Rock Identifier
Iron meteorite fragment (likely weathered meteorite) (Fe–Ni metal, commonly kamacite with taenite; possible stony-iron or iron-oxide fusion crust) — meteorite
meteorite

Iron meteorite fragment (likely weathered meteorite)

Fe–Ni metal, commonly kamacite with taenite; possible stony-iron or iron-oxide fusion crust

AI-generated identification · may be incorrect

Dark metallic-gray, irregular thumb-sized fragment with rusty brown oxidation and a lighter gray, possibly melted/fused surface. Typical iron meteorites have Mohs hardness about 4–5, metallic luster, high density (~7–8 g/cm³), and no cleavage; visual identification alone is uncertain.

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Physical properties

Dark metallic-gray, irregular thumb-sized fragment with rusty brown oxidation and a lighter gray, possibly melted/fused surface. Typical iron meteorites have Mohs hardness about 4–5, metallic luster, high density (~7–8 g/cm³), and no cleavage; visual identification alone is uncertain.

Formation & geological history

Formed in the metallic core of a differentiated asteroid, then melted during atmospheric entry and cooled in space; most are older than Earth (~4.56 billion years). The pale crust may be terrestrial weathering or impact-fused material.

Uses & applications

Primarily a collector specimen; cut and etched iron meteorites are valued for Widmanstätten patterns, while nickel-iron is occasionally used decoratively.

Geological facts

A strong magnet attraction and unusually high weight are useful clues, but slag, industrial iron, and hematite can look similar. A definitive identification requires nickel testing, density, and ideally laboratory analysis.

Field identification & locations

Check for regmaglypts, a thin fusion crust, magnetic response, and absence of vesicles; avoid destructive acid tests. Common finds include deserts, Antarctica, and known strewn fields.