Out of stock

NWA 7397 #1 Paired – 2,7 g

802,60 $

NWA 7397 is a Martian meteorite of the shergottite type, it was discovered in the mythical concentration zone of Chwichiya in Morocco.

The piece for sale is of great quality and has a fusion crust.

The price of Martian meteorites is only increasing, they have become rarer than lunar meteorites.

 

 

Jdiriya 005 #7 Aubrite – 1 g

59,45 $

Jdiriya 005 is an Aubrite meteorite of only 35.6 grams, discovered by Brahim Ikken in 2018 in Morocco.

A new theory carried by a French scientific team talks about the possibility of a link between the Aubrites and the planet Mercury.

To date only 76 such meteorites have been classified.

It is a rare type of meteorite, difficult to find on the market.

The name Aubrites is linked to the fall of a meteorite in Aubres, France in 1836. They are composed mainly of orthopyroxene to enstatite.

Writeup from MB 111:

Jdiriya 005 27°33’23.45″N, 10°31’29.87″W

Saguia el Hamra, Western Sahara

Find: 2018

Classification: Enstatite achondrite (Aubrite)

History: Found by Brahim Ikken in 2018. Bought By Jean Redelsperger from Mohamed Elguirah in 2021.

Physical characteristics: Several irregular dark pieces.

Petrography: (J. Gattacceca, B. Devouard, CEREGE) Coarse-grained unbrecciated rock with granular texture made up primarily of enstatite (61 vol%) with typical grain size 5mm. No relict chondrules are observed. Other silicates are sodic plagioclase (3.6 vol%) with typical gain size 700 μm, and Si-rich glass. Opaque minerals (35 vol%), under the form of mm sized rounded grains, are all weathered except Zn-rich daubreelite that makes up 0.2 vol% of the meteorite.

Geochemistry: Enstatite Fs0.3±0.2Wo0.6±0.1, CaO 0.33±0.06 (n=6). Plagioclase An6.7±0.1Ab89.7±0.1Or3.6±0.1 (n=3). Daubréelite contains up to 6 wt% Zn.

Classification: Aubrite.

Specimens: Type specimen at CEREGE. Main mass with Jean Redelsperger.

 

Out of stock

Jdiriya 005 #6 Aubrite – 0.9 g

53,51 $

Jdiriya 005 is an Aubrite meteorite of only 35.6 grams, discovered by Brahim Ikken in 2018 in Morocco.

A new theory carried by a French scientific team talks about the possibility of a link between the Aubrites and the planet Mercury.

To date only 76 such meteorites have been classified.

It is a rare type of meteorite, difficult to find on the market.

The name Aubrites is linked to the fall of a meteorite in Aubres, France in 1836. They are composed mainly of orthopyroxene to enstatite.

Writeup from MB 111:

Jdiriya 005 27°33’23.45″N, 10°31’29.87″W

Saguia el Hamra, Western Sahara

Find: 2018

Classification: Enstatite achondrite (Aubrite)

History: Found by Brahim Ikken in 2018. Bought By Jean Redelsperger from Mohamed Elguirah in 2021.

Physical characteristics: Several irregular dark pieces.

Petrography: (J. Gattacceca, B. Devouard, CEREGE) Coarse-grained unbrecciated rock with granular texture made up primarily of enstatite (61 vol%) with typical grain size 5mm. No relict chondrules are observed. Other silicates are sodic plagioclase (3.6 vol%) with typical gain size 700 μm, and Si-rich glass. Opaque minerals (35 vol%), under the form of mm sized rounded grains, are all weathered except Zn-rich daubreelite that makes up 0.2 vol% of the meteorite.

Geochemistry: Enstatite Fs0.3±0.2Wo0.6±0.1, CaO 0.33±0.06 (n=6). Plagioclase An6.7±0.1Ab89.7±0.1Or3.6±0.1 (n=3). Daubréelite contains up to 6 wt% Zn.

Classification: Aubrite.

Specimens: Type specimen at CEREGE. Main mass with Jean Redelsperger.

 

Out of stock

Jdiriya 005 #5 Aubrite – 1,3 g

77,29 $

Jdiriya 005 is an Aubrite meteorite of only 35.6 grams, discovered by Brahim Ikken in 2018 in Morocco.

A new theory carried by a French scientific team talks about the possibility of a link between the Aubrites and the planet Mercury.

To date only 76 such meteorites have been classified.

It is a rare type of meteorite, difficult to find on the market.

The name Aubrites is linked to the fall of a meteorite in Aubres, France in 1836. They are composed mainly of orthopyroxene to enstatite.

