a polished mount shows this meteorite to be an olivine-phyric shergottite. Olivine phenocrysts display core-rim igneous zoning. Plagioclase has been converted to maskelynite. Fine-grained pigeonite and maskelynite make up the groundmass. Minor amounts of chromite, Ti-magnetite, and troilite are ubiquitous.

Geochemistry: (T. Shisseh, UNM) Olivine Fa32.6±12.1, Fe/Mn=53±4, n=13; pigeonite Fs23.3±3.2Wo4.9±2.2, Fe/Mn=30±1, n=17; maskelynite An54.9±3.5Ab44.7±3.5, n=4.

Classification: Martian, olivine-phyric shergottite. Visually, the macroscopic texture of this meteorite is reminiscent of NWA 10416, however they are not paired. This meteorite lacks augite and altered olivine, it also has maskelynite-only, with no remnant plagioclase present. This meteorite has olivine that is significantly more forsteritic than NWA 10416.

Specimens: 48 g on deposit at UNM, Ali Muftah holds the main mass, Eric Twelker holds a 410.7 g piece.

Tarkint 001 Mars Shergottite #26 - 2,8 g

Tarkint 001 Mars Shergottite #26 – 2,8 g

393,12 $

Tarkint 001 is a rare meteorite from Mars, classified as Shergottite (olivine-phyric).

It was discovered in Gao, Mali, in 2025.

Its surface reveals numerous brown-green olivine phenocrystals measuring a few millimeters, embedded in a fine-grained, light beige matrix.

The unique feature of this meteorite is that it is unlike any other Martian meteorite.

The total known weight of this meteorite is only 2 kg, so there won’t be enough for everyone !

Tarkint 001 17.4959263, 0.6428554

Gao, Mali

Find: 2025

Classification: Martian meteorite (Shergottite)

History: In 2025, fragments of a meteorite were discovered in a desert area 60 km east of the village of Tarkint and approximately 150 km northeast of the city of Gao, Mali. The discovery occurred by chance during a local field survey, where the distinctive surface features of the stones drew the attention of the field researchers. Purchased by Ali Muftah in 2025.

Physical characteristics: The total collected mass was approximately 2 kg. The deposit samples display an exterior partially covered with dark, slightly abraded fusion crust. Sawcut surface reveals many distinctive mm-sized brown-green olivine phenocrysts set in light tan-colored, fine-grained groundmass.

Petrography: (C. Agee, UNM) Electron microprobe analysis of a polished mount shows this meteorite to be an olivine-phyric shergottite. Olivine phenocrysts display core-rim igneous zoning. Plagioclase has been converted to maskelynite. Fine-grained pigeonite and maskelynite make up the groundmass. Minor amounts of chromite, Ti-magnetite, and troilite are ubiquitous.

Geochemistry: (T. Shisseh, UNM) Olivine Fa32.6±12.1, Fe/Mn=53±4, n=13; pigeonite Fs23.3±3.2Wo4.9±2.2, Fe/Mn=30±1, n=17; maskelynite An54.9±3.5Ab44.7±3.5, n=4.

Classification: Martian, olivine-phyric shergottite. Visually, the macroscopic texture of this meteorite is reminiscent of NWA 10416, however they are not paired. This meteorite lacks augite and altered olivine, it also has maskelynite-only, with no remnant plagioclase present. This meteorite has olivine that is significantly more forsteritic than NWA 10416.

Specimens: 48 g on deposit at UNM, Ali Muftah holds the main mass, Eric Twelker holds a 410.7 g piece.

Tarkint 001 Mars Shergottite #25 - 3,2 g

Tarkint 001 Mars Shergottite #25 – 3,2 g

449,28 $

Tarkint 001 is a rare meteorite from Mars, classified as Shergottite (olivine-phyric).

It was discovered in Gao, Mali, in 2025.

Its surface reveals numerous brown-green olivine phenocrystals measuring a few millimeters, embedded in a fine-grained, light beige matrix.

The unique feature of this meteorite is that it is unlike any other Martian meteorite.

