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Chondrules in Meteorites

Abstract Chondrules are millimeter-scale rocky particles that occur as the dominant component in most chondrite meteorites. Chondrules formed within the first few million years of formation of the first solids in the solar system, 4,562–4,567 million years ago.
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Chondrules: Suggestion Concerning the Origin

Science, 1966
The millimeter-sized, sometimes glassy spheroids called chondrules that occur abundantly in stony meteorites may have been produced by lightning in the primitive Laplacian-type nebula while earthy materials were condensing and collecting to form the asteroids and the terrestrial planets.
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Chondrule

2011
Frank Sohl, Tilman Spohn
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In situ Si isotope and chemical constraints on formation and processing of chondrules in the Allende meteorite

Geochimica Et Cosmochimica Acta, 2021
Yogita Kadlag   +2 more
exaly  

Early evolution of the solar accretion disk inferred from Cr-Ti-O isotopes in individual chondrules

Earth and Planetary Science Letters, 2020
Yves Marrocchi   +2 more
exaly  

Compound chondrules

Geochimica et Cosmochimica Acta, 1995
John T. Wasson   +3 more
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