meteorite
Chondrite Meteorite
Stony Meteorite (Ordinary Chondrite)
Hardness: 5-6 (Mohs), Color: Dark brown to black fusion crust with grey/tan interior, Luster: Sub-metallic to dull, Structure: Contains small spherical chondrules, Cleavage: None, Specific Gravity: 3.0-3.8
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Physical properties
Hardness: 5-6 (Mohs), Color: Dark brown to black fusion crust with grey/tan interior, Luster: Sub-metallic to dull, Structure: Contains small spherical chondrules, Cleavage: None, Specific Gravity: 3.0-3.8
Formation & geological history
Formed from the solar nebula approximately 4.5 billion years ago. These are remnants of protoplanetary disks that never merged into planets, primarily originating from the asteroid belt.
Uses & applications
Scientific study of early solar system history, private collecting, and decorative display pieces.
Geological facts
Chondrites are the most common type of meteorite falling to Earth, accounting for about 86% of all falls. They contain the oldest solid materials in our solar system.
Field identification & locations
Identify by looking for a fusion crust (thin burnt outer layer), presence of metal flakes (attracts a magnet), and lack of vesicles (gas bubbles). Common in desert regions like the Sahara where they are easier to spot against the sand.
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