The total known weight of this meteorite is only 2 kg, so there won’t be enough for everyone !

Tarkint 001 17.4959263, 0.6428554

Gao, Mali

Find: 2025

Classification: Martian meteorite (Shergottite)

History: In 2025, fragments of a meteorite were discovered in a desert area 60 km east of the village of Tarkint and approximately 150 km northeast of the city of Gao, Mali. The discovery occurred by chance during a local field survey, where the distinctive surface features of the stones drew the attention of the field researchers. Purchased by Ali Muftah in 2025.

Physical characteristics: The total collected mass was approximately 2 kg. The deposit samples display an exterior partially covered with dark, slightly abraded fusion crust. Sawcut surface reveals many distinctive mm-sized brown-green olivine phenocrysts set in light tan-colored, fine-grained groundmass.

Petrography: (C. Agee, UNM) Electron microprobe analysis of a polished mount shows this meteorite to be an olivine-phyric shergottite. Olivine phenocrysts display core-rim igneous zoning. Plagioclase has been converted to maskelynite. Fine-grained pigeonite and maskelynite make up the groundmass. Minor amounts of chromite, Ti-magnetite, and troilite are ubiquitous.

Geochemistry: (T. Shisseh, UNM) Olivine Fa32.6±12.1, Fe/Mn=53±4, n=13; pigeonite Fs23.3±3.2Wo4.9±2.2, Fe/Mn=30±1, n=17; maskelynite An54.9±3.5Ab44.7±3.5, n=4.

Classification: Martian, olivine-phyric shergottite. Visually, the macroscopic texture of this meteorite is reminiscent of NWA 10416, however they are not paired. This meteorite lacks augite and altered olivine, it also has maskelynite-only, with no remnant plagioclase present. This meteorite has olivine that is significantly more forsteritic than NWA 10416.

Specimens: 48 g on deposit at UNM, Ali Muftah holds the main mass, Eric Twelker holds a 410.7 g piece.

Gyarub Zangbo 001 Pallasite #33 - 8 g

Gyarub Zangbo 001 Pallasite #33 – 8 g

397,80 $

Gyarub Zangbo is a pallasite meteorite discovered in Tibet in 2020, weighing just 18 kg.
Its mineral composition, the oxygen and chromium isotopes in the olivine, and the metallic phase classify this pallasite as an anomalous carbonaceous pallasite.

Gyarub Zangbo appears to be a unique pallasite collected from an asteroid not yet represented in the pallasite collection.

 

Pallasites are unique stony-iron meteorites composed primarily of olivine and iron-rich metal.
They are believed to have formed in the boundary region between the core and the mantle of asteroids, within the asteroids themselves.

Pallasites are meteorites composed of olivine crystals embedded in an iron-nickel matrix.
Pallasites are among the most aesthetically pleasing meteorites.

Exceptional quality !

A thin, translucent slice protected by a very thin layer of resin.

Comes with certificate.

 

Gyarub Zangbo 001 Pallasite #32 - 3,5 g

Gyarub Zangbo 001 Pallasite #32 – 3,5 g

327,60 $

Gyarub Zangbo is a pallasite meteorite discovered in Tibet in 2020, weighing just 18 kg.
Its mineral composition, the oxygen and chromium isotopes in the olivine, and the metallic phase classify this pallasite as an anomalous carbonaceous pallasite.

Gyarub Zangbo appears to be a unique pallasite collected from an asteroid not yet represented in the pallasite collection.

 

Pallasites are unique stony-iron meteorites composed primarily of olivine and iron-rich metal.
They are believed to have formed in the boundary region between the core and the mantle of asteroids, within the asteroids themselves.

Pallasites are meteorites composed of olivine crystals embedded in an iron-nickel matrix.
Pallasites are among the most aesthetically pleasing meteorites.

Exceptional quality !

A thin, translucent slice protected by a very thin layer of resin.

Comes with certificate.

