Rock Identifier
Chondrite Meteorite (Ordinary Chondrite (L or H group)) — igneous
igneous

Chondrite Meteorite

Ordinary Chondrite (L or H group)

Hardness: 5-6 Mohs. Color: Dark grey to brown exterior (fusion crust), grey interior with metallic flakes. Luster: Metallic flecks within a dull stony matrix. Structure: Contains chondrules (round grains) and nickel-iron grains. Specific Gravity: 3.0-3.8.

Hardness
5-6 Mohs
Luster
Metallic flecks within a dull stony matrix
Identified More igneous
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Physical properties

Hardness: 5-6 Mohs. Color: Dark grey to brown exterior (fusion crust), grey interior with metallic flakes. Luster: Metallic flecks within a dull stony matrix. Structure: Contains chondrules (round grains) and nickel-iron grains. Specific Gravity: 3.0-3.8.

Formation & geological history

Formed from the solar nebula approximately 4.5 billion years ago. These are primitive rocks that never underwent melting or differentiation within a planetary body.

Uses & applications

Scientific research into the origin of the solar system, private collection, and occasionally used in custom jewelry or decorative watches.

Geological facts

Chondrites are the most common type of meteorite falling to Earth, accounting for about 85% of all falls. They contain the oldest solid materials in the solar system.

Field identification & locations

Identify by the presence of a thin, dark fusion crust on the exterior and small, shiny metal flakes on a cut surface. Usually magnetic. Commonly found in deserts or Antarctica where they are easily spotted.