
meteorite
Iron Meteorite
Siderite (Iron-Nickel Alloy)
AI-generated identification · may be incorrectHardness: 4.0-5.0 on Mohs scale; Color: Dark brown/black fusion crust to metallic silver interior; Luster: Sub-metallic to metallic; Structure: Octahedrite or Hexahedrite; Specific Gravity: 7.0-8.0. Highly magnetic.
- Hardness
- 4
- Color
- Dark brown/black fusion crust to metallic silver interior
- Luster
- Sub-metallic to metallic
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Physical properties
Hardness: 4.0-5.0 on Mohs scale; Color: Dark brown/black fusion crust to metallic silver interior; Luster: Sub-metallic to metallic; Structure: Octahedrite or Hexahedrite; Specific Gravity: 7.0-8.0. Highly magnetic.
Formation & geological history
Formed in the molten cores of planetary embryos or large asteroids at the beginning of the solar system (approx. 4.5 billion years ago). These bodies were later shattered by collisions, releasing the metallic core fragments into space.
Uses & applications
Scientific research, high-end collector specimens, and occasionally used in custom jewelry or luxury cutlery (meteoritic steel).
Geological facts
Iron meteorites are composed primarily of iron and nickel. When etched with acid, many show a unique interlocking crystal pattern called 'Widmanstatten patterns' which cannot be replicated on Earth because they require millions of years of cooling.
Field identification & locations
Identified by high density, magnetic properties, and the presence of 'regmaglypts' (thumbprint-like depressions) caused by atmospheric ablation. Commonly found in arid desert regions or Antarctica where they are easily spotted.
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