Writeup from MB 111:

Jdiriya 005 27°33’23.45″N, 10°31’29.87″W

Saguia el Hamra, Western Sahara

Find: 2018

Classification: Enstatite achondrite (Aubrite)

History: Found by Brahim Ikken in 2018. Bought By Jean Redelsperger from Mohamed Elguirah in 2021.

Physical characteristics: Several irregular dark pieces.

Petrography: (J. Gattacceca, B. Devouard, CEREGE) Coarse-grained unbrecciated rock with granular texture made up primarily of enstatite (61 vol%) with typical grain size 5mm. No relict chondrules are observed. Other silicates are sodic plagioclase (3.6 vol%) with typical gain size 700 μm, and Si-rich glass. Opaque minerals (35 vol%), under the form of mm sized rounded grains, are all weathered except Zn-rich daubreelite that makes up 0.2 vol% of the meteorite.

Geochemistry: Enstatite Fs0.3±0.2Wo0.6±0.1, CaO 0.33±0.06 (n=6). Plagioclase An6.7±0.1Ab89.7±0.1Or3.6±0.1 (n=3). Daubréelite contains up to 6 wt% Zn.

Classification: Aubrite.

Specimens: Type specimen at CEREGE. Main mass with Jean Redelsperger.

 

Out of stock

Jdiriya 005 #4 Aubrite – 4,3 g

255,64 $

Jdiriya 005 is an Aubrite meteorite of only 35.6 grams, discovered by Brahim Ikken in 2018 in Morocco.

A new theory carried by a French scientific team talks about the possibility of a link between the Aubrites and the planet Mercury.

To date only 76 such meteorites have been classified.

It is a rare type of meteorite, difficult to find on the market.

The name Aubrites is linked to the fall of a meteorite in Aubres, France in 1836. They are composed mainly of orthopyroxene to enstatite.

Writeup from MB 111:

Jdiriya 005 27°33’23.45″N, 10°31’29.87″W

Saguia el Hamra, Western Sahara

Find: 2018

Classification: Enstatite achondrite (Aubrite)

History: Found by Brahim Ikken in 2018. Bought By Jean Redelsperger from Mohamed Elguirah in 2021.

Physical characteristics: Several irregular dark pieces.

Petrography: (J. Gattacceca, B. Devouard, CEREGE) Coarse-grained unbrecciated rock with granular texture made up primarily of enstatite (61 vol%) with typical grain size 5mm. No relict chondrules are observed. Other silicates are sodic plagioclase (3.6 vol%) with typical gain size 700 μm, and Si-rich glass. Opaque minerals (35 vol%), under the form of mm sized rounded grains, are all weathered except Zn-rich daubreelite that makes up 0.2 vol% of the meteorite.

Geochemistry: Enstatite Fs0.3±0.2Wo0.6±0.1, CaO 0.33±0.06 (n=6). Plagioclase An6.7±0.1Ab89.7±0.1Or3.6±0.1 (n=3). Daubréelite contains up to 6 wt% Zn.

Classification: Aubrite.

Specimens: Type specimen at CEREGE. Main mass with Jean Redelsperger.

 

Out of stock

Jdiriya 005 #3 Aubrite – 4,7 g

279,42 $

Jdiriya 005 is an Aubrite meteorite of only 35.6 grams, discovered by Brahim Ikken in 2018 in Morocco.

A new theory carried by a French scientific team talks about the possibility of a link between the Aubrites and the planet Mercury.

To date only 76 such meteorites have been classified.

It is a rare type of meteorite, difficult to find on the market.

The name Aubrites is linked to the fall of a meteorite in Aubres, France in 1836. They are composed mainly of orthopyroxene to enstatite.

Writeup from MB 111:

Jdiriya 005 27°33’23.45″N, 10°31’29.87″W

Saguia el Hamra, Western Sahara

Find: 2018

Classification: Enstatite achondrite (Aubrite)

History: Found by Brahim Ikken in 2018. Bought By Jean Redelsperger from Mohamed Elguirah in 2021.

Physical characteristics: Several irregular dark pieces.

Petrography: (J. Gattacceca, B. Devouard, CEREGE) Coarse-grained unbrecciated rock with granular texture made up primarily of enstatite (61 vol%) with typical grain size 5mm. No relict chondrules are observed. Other silicates are sodic plagioclase (3.6 vol%) with typical gain size 700 μm, and Si-rich glass. Opaque minerals (35 vol%), under the form of mm sized rounded grains, are all weathered except Zn-rich daubreelite that makes up 0.2 vol% of the meteorite.

