
meteorite
Chondrite Meteorite
Ordinary Chondrite (Undifferentiated Meteorite)
Hardness: 5-6 (Mohs); Color: Dark brown to black fusion crust, grayish interior; Luster: Dull to metallic (if iron grains present); Crystal structure: Contains spherical chondrules; Specific Gravity: 3.0-3.8.
- Hardness
- 5-6 (Mohs)
- Color
- Dark brown to black fusion crust, grayish interior
- Luster
- Dull to metallic (if iron grains present)
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Physical properties
Hardness: 5-6 (Mohs); Color: Dark brown to black fusion crust, grayish interior; Luster: Dull to metallic (if iron grains present); Crystal structure: Contains spherical chondrules; Specific Gravity: 3.0-3.8.
Formation & geological history
Formed from the solar nebula over 4.5 billion years ago. These are fragments of asteroids that never underwent melting or differentiation. They represent the oldest solid material in our solar system.
Uses & applications
Scientific research, educational specimens, and highly sought-after by private collectors of space artifacts.
Geological facts
Chondrites represent about 86% of all meteorites that fall to Earth. They are called chondrites because they contain chondrules, which are small mineral beads that formed in space before the planets existed.
Field identification & locations
Identify by checking for a magnetic response (most contain nickel-iron), high density for their size, and a thin, dark fusion crust. Often found in arid deserts or Antarctica where they are easily spotted against the ground.
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Chondrite Meteorite
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