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Hibonite-bearing microspherules - A new type of refractory inclusions with large isotopic anomaliesThis paper presents petrographic description as well as results on the major- and trace-element chemistry and on Mg, Ca, and Ti isotopic compositions of three refractory inclusions, including 3413-1/31 inclusion from Lance and Murchison 7-228 and 7-753, the mineralogy of which is dominated by the oxide minerals spinel, hibonite, and perovskite. The microspherules examined seem to constitute a separate class of refractory inclusions, characterized by a distinct morphology and mineralogy; large excesses of Ca-48 and Ti-50, and Mg-26 depletions. It is suggested that this type of inclusions must have formed early, prior to the dilution of isotopic anomalies by mixing processes, and in an area characterized by excesses of Ca-48 and Ti-50, depletions of Mg-26, and a lack of Al-26.
Document ID
19910040103
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Ireland, T. R.
(Washington Univ. Saint Louis, MO, United States)
Fahey, A. J.
(Washington Univ. Saint Louis, MO, United States)
Zinner, E. K.
(Washington University Saint Louis, MO, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1991
Publication Information
Publication: Geochimica et Cosmochimica Acta
Volume: 55
ISSN: 0016-7037
Subject Category
Lunar And Planetary Exploration
Accession Number
91A24726
Funding Number(s)
CONTRACT_GRANT: NAG9-55
Distribution Limits
Public
Copyright
Other

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