Rock Identifier
Iron Meteorite (Siderite (Fe-Ni alloy, primarily Kamacite and Taenite)) — igneous
igneous

Iron Meteorite

Siderite (Fe-Ni alloy, primarily Kamacite and Taenite)

Hardness: 4-5 on Mohs scale; Color: Dark brown to black (fusion crust/weathered) or metallic silver (fresh interior); Luster: Metallic; Crystal Structure: Isometric (often with Widmanstätten patterns); Cleavage: None; Specific Gravity: 7.0–8.0 (extremely heavy).

Hardness
4-5 on Mohs scale
Luster
Metallic
Identified More igneous

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Physical properties

Hardness: 4-5 on Mohs scale; Color: Dark brown to black (fusion crust/weathered) or metallic silver (fresh interior); Luster: Metallic; Crystal Structure: Isometric (often with Widmanstätten patterns); Cleavage: None; Specific Gravity: 7.0–8.0 (extremely heavy).

Formation & geological history

Formed in the molten cores of asteroids or planetesimals during the early formation of the solar system (approx. 4.5 billion years ago) that were later shattered by collisions.

Uses & applications

Used primarily for scientific research, high-end collector specimens, unique jewelry (slices), and as a historical source of iron before ore mining.

Geological facts

Iron meteorites represent the cores of early planetary bodies. The Gibeon meteorite and Canyon Diablo (Meteor Crater) specimens are among the most famous examples of this material.

Field identification & locations

Identify by extreme weight for its size, strong magnetism, and a characteristic 'fusion crust' or regmaglypts (thumbprint-like indentations) on the surface. Found globally but most easily recovered in deserts or polar regions.