
meteorite
Chondrite Meteorite
Ordinary Chondrite (L or H class)
Hardness: 4.5-5.5 (approximate), Color: Dark brown to black fusion crust with grey/mottled interior, Luster: Dull to metallic (if iron grains are visible), Crystal structure: Granular with chondrules (spherical grains), Specific Gravity: 3.0-3.8.
- Hardness
- 4
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Physical properties
Hardness: 4.5-5.5 (approximate), Color: Dark brown to black fusion crust with grey/mottled interior, Luster: Dull to metallic (if iron grains are visible), Crystal structure: Granular with chondrules (spherical grains), Specific Gravity: 3.0-3.8.
Formation & geological history
Formed from the solar nebula approximately 4.5 billion years ago, representing the primordial matter of the early solar system. These are fragments of asteroids that fall to Earth's surface.
Uses & applications
Scientific research into the origin of the solar system, private collection, and occasionally sliced for jewelry or pendants.
Geological facts
Chondrites are the most common type of meteorite, accounting for about 86% of all falls. They contain tiny round grains called chondrules, which were once molten droplets in space before the planets formed.
Field identification & locations
Identify by a dark 'fusion crust' formed during entry, smooth but irregular surface (regmaglypts), and magnetism due to iron content. Look for small circular chondrule patterns on broken or polished surfaces.
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