Rock Identifier
Chondrite Meteorite (Ordinary Chondrite (S-type asteroid origin)) — igneous
igneous

Chondrite Meteorite

Ordinary Chondrite (S-type asteroid origin)

Hardness: 5-6 (Mohs); Color: Dark brown to black fusion crust with lighter interior; Luster: Dull or sub-metallic; Crystal structure: Contains spherical chondrules; Cleavage: None; Specific gravity: 3.0-3.8 (relatively heavy due to iron content).

Hardness
5-6 (Mohs)
Color
Dark brown to black fusion crust with lighter interior
Luster
Dull or sub-metallic
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Physical properties

Hardness: 5-6 (Mohs); Color: Dark brown to black fusion crust with lighter interior; Luster: Dull or sub-metallic; Crystal structure: Contains spherical chondrules; Cleavage: None; Specific gravity: 3.0-3.8 (relatively heavy due to iron content).

Formation & geological history

Formed through the accretion of dust and grit in the early solar system approximately 4.5 billion years ago. They are non-metallic asteroids that have not been modified by melting or differentiation of the parent body.

Uses & applications

Major scientific value for understanding the origin of the solar system; highly collectible by enthusiasts and museums.

Geological facts

Chondrites are the most common type of meteorite falling to Earth, accounting for about 86% of all falls. They contain the oldest solid materials known to exist in our solar system.

Field identification & locations

Identify in the field by checking for a thin, dark 'fusion crust,' attraction to a strong magnet (due to nickel-iron grains), and a weight that feels heavy for its size. Common locations include dry deserts or ice fields like Antarctica where they are easier to spot.

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