Macrochondrules in chondrites—Formation by melting of mega‐sized dust aggregates and/or by rapid collisions at high temperatures?
Open Access
- 3 October 2012
- journal article
- Published by Wiley in Meteoritics & Planetary Science
- Vol. 47 (12), 2237-2250
- https://doi.org/10.1111/j.1945-5100.2012.01403.x
Abstract
No abstract availableThis publication has 41 references indexed in Scilit:
- Ultrarapid chondrite formation by hot chondrule accretion? Evidence from unequilibrated ordinary chondritesMeteoritics & Planetary Science, 2012
- Late accretion and lithification of chondritic parent bodies: Mg isotope studies on fragments from primitive chondrites and chondritic brecciasMeteoritics & Planetary Science, 2007
- Evidence for the presence of planetesimal material among the precursors of magnesian chondrules of nebular originEarth and Planetary Science Letters, 2007
- Origin of SiO2-rich components in ordinary chondritesGeochimica et Cosmochimica Acta, 2006
- Young chondrules in CB chondrites from a giant impact in the early Solar SystemNature, 2005
- Chondrule and metal grain size sorting from jet flowsMeteoritics & Planetary Science, 2005
- Devgaon (H3) chondrite: Classification and complex cosmic ray exposure historyMeteoritics & Planetary Science, 2004
- Petrologic, geochemical and experimental constraints on models of chondrule formationEarth-Science Reviews, 2000
- Chemical and isotopic fractionation by grain size separatesEarth and Planetary Science Letters, 1980
- An exceptionally large chondrule in the Parnallee meteoriteMineralogical Magazine and Journal of the Mineralogical Society, 1967