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کندریت

File:NWA869Meteorite.jpg · Wikimedia Commons · See Wikimedia Commons

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کندریت

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Also known as chondrite meteorite

A chondrite (, ) is a stony (non-metallic) meteorite that has not been modified by either melting or differentiation of the parent body. They are formed when various types of dust and small grains in the early Solar System accreted to form primitive asteroids. Some such bodies that are captured in the planet's gravity well become the most common type of meteorite by arriving on a trajectory toward the planet's surface. Estimates for their contribution to the total meteorite population vary between 85.7% and 86.2%.

Key facts

Meteorite subdivision.Subdivision
Type
Meteorite subdivision.Name
Chondrite
Meteorite subdivision.Image
NWA869Meteorite.jpg
Meteorite subdivision.Image_caption
A specimen of the NWA 869 chondrite (type L4–6), showing chondrules and metal flakes
Meteorite subdivision.Compositional_type
Stony
Meteorite subdivision.Parent_body
Small to medium asteroids that were never part of a body large enough to undergo melting and planetary differentiation.
Meteorite subdivision.Petrologic_type
3–6
Meteorite subdivision.Number_of_specimens
Over 27,000

via Wikipedia infobox

Wikidata facts

Subclass of
stony meteorite
Image
Chondrite meteorite Mauerkirchen.jpg
Show 3 more facts
Commons category
Chondrite meteorites
topic's main category
Category:Chondrite meteorites
Sources (4)

via Wikidata · CC0

Gallery (20)