Silica-bearing chondrules and clasts in ordinary chondrites

Details Silica-bearing chondrules and clasts in ordinary chondrites Silica-bearing chondrules and clasts in ordinary chondrites

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986gecoa..50.1655b&link_type=abstract

Geochimica et Cosmochimica Acta (ISSN 0016-7037), vol. 50, Aug. 1986, p. 1655-1666.

Computer Science

14

Chondrites, Chondrule, Meteoritic Composition, Mineralogy, Silicon Oxides, Electron Microscopy, Fayalite, Microstructure, Pyroxenes

Scientific paper

The solar system has comparable atomic abundances of Mg, Si, and Fe. Chondritic materials have approximately solar proportions of major elements; consequently, even if significant quantities of Fe are present as metal and sulfide phases, the resultant abundances dictate that olivine-normative materials will be formed. In this study the authors consider distinct occurrences of silica-bearing chondrules/clasts from a variety of unequilibrated ordinary chondrites.

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