meteorite
Chondrite Meteorite
L or H Ordinary Chondrite
AI-generated identification · may be incorrectHardness: 5-6 (Mohs); Color: Rusty brown/ochre with metallic flecks; Luster: Dull/Sub-metallic; Crystal structure: Contains small spherical chondrules; Specific gravity: 3.0-3.8
- Hardness
- 5-6 (Mohs)
- Color
- Rusty brown/ochre with metallic flecks
- Luster
- Dull/Sub-metallic
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Physical properties
Hardness: 5-6 (Mohs); Color: Rusty brown/ochre with metallic flecks; Luster: Dull/Sub-metallic; Crystal structure: Contains small spherical chondrules; Specific gravity: 3.0-3.8
Formation & geological history
Formed in the early solar nebula approximately 4.5 billion years ago. These are remnants of protoplanetary materials that never merged into planets. This specimen shows a fusion crust and regmaglypts (thumbprint-like indentations) caused by atmospheric entry.
Uses & applications
Scientific research, hobbyist collecting, and metaphysical displays.
Geological facts
Ordinary chondrites make up about 85% of all meteorites that fall to Earth. They contain the oldest solid materials in the solar system.
Field identification & locations
Identify in the field by checking for high magnetic attraction, higher density than terrestrial rocks, and the presence of a fusion crust. Many are found in arid deserts or Antarctica where they are better preserved.
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