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This polished slice reveals the typical mesosiderite brecciated structure with silicate clasts embedded in a fine-grained matrix containing dispersed iron-nickel metal
making them both scientifically valuable and visually stunning
Mesosiderites are believed to have formed through massive asteroid collisions early in the history of the Solar System
Official classification can be verified in the Meteorite Bulletin Database:https://www
NWA 12241 Martian Meteorite – 0
Brachinite NWA 11756 (3.22 g) L3 This polished slice reveals theNWA 11756 Olivine rich asteroid interior slice with enhanced collector appeal. This brachinite meteorite (NWA 11756) is a rare primitive achondrite, formed through partial melting processes inside early asteroids. Unlike ordinary meteorites, this specimen represents olivine rich material derived from the interior of a differentiated asteroid, offering insight into early planetary formation. Brachinites are among the rarest meteorites and are known for
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