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• Eucrite Meteorites

Eucrite meteorites are part of the HED (Howardite–Eucrite–Diogenite) group and are believed to originate from the crust of asteroid Vesta, one of the largest bodies in the asteroid belt. Eucrites are achondrite meteorites, meaning they formed through volcanic processes similar to igneous rocks on Earth.

Formed over 4.5 billion years ago, eucrite meteorites represent ancient basaltic lava flows that solidified on the surface of a differentiated asteroid. Their composition and texture provide important insight into early planetary crust formation in the solar system.

Eucrites typically display fine-grained basaltic textures and can range from light gray to darker tones depending on mineral composition. These scientifically important meteorites are highly collectible and represent genuine material from the crust of asteroid Vesta.