
mineral
Iron Meteorite
Siderite (meteoritic iron, Fe-Ni alloy)
Hardness: 4.0-5.0 on Mohs scale; Color: Silvery-grey to black fusion crust; Luster: Metallic; Crystal Structure: Isometric; Cleavage: None; Specific Gravity: 7.0-8.0 (very dense)
- Hardness
- 4
- Color
- Silvery-grey to black fusion crust
- Luster
- Metallic
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Physical properties
Hardness: 4.0-5.0 on Mohs scale; Color: Silvery-grey to black fusion crust; Luster: Metallic; Crystal Structure: Isometric; Cleavage: None; Specific Gravity: 7.0-8.0 (very dense)
Formation & geological history
Formed in the molten cores of planetary embryos or asteroids approximately 4.5 billion years ago. They reach Earth after survived atmospheric entry which creates regmaglypts (thumbprint-like indentations) and a fusion crust.
Uses & applications
Highly prized by collectors and researchers for studying the early solar system. Used historically for tool making and currently in high-end jewelry (Widmanstatten pattern slices).
Geological facts
Iron meteorites consist mostly of kamacite and taenite minerals. When etched with acid, they often reveal the Widmanstatten pattern, a unique interlocking crystal structure that cannot be replicated on Earth.
Field identification & locations
Identify by extreme density (weight), strong magnetic attraction, and the presence of a thin, dark fusion crust. Often found in deserts or Antarctica where they stand out against the landscape.
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