
meteorite
Chondrite Meteorite
Ordinary Chondrite (L, LL, or H type)
Hardness: 5-6 Mohs. Color: Dark brown to black fusion crust with lighter interior. Luster: Dull to sub-metallic. Structure: Contains small, spherical grains called chondrules. Specific gravity: 3.0-3.8. Highly magnetic due to iron-nickel content.
- Hardness
- 5-6 Mohs
- Color
- Dark brown to black fusion crust with lighter interior
- Luster
- Dull to sub-metallic
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Physical properties
Hardness: 5-6 Mohs. Color: Dark brown to black fusion crust with lighter interior. Luster: Dull to sub-metallic. Structure: Contains small, spherical grains called chondrules. Specific gravity: 3.0-3.8. Highly magnetic due to iron-nickel content.
Formation & geological history
Formed in the early solar nebula approximately 4.5 billion years ago. These are remnants of protoplanetary material that never incorporated into a larger planet.
Uses & applications
Scientific research into the origin of the solar system, private collection, and occasionally used as a source for unique jewelry.
Geological facts
Chondrites make up about 86% of all meteorites that fall to Earth. They are the oldest known rocks in the solar system, containing the original building blocks of planets.
Field identification & locations
Identified in the field by presence of a dark fusion crust (from atmospheric entry), attraction to magnets, and significantly higher density than typical Earth rocks. Found globally, especially in deserts or Antarctica.
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