igneous
Chondrite Meteorite
Ordinary Chondrite (L or H Type)
Hardness: 5-6 Mohs. Color: Dark brown to black fusion crust with a grayish interior. Luster: Sub-metallic to dull. Structure: Contains small spherical grains (chondrules). Density: High (3.0-3.8 g/cm3). Highly magnetic.
- Hardness
- 5-6 Mohs
- Color
- Dark brown to black fusion crust with a grayish interior
- Luster
- Sub-metallic to dull
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Physical properties
Hardness: 5-6 Mohs. Color: Dark brown to black fusion crust with a grayish interior. Luster: Sub-metallic to dull. Structure: Contains small spherical grains (chondrules). Density: High (3.0-3.8 g/cm3). Highly magnetic.
Formation & geological history
Formed or accreted in the early solar nebula approximately 4.5 billion years ago. These are remnants of planetesimals that never became part of a planet.
Uses & applications
Scientific research for understanding solar system history and high-end collector value. Large specimens are often used for display.
Geological facts
Chondrites make up approximately 86% of all meteorites that fall to Earth. They are among the oldest rocks in existence, pre-dating the formation of Earth's solid crust.
Field identification & locations
Check for a fusion crust (a thin, dark, glassy rind), magnetism, and high density. Professional testing for nickel content is required for confirmation. Common in desert environments like the Sahara or Antarctica.
