Rock Identifier
Micro-Meteorite (Micrometeoroid) (Extraterrestrial Spherule (Silicate or Iron-Nickel)) — mineral
mineral

Micro-Meteorite (Micrometeoroid)

Extraterrestrial Spherule (Silicate or Iron-Nickel)

Hardness: 5-6 (variable); Color: Black, brown, or dark grey; Luster: Metallic to sub-metallic; Crystal Structure: Often amorphous or polycrystalline due to rapid cooling; Size: 0.1 to 2 mm; Specific Gravity: Varying based on iron content.

Hardness
5-6 (variable)
Color
Black, brown, or dark grey
Luster
Metallic to sub-metallic
Identified More mineral

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Physical properties

Hardness: 5-6 (variable); Color: Black, brown, or dark grey; Luster: Metallic to sub-metallic; Crystal Structure: Often amorphous or polycrystalline due to rapid cooling; Size: 0.1 to 2 mm; Specific Gravity: Varying based on iron content.

Formation & geological history

Formed from interplanetary dust particles that melt and re-solidify upon entering the Earth's atmosphere. Most originate from comets or asteroids and are billions of years old.

Uses & applications

Primarily used for scientific research to understand the composition of the early solar system. High collector value for micrometeorite hunters.

Geological facts

Approximately 37,000 to 78,000 tons of space dust falls to Earth every year. Jon Larsen, a Norwegian jazz musician, pioneered the method to find these 'urban micrometeorites' on rooftops.

Field identification & locations

Identified by their spherical or aerodynamic shape and magnetic properties (if iron-nickel). Common locations include house gutters, flat rooftops, and polar ice sheets. Use a strong magnet and microscope for field identification.