Rock Identifier
Iron Meteorite (Siderite (comprised primarily of Kamacite and Taenite alloys)) — igneous
igneous

Iron Meteorite

Siderite (comprised primarily of Kamacite and Taenite alloys)

Hardness: 4.0-5.0 on Mohs scale; Color: Dark brown or black exterior (fusion crust), metallic silver interior; Luster: Metallic; Crystal Structure: Isometric (often showing Widmanstätten patterns when etched); Specific Gravity: 7.0-8.0 (very dense).

Hardness
4
Luster
Metallic
Identified More igneous

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Physical properties

Hardness: 4.0-5.0 on Mohs scale; Color: Dark brown or black exterior (fusion crust), metallic silver interior; Luster: Metallic; Crystal Structure: Isometric (often showing Widmanstätten patterns when etched); Specific Gravity: 7.0-8.0 (very dense).

Formation & geological history

Formed in the molten cores of differentiated asteroids roughly 4.5 billion years ago. They are liberated by catastrophic collisions in space and fall to Earth after surviving atmospheric entry.

Uses & applications

Used primarily for scientific research, high-end collector specimens, and occasionally fashioned into 'out of this world' jewelry or watch faces.

Geological facts

Iron meteorites were the first source of usable iron for humans before the Bronze Age. The Hoba meteorite in Namibia is the largest known single iron meteorite on Earth, weighing about 60 tons.

Field identification & locations

Identify in the field by its unusual weight (heavier than terrestrial rocks), strong magnetic attraction, and 'regmaglypts' (thumb-print-like indentations on the surface). Common locations include strewn fields like Campo del Cielo (Argentina) or Sikhote-Alin (Russia).