Showing 433–450 of 1197 results

Out of stock

NWA 13881 CV3 #10- 4,8 g

24,97 $

NWA 13881 is a CV3 type meteorite with very large chondrules.

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.

 

Out of stock

NWA 13881 CV3 #9- 14,9 g

95,12 $

NWA 13881 is a CV3 type meteorite with very large chondrules.

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 13881 CV3 #8- 13,5 g

70,15 $

NWA 13881 is a CV3 type meteorite with very large chondrules.

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 13881 CV3 #7- 74,8 g

399,52 $

NWA 13881 is a CV3 type meteorite with very large chondrules.

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.

 

Out of stock

Chwichiya 002 C3.00 Ung #43 – 2,1 g

620,68 $

Chwichiya 002 is an ordinary carbonaceous chondrite of type C3.00 ungrouped, it is the most primitive type that has ever been found in this date, it has not undergone any hydrated phase and no heating before its expulsion from the parent body.
This meteorite is perhaps one of the most important meteorites of all times, no doubt that the knowledge of our solar system will advance thanks to it.

It was discovered in the Western Sahara.
A must for a collection!

Out of stock

Chwichiya 002 C3.00 Ung #42 – 1,2 g

344,82 $

Chwichiya 002 is an ordinary carbonaceous chondrite of type C3.00 ungrouped, it is the most primitive type that has ever been found in this date, it has not undergone any hydrated phase and no heating before its expulsion from the parent body.
This meteorite is perhaps one of the most important meteorites of all times, no doubt that the knowledge of our solar system will advance thanks to it.

It was discovered in the Western Sahara.
A must for a collection!

Out of stock

Chwichiya 002 C3.00 Ung #40 – 1,1 g

324,60 $

Chwichiya 002 is an ordinary carbonaceous chondrite of type C3.00 ungrouped, it is the most primitive type that has ever been found in this date, it has not undergone any hydrated phase and no heating before its expulsion from the parent body.
This meteorite is perhaps one of the most important meteorites of all times, no doubt that the knowledge of our solar system will advance thanks to it.

It was discovered in the Western Sahara.
A must for a collection!

Out of stock

Chwichiya 002 C3.00 Ung #39 – 1 g

294,88 $

Chwichiya 002 is an ordinary carbonaceous chondrite of type C3.00 ungrouped, it is the most primitive type that has ever been found in this date, it has not undergone any hydrated phase and no heating before its expulsion from the parent body.
This meteorite is perhaps one of the most important meteorites of all times, no doubt that the knowledge of our solar system will advance thanks to it.

It was discovered in the Western Sahara.
A must for a collection!

Out of stock

Chwichiya 002 C3.00 Ung #38 – 0,24 g

71,34 $

Chwichiya 002 is an ordinary carbonaceous chondrite of type C3.00 ungrouped, it is the most primitive type that has ever been found in this date, it has not undergone any hydrated phase and no heating before its expulsion from the parent body.
This meteorite is perhaps one of the most important meteorites of all times, no doubt that the knowledge of our solar system will advance thanks to it.

It was discovered in the Western Sahara.
A must for a collection!

Chwichiya 002 C3.00 Ung #37 – 0,21 g

61,82 $

Chwichiya 002 is an ordinary carbonaceous chondrite of type C3.00 ungrouped, it is the most primitive type that has ever been found in this date, it has not undergone any hydrated phase and no heating before its expulsion from the parent body.
This meteorite is perhaps one of the most important meteorites of all times, no doubt that the knowledge of our solar system will advance thanks to it.

It was discovered in the Western Sahara.
A must for a collection!

Chwichiya 002 C3.00 Ung #36 – 0,17 g

49,94 $

Chwichiya 002 is an ordinary carbonaceous chondrite of type C3.00 ungrouped, it is the most primitive type that has ever been found in this date, it has not undergone any hydrated phase and no heating before its expulsion from the parent body.
This meteorite is perhaps one of the most important meteorites of all times, no doubt that the knowledge of our solar system will advance thanks to it.

It was discovered in the Western Sahara.
A must for a collection!

Chwichiya 002 C3.00 Ung #35 – 0,8 g

236,62 $

Chwichiya 002 is an ordinary carbonaceous chondrite of type C3.00 ungrouped, it is the most primitive type that has ever been found in this date, it has not undergone any hydrated phase and no heating before its expulsion from the parent body.
This meteorite is perhaps one of the most important meteorites of all times, no doubt that the knowledge of our solar system will advance thanks to it.

It was discovered in the Western Sahara.
A must for a collection!

Acfer 328 CV3 #1- 2,7 g

95,12 $

Acfer 328 is a CV3 carbonaceous meteorite discovered by two Frenchmen, F. Beroud and C. Boucher, in Algeria in 2001, and classified by the Museum National d’Histoire Naturelle in Paris.