Geochemistry: Enstatite Fs0.3±0.2Wo0.6±0.1, CaO 0.33±0.06 (n=6). Plagioclase An6.7±0.1Ab89.7±0.1Or3.6±0.1 (n=3). Daubréelite contains up to 6 wt% Zn.

Classification: Aubrite.

Specimens: Type specimen at CEREGE. Main mass with Jean Redelsperger.

 

Jdiriya 005 #2 Aubrite – 3,9 g

231,86 $

Jdiriya 005 is an Aubrite meteorite of only 35.6 grams, discovered by Brahim Ikken in 2018 in Morocco.

A new theory carried by a French scientific team talks about the possibility of a link between the Aubrites and the planet Mercury.

To date only 76 such meteorites have been classified.

It is a rare type of meteorite, difficult to find on the market.

The name Aubrites is linked to the fall of a meteorite in Aubres, France in 1836. They are composed mainly of orthopyroxene to enstatite.

Writeup from MB 111:

Jdiriya 005 27°33’23.45″N, 10°31’29.87″W

Saguia el Hamra, Western Sahara

Find: 2018

Classification: Enstatite achondrite (Aubrite)

History: Found by Brahim Ikken in 2018. Bought By Jean Redelsperger from Mohamed Elguirah in 2021.

Physical characteristics: Several irregular dark pieces.

Petrography: (J. Gattacceca, B. Devouard, CEREGE) Coarse-grained unbrecciated rock with granular texture made up primarily of enstatite (61 vol%) with typical grain size 5mm. No relict chondrules are observed. Other silicates are sodic plagioclase (3.6 vol%) with typical gain size 700 μm, and Si-rich glass. Opaque minerals (35 vol%), under the form of mm sized rounded grains, are all weathered except Zn-rich daubreelite that makes up 0.2 vol% of the meteorite.

Geochemistry: Enstatite Fs0.3±0.2Wo0.6±0.1, CaO 0.33±0.06 (n=6). Plagioclase An6.7±0.1Ab89.7±0.1Or3.6±0.1 (n=3). Daubréelite contains up to 6 wt% Zn.

Classification: Aubrite.

Specimens: Type specimen at CEREGE. Main mass with Jean Redelsperger.

 

Out of stock

Jdiriya 005 #1 Aubrite – 3,1 g

184,30 $

Jdiriya 005 is an Aubrite meteorite of only 35.6 grams, discovered by Brahim Ikken in 2018 in Morocco.

A new theory carried by a French scientific team talks about the possibility of a link between the Aubrites and the planet Mercury.

To date only 76 such meteorites have been classified.

It is a rare type of meteorite, difficult to find on the market.

The name Aubrites is linked to the fall of a meteorite in Aubres, France in 1836. They are composed mainly of orthopyroxene to enstatite.

Writeup from MB 111:

Jdiriya 005 27°33’23.45″N, 10°31’29.87″W

Saguia el Hamra, Western Sahara

Find: 2018

Classification: Enstatite achondrite (Aubrite)

History: Found by Brahim Ikken in 2018. Bought By Jean Redelsperger from Mohamed Elguirah in 2021.

Physical characteristics: Several irregular dark pieces.

Petrography: (J. Gattacceca, B. Devouard, CEREGE) Coarse-grained unbrecciated rock with granular texture made up primarily of enstatite (61 vol%) with typical grain size 5mm. No relict chondrules are observed. Other silicates are sodic plagioclase (3.6 vol%) with typical gain size 700 μm, and Si-rich glass. Opaque minerals (35 vol%), under the form of mm sized rounded grains, are all weathered except Zn-rich daubreelite that makes up 0.2 vol% of the meteorite.

Geochemistry: Enstatite Fs0.3±0.2Wo0.6±0.1, CaO 0.33±0.06 (n=6). Plagioclase An6.7±0.1Ab89.7±0.1Or3.6±0.1 (n=3). Daubréelite contains up to 6 wt% Zn.

Classification: Aubrite.

Specimens: Type specimen at CEREGE. Main mass with Jean Redelsperger.

 

Out of stock

Al Haggounia 002 H4 #2 – 86 g

61,82 $

Al Haggounia 002 is a meteorite of 1350 g classified H4, it was discovered in the Western Sahara in the Al Haggounia concentration area in 2014.

There are only two pieces left for sale.

Out of stock

Al Haggounia 002 H4 #1 – 106 g

76,09 $

Al Haggounia 002 is a meteorite of 1350 g classified H4, it was discovered in the Western Sahara in the Al Haggounia concentration area in 2014.

There are only two pieces left for sale.

