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Trace Element Distribution Between Olivine and Kirschsteinite in Angra Dos Reis

Authors :
Fittipaldo, M. M
Jones, R. H
Shearer, C. K
Source :
Lunar and Planetary Science XXXIV.
Publication Year :
2003
Publisher :
United States: NASA Center for Aerospace Information (CASI), 2003.

Abstract

The angrites are a small and enigmatic group of basaltic achondrites that possess unique mineralogical and chemical properties. The dominant mineralogy of the seven angrite members (Angra dos Reis, LEW 86010, LEW 87051, Asuka 881371, Sahara 99555, D Orbigny, and a new Moroccan member) is fassaite, olivine, and plagioclase. Angrites display a wide range of thermal histories, with Angra dos Reis (AdoR) exhibiting a cooling history different from that of the rapidly cooled members and from LEW86010, a more slowly cooled member. AdoR could represent either a cumulate or a porphyritic igneous rock that was later altered by metamorphism. We are re-examining the thermal history of AdoR in light of the more recently described angrite members. Our emphasis is a trace element study of low-Ca olivine, which we refer to as olivine, and high-Ca olivine, which we refer to as kirschsteinite, in AdoR.

Details

Language :
English
Database :
NASA Technical Reports
Journal :
Lunar and Planetary Science XXXIV
Notes :
NAG5-9463
Publication Type :
Report
Accession number :
edsnas.20030111057
Document Type :
Report