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Minor and trace element distribution in melilite and pyroxene from the Allende meteoriteMelilite and pyroxene were separated from a coarsely crystalline chondrule in the Allende meteorite and analyzed by microprobe and spark source mass spectrometer techniques. Elemental abundances in the bulk chondrule are consistent with a mixture of equal amounts of the two minerals, as observed microscopically. The lanthanide distributions are markedly different in the two minerals; relative to chondrite abundances, melilite shows progressive depletion of the lanthanides La-Sm, a positive Eu anomaly, and relatively constant abundances of the heavier lanthanides (Gd-Yb, and Y) whereas pyroxene shows progressive enrichment towards the heavier lanthanides, on which is superimposed a negative Eu anomaly. Both minerals, and the bulk chondrule, show unusual concentrations of the platinum metals, but the crystallographic site or sites of these metals remains to be determined.
Document ID
19740048210
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Mason, B.
(Smithsonian Institution Washington, D.C., United States)
Martin, P. M.
(Australian National University Canberra, Australia)
Date Acquired
August 7, 2013
Publication Date
May 1, 1974
Publication Information
Publication: Earth and Planetary Science Letters
Volume: 22
Issue: 2, Ma
Subject Category
Chemistry
Accession Number
74A30960
Funding Number(s)
CONTRACT_GRANT: NGR-09-015-170
Distribution Limits
Public
Copyright
Other

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