igneous
Chondrite Meteorite
Stony Meteorite (Ordinary Chondrite)
Hardness: 5.5-6.5 (Mohs scale); Color: Black to dark brown fusion crust, lighter gray interior; Luster: Matte or dull; Crystal structure: Contains spherical silicate chondrules; Cleavage: None; Specific Gravity: 3.0-3.8
- Hardness
- 5
- Color
- Black to dark brown fusion crust, lighter gray interior
- Luster
- Matte or dull
Identified More igneous →
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Physical properties
Hardness: 5.5-6.5 (Mohs scale); Color: Black to dark brown fusion crust, lighter gray interior; Luster: Matte or dull; Crystal structure: Contains spherical silicate chondrules; Cleavage: None; Specific Gravity: 3.0-3.8
Formation & geological history
Formed in the early solar system approximately 4.5 billion years ago from solar nebula dust. These were parts of undifferentiated asteroids that fell to Earth through the atmosphere.
Uses & applications
Scientific research for solar system history, high-value collector items, and occasionally used in custom extraterrestrial jewelry.
Geological facts
Ordinary chondrites are the most common type of meteorite falling to Earth, accounting for about 85% of all falls. They contain the oldest solid materials in our solar system.
Field identification & locations
Identify by the presence of a fusion crust (a thin, burnt outer layer), regmaglypts (thumbprint-like indentations), and high magnetism. Found in deserts or Antarctica where they are easily spotted against the landscape.
