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Title: Correlated morphological, chemical, and isotopic characteristics of hibonites from the Murchison carbonaceous chondrite

Journal Article · · Geochimica et Cosmochimica Acta; (USA)
 [1]
  1. Australian National Univ., Canberra (Australia)

Twenty-four hibonite-dominated refractory grains from the Murchison carbonaceous chondrite have been identified from polished grain-mounts of density separates, and have been morphologically and chemically divided into three groups: (1) 14 colorless PLAty Crystal fragments (PLACs) with less than 2.7% TiO{sub 2}; (2) 3 pleochroic Blue AGgregates (BAGs) which are composed of crystal plates and fragments and have TiO{sub 2} concentrations between 5.1% and 6.5%; (3) Six Spinel-HIBonite spherules and crystal aggregates (SHIBs), often with spinel, Fe-silicate, and clino-pyroxene rims. The maximum TiO{sub 2} concentrations of hibonite in the SHIBs ranges from 3.5 to 7.6%, but the TiO{sub 2} concentration in one grain was heterogeneous and ranged from 0.5% to 5.0%. Hibonite in all types is stoichiometric with Ti and Mg predominantly in a coupled substitution of Mg{sup 2+} and Ti{sup 4+} for 2Al{sup 3+}. One grain with a rounded hibonite core does not clearly fit into the three designated groups. The hibonites have been analyzed by ion microprobe mass spectrometry for their Mg and Ti isotopic compositions. The presence of hibonite populations with distinct morphological, chemical and Mg isotopic systematics suggests that there were several hibonite formation episodes within the early solar system. The hibonites probably formed by the melting of refractory dust aggregates during local transient thermal events.

OSTI ID:
5013954
Journal Information:
Geochimica et Cosmochimica Acta; (USA), Vol. 52:12; ISSN 0016-7037
Country of Publication:
United States
Language:
English

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