meteorite

Chondrite Meteorite

L or H Ordinary Chondrite

AI-generated identification · may be incorrect

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

Hardness: 5-6 (Mohs)
Color: Rusty brown/ochre with metallic flecks
Luster: Dull/Sub-metallic

Identified July 3, 2026More meteorite →

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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.