Computer Science
Scientific paper
Feb 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991gecoa..55..601m&link_type=abstract
Geochimica et Cosmochimica Acta (ISSN 0016-7037), vol. 55, Feb. 1991, p. 601-619.
Computer Science
25
Chemical Composition, Chondrites, Chondrule, Metamorphism (Geology), Olivine, Silicates, Concentration (Composition), Microstructure, Mineralogy, Planetary Evolution, Pyroxenes, Meteorites, Composition, Chondrules, Silicates, Ll3 Chondrites, Origin, Ll4 Chondrites, Ll5 Chondrites, Ll Chondrites, Chondrites, Parnellee, Stony Meteorites, Parent Bodies, Metamorphism, Semarkona, Petrology, Enrichment, Depletion, Iron, Manganese, Magnesium, Chromium, Calcium, Aluminum, Ordinary Chondrites, Formation, Samples, Me
Scientific paper
The composition of 75 type-IA and type-II porphyritic olivine chondrules from nine LL type 3 to type 5 chondrites was determined and was compared with that of chondrules from the Semarkona type 3.0 meteorite. Chemical data for silicates in the LL3.3-5 chondrites indicated that porphyritic olivine chondrules in these chondrites could be derived from chondrules similar to those from the Semarkona LL3.0, the least metamorphosed one of the known LL chondrites. It is shown that the chemical trends defined by the minerals of type-IA and type-II chondrules can be satisfactorily accounted for by the process of solid-state diffusive equilibration between minerals in chondrules and the opaque matrix rather than by changes in conditions during chondrule crystallization.
Jeffrey Taylor G.
Jones Rhian H.
Keil Klaus
McCoy Timothy James
Scott Edward R. D.
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