 

Jiddat al Harasis 626 Eucrite, polymict #1 – 6 g

261,59 $

This beautiful meteorite was discovered by Marie Gerbet in 2010 in the Jiddat al Harasis, a rocky desert north of the Dhofar region and in south-central Oman.

This meteorite was used by NASA to calibrate the spectrometer of the DAWN probe that studied the asteroid Vesta !

Out of stock

Itqiy EH7-an #1 – 5,63 g

1.115,32 $

To date, Itqiy is the only meteorite in the world classified as EH7-an.

It is an enstatite chondrite, an important class of chondrites that mostly exhibit sub-solar Mg/Si and refractory/Si ratios, oxygen isotopic compositions close to the terrestrial fractionation line and highly reduced mineral assemblages (containing little FeO, Si-bearing metal and sulfides of elements normally considered lithophilic).

This highly metamorphosed meteorite has a very unique texture !

The Earth seems to have been formed from celestial bodies whose composition is close to that of enstatite chondrites.

 

 

Out of stock

NWA 15169 Lunaire #23 – 50 g

2.972,58 $

NWA 15169 is a lunar meteorite discovered in 2021 in Morocco near Dakhla in the Wad Oum Sfia area by Omar Ben Chaoud and Mouloud Oudinat.

NWA 15169 is a rare lunar meteorite (anorthosite).

This is a very nice and colorful lunar meteorite offered at a very good price.

About fifteen years ago, lunar meteorites were sold for almost 1000 euros per gram !

Writeup from MB 112:

Northwest Africa 15169 (NWA 15169)

Morocco

Purchased: 2021

Classification: Lunar meteorite (anorth)

History: Found by Omar Ben Chaoud and Mouloud Oudinat in the Dakhla, Wad Oum Sfia area. Later bought by Jean Redelsperger from Mohamed Elguirah in 2021.

Physical characteristics: Several stones: a complete 50 g crusted stone, and several gray fragments without fusion crust, the largest one being 52 g.

Petrography: (J. Gattacceca, B. Devouard, CEREGE) Brecciated igneous rock composed primarily of anorthitic plagioclase, and mm-sized poikilitic microgabbroic clasts with plagioclase chadacrysts set in olivine and pyroxene. Accessory minerals: metal, ulvöspinel, chromite. Barite, from terrestrial weathering, is present as veins.

Geochemistry: Plagioclase An93.4±2.7Ab6.3±2.5Or0.2±0.2 (n=4). Olivine (altered) Fo 43.5±5.9, FeO/MnO=143.4, analytical totals 90.9±2.2 (n=9). Orthopyroxene Fs26.0Wo9.0, Fs16.3Wo36.9, FeO/MnO = 50.8 (n=2). Chromite Cr#=0.73 (n=1).

Classification: Lunar (anorthosite). Contains microgabbroic clasts. Olivine, pigeonite and plagioclase are within the ferroan anorthositic suite (FAS) field defined by Warren (1993). Olivine has been altered on Earth, as indicated by the low analytical totals.

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

Out of stock

Almahata Sitta #1 Bencubbinite – 0,45 g

1.426,84 $

Almahata Sitta is a unique meteorite !

This meteorite fell on October 7, 2008 in Sudan.

But the particularity of this meteorite is that astronomers followed it from space until it entered the atmosphere,

a world first.

Another surprise awaited scientists :

Sur les 660 météorites de la chute de Almahata Sitta qui ont été classées, on a trouvé au total 17 classifications différentes : Ureilite, H5/6, LL4, EH4/5, EL6, EL5/6, EL3, EL6, H5, CH, EH3, EL3-, EL5, EL3/4, L4-, rumuritite, et bencubinite.

Even better, diamonds contained in the meteorite indicate that it could have belonged to a planet the size of Mercury or Mars !

The slice that is being sold is part of a single piece that was only 58.63 grams.

This slice is from the “Haberer Meteorite” website.

 

El Hammami H5 #1 – 382 g

570,73 $

El Hammami is one of the first meteorites found in the Sahara and which was traded.

It was found in Mauritania in 1997, and yet it was also sold under the name of Mhamid, in Morocco, because they are Moroccans

of this city which made the trade of it.

In 1997 November, Mr. Thompson traveled to Mauritania and collected six fresh-looking stones totaling ~200 kg (individual masses of 80, 51, 30, 26,

8 and 4 kg) at the foot of the El Hammami mountains in Mauritania (1000 km southwest of Mhamid, Morocco).

Some of the material looks weathered and rusts easily, but most of it is fairly fresh.

A legend tells that the most oxidized specimens are the ones that were in direct contact with the skin of the camels used to transport the specimens.