Babaudus #5 – 122 g

17,83 $
An impactite is a terrestrial rock modified by the impact of a large meteorite.
These rocks contain an agglomeration of fallout dust and fragments.
The Rochechouart impactites were formed as a result of a meteorite impact about 207 million years ago in New Aquitaine in the Rochechouart district.
The impact crater of the Rochechouart meteorite is called “Astroblème” because it is no longer visible following erosion.
There are several types of rocks :
Babaudus-type breccias, rich in fluid-textured glass and vacuoles, are found only in the center of the astroblast.
These breccias are contaminated with chromium, nickel and cobalt, metals coming mostly from the asteroid.
The “breccias” of Montoume type, red because of their richness in iron, metal supposed to come from the asteroid.
The “breccias” of Chassenon type, debris of glass of greenish tint.
The “breccias” of Rochechouart type, contain little glass and are constituted of elements of varied size and lithology.
Out of stock

Babaudus #4 – 105 g

17,83 $
An impactite is a terrestrial rock modified by the impact of a large meteorite.
These rocks contain an agglomeration of fallout dust and fragments.
The Rochechouart impactites were formed as a result of a meteorite impact about 207 million years ago in New Aquitaine in the Rochechouart district.
The impact crater of the Rochechouart meteorite is called “Astroblème” because it is no longer visible following erosion.
There are several types of rocks :
Babaudus-type breccias, rich in fluid-textured glass and vacuoles, are found only in the center of the astroblast.
These breccias are contaminated with chromium, nickel and cobalt, metals coming mostly from the asteroid.
The “breccias” of Montoume type, red because of their richness in iron, metal supposed to come from the asteroid.
The “breccias” of Chassenon type, debris of glass of greenish tint.
The “breccias” of Rochechouart type, contain little glass and are constituted of elements of varied size and lithology.
Out of stock

Babaudus #3 – 139 g

19,02 $
An impactite is a terrestrial rock modified by the impact of a large meteorite.
These rocks contain an agglomeration of fallout dust and fragments.
The Rochechouart impactites were formed as a result of a meteorite impact about 207 million years ago in New Aquitaine in the Rochechouart district.
The impact crater of the Rochechouart meteorite is called “Astroblème” because it is no longer visible following erosion.
There are several types of rocks :
Babaudus-type breccias, rich in fluid-textured glass and vacuoles, are found only in the center of the astroblast.
These breccias are contaminated with chromium, nickel and cobalt, metals coming mostly from the asteroid.
The “breccias” of Montoume type, red because of their richness in iron, metal supposed to come from the asteroid.
The “breccias” of Chassenon type, debris of glass of greenish tint.
The “breccias” of Rochechouart type, contain little glass and are constituted of elements of varied size and lithology.
Out of stock

Babaudus #2 – 167 g

19,02 $
An impactite is a terrestrial rock modified by the impact of a large meteorite.
These rocks contain an agglomeration of fallout dust and fragments.
The Rochechouart impactites were formed as a result of a meteorite impact about 207 million years ago in New Aquitaine in the Rochechouart district.
The impact crater of the Rochechouart meteorite is called “Astroblème” because it is no longer visible following erosion.
There are several types of rocks :
Babaudus-type breccias, rich in fluid-textured glass and vacuoles, are found only in the center of the astroblast.
These breccias are contaminated with chromium, nickel and cobalt, metals coming mostly from the asteroid.
The “breccias” of Montoume type, red because of their richness in iron, metal supposed to come from the asteroid.
The “breccias” of Chassenon type, debris of glass of greenish tint.
The “breccias” of Rochechouart type, contain little glass and are constituted of elements of varied size and lithology.
Out of stock

Babaudus #1 – 116 g

17,83 $
An impactite is a terrestrial rock modified by the impact of a large meteorite.
These rocks contain an agglomeration of fallout dust and fragments.
The Rochechouart impactites were formed as a result of a meteorite impact about 207 million years ago in New Aquitaine in the Rochechouart district.
The impact crater of the Rochechouart meteorite is called “Astroblème” because it is no longer visible following erosion.
There are several types of rocks :
Babaudus-type breccias, rich in fluid-textured glass and vacuoles, are found only in the center of the astroblast.
These breccias are contaminated with chromium, nickel and cobalt, metals coming mostly from the asteroid.
The “breccias” of Montoume type, red because of their richness in iron, metal supposed to come from the asteroid.
The “breccias” of Chassenon type, debris of glass of greenish tint.
The “breccias” of Rochechouart type, contain little glass and are constituted of elements of varied size and lithology.

Al Haggounia 001 Enstatite #7 – 3,2 g

14,27 $

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 Enstatite #6 – 7,8 g

28,54 $

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.

 

 

Out of stock

Al Haggounia 001 Enstatite #5 – 8,9 g

32,10 $

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.