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Chemical composition of the Howardite Parent Body deduced from Kapoeta primary 'mafic' magmasChemical data are presented for three 'mafic' clasts extracted from the Kapoeta howardite. Bulk compositions and petrologic observations suggest that two of these lithic clasts represent olivine-plagioclase bearing orthopyroxenites. Chondrite-relative refractory large ion lithophile abundances of two of the clasts are inferred to represent primary Mg-rich magmas produced by extensive (greater than about 70%) partial melting of a source composition indistinguishable from the silicate fraction of average CH-CL ordinary chondrites, with the exception of the depletion of the alkalis Na and K by a factor of 13 + or - 1 in the source composition. A metal-free and volatile depleted Kapoeta Parent Body (KPB) is subsequently deduced and is shown to compare very well with other similarly derived Achondrite Parent Body and Howardite Parent Body estimates but not to parent body estimates derived from inferences based on eucrite phase equilibrium studies. Other implications suggest that the KPB is heterogeneous with respect to Fe/Mg ratios.
Document ID
19830034140
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Smith, M. R.
(Oregon State Univ. Corvallis, OR, United States)
Schmitt, R. A.
(Oregon State University Corvallis, OR, United States)
Date Acquired
August 11, 2013
Publication Date
January 1, 1982
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: Houston, TX
Start Date: March 15, 1982
End Date: March 19, 1982
Accession Number
83A15358
Funding Number(s)
CONTRACT_GRANT: NGL-38-002-039
Distribution Limits
Public
Copyright
Other

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