meteorite

Carbonaceous Chondrite (CV3 type)

Carbonaceous Chondrite (CV3 group)

AI-generated identification · may be incorrect

Hardness: 3-5 Mohs. Color: Dark gray to black matrix with white/tan inclusions. Luster: Dull to sub-metallic. Contains Chondrules (round grains) and CAIs (white Calcium-Aluminum-rich inclusions). Presence of organic compounds and water-bearing minerals.

Hardness: 3-5 Mohs
Color: Dark gray to black matrix with white/tan inclusions
Luster: Dull to sub-metallic

Identified July 4, 2026More meteorite →

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Physical properties

Formation & geological history

Formed in the early solar nebula approximately 4.56 billion years ago. These are some of the most primitive materials in the solar system, originating from undifferentiated asteroids that have remained largely unchanged since their formation.

Uses & applications

Scientific research into the origins of the solar system and life, high-end collector market, and educational museum displays.

Geological facts

The CV3 group is famously represented by the Allende meteorite, which fell in Mexico in 1969. It contains pre-solar grains that are older than the Sun itself.

Field identification & locations

Identify by a dark, charcoal-like appearance, a thin fusion crust if fresh, and the presence of small spherical chondrules when sliced. Usually found using metal detectors or visual surveys in arid desert regions like the Sahara or Antarctica.