igneous
Chondrite Meteorite
L or H Ordinary Chondrite
Hardness: 5-6 Mohs. Color: Rusty brown fusion crust with a grey/silvery interior containing metallic flecks. Luster: Dull/earthy exterior, metallic interior. Structure: Granular with visible chondrules. SG: 3.0-3.8.
- Hardness
- 5-6 Mohs
- Luster
- Dull/earthy exterior, metallic interior
Identified More igneous →
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Physical properties
Hardness: 5-6 Mohs. Color: Rusty brown fusion crust with a grey/silvery interior containing metallic flecks. Luster: Dull/earthy exterior, metallic interior. Structure: Granular with visible chondrules. SG: 3.0-3.8.
Formation & geological history
Formed through the accretion of dust and granules (chondrules) in the early solar nebula approximately 4.5 billion years ago. These are primitive rocks that never underwent melting in a planetary body.
Uses & applications
Primarily used for scientific research into the early solar system, high-end private collecting, and occasionally used in unique jewelry pieces.
Geological facts
Ordinary chondrites are the most common type of meteorite falling to Earth, accounting for about 85% of all falls. They contain the oldest solid matter in the solar system.
Field identification & locations
Identify in the field by their high density, attraction to strong magnets (due to iron-nickel content), and the presence of a thin, dark fusion crust. Found globally, especially in deserts and Antarctica.
