Rock Identifier
Iron-rich meteorite candidate (possibly stony-iron or iron meteorite) (Unclassified meteoritic material; likely Fe–Ni metal with weathering oxides) — meteorite
meteorite

Iron-rich meteorite candidate (possibly stony-iron or iron meteorite)

Unclassified meteoritic material; likely Fe–Ni metal with weathering oxides

AI-generated identification · may be incorrect

Dark brown-black, heavily weathered, dull to weakly metallic luster, irregular rounded shape, and a pitted surface. Likely dense and moderately hard (about 4–6 Mohs); a magnet test would be informative, while visible fusion crust or Widmanstätten patterns are not evident.

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Physical properties

Dark brown-black, heavily weathered, dull to weakly metallic luster, irregular rounded shape, and a pitted surface. Likely dense and moderately hard (about 4–6 Mohs); a magnet test would be informative, while visible fusion crust or Widmanstätten patterns are not evident.

Formation & geological history

If genuine, it formed in an asteroid and was melted or brecciated early in Solar System history, about 4.56 billion years ago, before atmospheric entry produced a fusion crust. Its appearance could also match terrestrial ironstone, slag, or hematite-rich rock.

Uses & applications

Meteorites have scientific and collector value; iron-rich terrestrial rocks are mainly curiosities or iron-ore specimens and have little industrial value as individual pieces.

Geological facts

The image alone cannot confirm a meteorite. Strong magnetism, unusually high density, a thin dark fusion crust, and lack of vesicles support meteoritic origin; rusty weathering and abundant terrestrial rock texture argue against it.

Field identification & locations

Check for magnetism, streak on unglazed ceramic, density, and nickel using a professional assay; do not cut or acid-test a potential meteorite before documentation. Common iron meteorites occur worldwide, especially in dry deserts and Antarctica.