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
Identified More igneous →
Explore Chondrite Meteorite in the encyclopedia →Identify your own rocks.
Get a report just like this from any photo, free.
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.
