Rock Identifier
Small metallic meteorite fragment (probable chondrite) (Unclassified ordinary chondrite; composition chiefly Fe–Ni metal, olivine, and pyroxene) — meteorite
meteorite

Small metallic meteorite fragment (probable chondrite)

Unclassified ordinary chondrite; composition chiefly Fe–Ni metal, olivine, and pyroxene

AI-generated identification · may be incorrect

Irregular dark gray-brown fragment with metallic-looking flecks and possible fusion crust; typical meteorite hardness is about 6–7 Mohs, dense, opaque, and weakly to strongly magnetic. The image is insufficient for reliable mineral or meteorite confirmation.

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Physical properties

Irregular dark gray-brown fragment with metallic-looking flecks and possible fusion crust; typical meteorite hardness is about 6–7 Mohs, dense, opaque, and weakly to strongly magnetic. The image is insufficient for reliable mineral or meteorite confirmation.

Formation & geological history

If genuine, it formed in the early Solar System about 4.56 billion years ago and later survived atmospheric entry as a meteorite fragment. Its terrestrial location and geological classification cannot be determined visually.

Uses & applications

Primarily used for scientific study and collecting; attractive authenticated specimens may be sold as display pieces or jewelry components. It has no ordinary construction use.

Geological facts

Most suspected meteorites are terrestrial slag, ironstone, or weathered rock. Confirmation requires density, magnetic response, nickel testing, petrographic examination, and ideally laboratory classification.

Field identification & locations

Possible indicators include unusually high density, a thin dark fusion crust, rounded aerodynamic edges, and magnetism; a fresh cut surface may show metal grains or chondrules. Do not rely on appearance alone.