Pack !!! Meteorite NWA 869, legendary fall Type L3-6 - 25 g






Over 20 years collecting meteorites; former museum curator and experienced restorer.
Catawiki Buyer Protection
Your payment’s safe with us until you receive your object.View details
Trustpilot 4.4 | 137154 reviews
Rated Excellent on Trustpilot.
NWA 869 meteorite, an L3-6 chondrite, from Tindouf, Algeria, weighing 25 g, with a primary fusion crust (Piedra del Aire, Costra de fusión).
Description from the seller
The NWA 869 chondrite is the largest known rocky meteorite fall, making it one of the most famous falls.
Magnificent pieces in which we can observe the primary fusion crust.
Indicative photo of pieces with a weight of 25 grams.
Chondrites are among the oldest materials in the solar system, with an estimated formation age of 4.55 billion years. They are undifferentiated meteorites, which is why they contain iron, in this case in small amounts since they are L-type.
Most of them come from the asteroid belt located between Mars and Jupiter.
A hallmark of chondrites is the presence of chondrules, small millimeter-sized spheres composed largely of silicates.
The standard model for their initial formation is that they formed during the condensation of the solar nebula, from cosmic dust.
Chondrites are considered as the earliest building blocks from which planets form.
At Expometeoritos, we handle outreach, talks, workshops, analyses, classification, and exhibitions of meteorites.
We are members of:
- IMCA (International Meteorite Collectors Association) #8187
- Meteoritical Society
- American Meteor Society
All our pieces are certified and, in addition, we provide the chemical composition analysis if the piece’s value exceeds €300, performed at our facilities by X-ray spectrography.
Seller's Story
The NWA 869 chondrite is the largest known rocky meteorite fall, making it one of the most famous falls.
Magnificent pieces in which we can observe the primary fusion crust.
Indicative photo of pieces with a weight of 25 grams.
Chondrites are among the oldest materials in the solar system, with an estimated formation age of 4.55 billion years. They are undifferentiated meteorites, which is why they contain iron, in this case in small amounts since they are L-type.
Most of them come from the asteroid belt located between Mars and Jupiter.
A hallmark of chondrites is the presence of chondrules, small millimeter-sized spheres composed largely of silicates.
The standard model for their initial formation is that they formed during the condensation of the solar nebula, from cosmic dust.
Chondrites are considered as the earliest building blocks from which planets form.
At Expometeoritos, we handle outreach, talks, workshops, analyses, classification, and exhibitions of meteorites.
We are members of:
- IMCA (International Meteorite Collectors Association) #8187
- Meteoritical Society
- American Meteor Society
All our pieces are certified and, in addition, we provide the chemical composition analysis if the piece’s value exceeds €300, performed at our facilities by X-ray spectrography.
