Origin of fayalitic olivine rims and lath‐shaped matrix olivine in the CV3 chondrite Allende and its dark inclusions
- 1 January 1997
- journal article
- Published by Wiley in Meteoritics & Planetary Science
- Vol. 32 (1), 31-49
- https://doi.org/10.1111/j.1945-5100.1997.tb01238.x
Abstract
No abstract availableKeywords
This publication has 37 references indexed in Scilit:
- Correlated alteration effects in CM carbonaceous chondritesGeochimica et Cosmochimica Acta, 1996
- Interstellar water in meteorites?Geochimica et Cosmochimica Acta, 1995
- Origin of dark clasts in the Acfer 059/El Djouf 001 CR2 chondriteMeteoritics, 1994
- Oxygen Isotopes in MeteoritesAnnual Review of Earth and Planetary Sciences, 1993
- Matrix and fine-grained rims in the unequilibrated CO3 chondrite, ALHA77307: Origins and evidence for diverse, primitive nebular dust componentsGeochimica et Cosmochimica Acta, 1993
- Water and the thermal evolution of carbonaceous chondrite parent bodiesIcarus, 1989
- Origin of chondrule rims and interchondrule matrices in unequilibrated ordinary chondritesEarth and Planetary Science Letters, 1989
- Incompletely transformed serpentine-type phyllosilicates in the matrix of Antarctic CM chondritesGeochimica et Cosmochimica Acta, 1988
- Formation of ureilites by nebular processesGeochimica et Cosmochimica Acta, 1988
- The oxygen isotope record in Murchison and other carbonaceous chondritesEarth and Planetary Science Letters, 1984