 

Gyarub Zangbo 001 Pallasite #31 - 5,6 g

Gyarub Zangbo 001 Pallasite #31 – 5,6 g

366,20 $

Gyarub Zangbo is a pallasite meteorite discovered in Tibet in 2020, weighing just 18 kg.
Its mineral composition, the oxygen and chromium isotopes in the olivine, and the metallic phase classify this pallasite as an anomalous carbonaceous pallasite.

Gyarub Zangbo appears to be a unique pallasite collected from an asteroid not yet represented in the pallasite collection.

 

Pallasites are unique stony-iron meteorites composed primarily of olivine and iron-rich metal.
They are believed to have formed in the boundary region between the core and the mantle of asteroids, within the asteroids themselves.

Pallasites are meteorites composed of olivine crystals embedded in an iron-nickel matrix.
Pallasites are among the most aesthetically pleasing meteorites.

Exceptional quality !

A thin, translucent slice protected by a very thin layer of resin.

Comes with certificate.

 

Gyarub Zangbo 001 Pallasite #30 - 5,7 g

Gyarub Zangbo 001 Pallasite #30 – 5,7 g

367,38 $

Gyarub Zangbo is a pallasite meteorite discovered in Tibet in 2020, weighing just 18 kg.
Its mineral composition, the oxygen and chromium isotopes in the olivine, and the metallic phase classify this pallasite as an anomalous carbonaceous pallasite.

Gyarub Zangbo appears to be a unique pallasite collected from an asteroid not yet represented in the pallasite collection.

 

Pallasites are unique stony-iron meteorites composed primarily of olivine and iron-rich metal.
They are believed to have formed in the boundary region between the core and the mantle of asteroids, within the asteroids themselves.

Pallasites are meteorites composed of olivine crystals embedded in an iron-nickel matrix.
Pallasites are among the most aesthetically pleasing meteorites.

Exceptional quality !

A thin, translucent slice protected by a very thin layer of resin.

Comes with certificate.

 

NWA 15878 OC4-melt breccia #14 - 988 gOut of stock

NWA 15878 OC4-melt breccia #14 – 988 g

4.680,00 $

A new type of chondrite meteorite has just been discovered; it is not an H, L or LL type chondrite.

This new type has been named OC4 (ordinary chondrite of petrological type 4).
This meteorite contains a high proportion of metal and its cross-sections are very attractive.

A real novelty !

 

 

 

NWA 16059 EL6 #2 - 9,6 gOut of stock

NWA 16059 EL6 #2 – 9,6 g

169,64 $

NWA 16059 is a low-metal enstatite chondrite meteorite weighing just 80 grams.

This type of meteorite is quite rare on the market.

Enstatite chondrites are considered relics of the primordial material that formed the Earth.

Very attractive!

NWA 16059 EL6 #1 - 8,7 gOut of stock

NWA 16059 EL6 #1 – 8,7 g

153,28 $

NWA 16059 is a low-metal enstatite chondrite meteorite weighing just 80 grams.

This type of meteorite is quite rare on the market.

Enstatite chondrites are considered relics of the primordial material that formed the Earth.

Very attractive !

NWA 18041 Howardite Anormale #6 - 0,4 g

NWA 18041 Howardite Anormale #6 – 0,4 g

21,06 $

NWA 18041 is an anomalous Howardite meteorite weighing just 190.8 grams.

To date, only four meteorites of this type have been discovered !

Howardite meteorites originate from the asteroid Vesta, which is located between Mars and Jupiter.

 

NWA 18041 Howardite Anormale #5 - 0,5 gOut of stock

NWA 18041 Howardite Anormale #5 – 0,5 g

25,74 $

NWA 18041 is an anomalous Howardite meteorite weighing just 190.8 grams.

To date, only four meteorites of this type have been discovered !

Howardite meteorites originate from the asteroid Vesta, which is located between Mars and Jupiter.

 

NWA 18041 Howardite Anormale #4 - 1 g

NWA 18041 Howardite Anormale #4 – 1 g

46,80 $

NWA 18041 is an anomalous Howardite meteorite weighing just 190.8 grams.

To date, only four meteorites of this type have been discovered !

Howardite meteorites originate from the asteroid Vesta, which is located between Mars and Jupiter.