Rock Identifier
Stardust (Micrometeorite) (Chondrite / Micrometeorite (Extraterrestrial Silicate)) — igneous
igneous

Stardust (Micrometeorite)

Chondrite / Micrometeorite (Extraterrestrial Silicate)

Hardness: 5-6 (Mohs); Color: Black, charcoal grey, or dark brown; Luster: Metallic to sub-metallic; Structure: Often spherical or irregular scoria; Specific Gravity: 3.0-3.8.

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

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Physical properties

Hardness: 5-6 (Mohs); Color: Black, charcoal grey, or dark brown; Luster: Metallic to sub-metallic; Structure: Often spherical or irregular scoria; Specific Gravity: 3.0-3.8.

Formation & geological history

Formed from the debris of the early solar system roughly 4.6 billion years ago. These particles enter Earth's atmosphere at high speeds, melting into 'cosmic spherules' due to friction before settling on the surface.

Uses & applications

Primarily used for scientific research to understand the chemical composition of the early solar nebula and the origins of water/organic molecules on Earth.

Geological facts

Approximately 5,200 tons of micrometeorites fall to Earth every year. They are the most common form of extraterrestrial matter found on our planet.

Field identification & locations

Identified by their magnetic properties and unique spherical shape under a microscope. Collectors often find them by placing magnets in rain gutters or searching in clean, isolated environments like Antarctic ice or deep-sea sediments.