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NWA 15417 – Eucrite Achondrite Meteorite Main Mass
Mesosiderites are believed to have formed through massive asteroid collisions early in the history of the solar system
purchased in 2020 from a dealer in Morocco
Visible minerals include low-Ca pyroxene and plagioclase along with iron-nickel metal phases such as kamacite and taenite
making it attractive for collectors seeking better visibility of internal features
NWA 14868 Diogenite PM 1.0 G Martian NWA 15417 – Eucrite AchondriteNWA 14868 Diogenite Meteorite Polymict HED Achondrite for SaleA rare polymict diogenite from Northwest Africa, NWA 14868 is part of the HED meteorite family, likely from asteroid 4 Vesta. This specimen features light brown fragments composed mainly of orthopyroxene, with minor plagioclase, silica, chromite, troilite, and metal. A stunning example of planetary crust material from deep space. DIM: 16 X10X2 MM
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