Chemical composition of HAL, an isotopically-unusual Allende inclusion

Details Chemical composition of HAL, an isotopically-unusual Allende inclusion Chemical composition of HAL, an isotopically-unusual Allende inclusion

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982gecoa..46.1627d&link_type=abstract

Geochimica et Cosmochimica Acta, vol. 46, Sept. 1982, p. 1627-1651. Research supported by the Alfred P. Sloan Research Foundati

Other

23

Chondrites, Isotopic Enrichment, Meteoritic Composition, Petrology, Rare Earth Elements, Trace Elements, Abundance, Barium, Cerium, Inclusions, Oxygen, Rims, Strontium, Uranium, Vanadium

Scientific paper

Samples of hibonite, black rim, and portions of friable rim from an unusual Allende inclusion, named HAL, were analyzed by INAA and RNAA for 37 major, minor, and trace elements. An unusually low amount of Ce was found in HAL, although it otherwise was highly enriched in REE compared to C1 chondrites. HAL is also depleted in Sr, Ba, U, V, Ru, Os, and Ir relative to other refractory elements. It is concluded that the distribution of REE between hibonite and rims was established when hibonite and other refractory minerals were removed at slightly different temperatures from a hot, oxidizing gas in which they previously coexisted as separate grains. Possible locations for the chemical and mass dependent isotopic fractionation are considered to be in ejecta from the low temperature helium-burning zone of a supernova and in the locally oxidizing environment generated by evaporation of interstellar grains of near-chondritic chemical composition.

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