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A refractory inclusion in the Kaba CV3 chondrite - Some implications for the origin of spinel-rich objects in chondritesThe first detailed petrographic and mineralogical study of a Ca, Al-rich inclusion (CAI) from the Kaba CV3 chondrite is reported. This 'fine-grained' CAI contains abundant small, rounded, rimmed, spinel-rich objects which have important features in common with the spinel-rich objects in other carbonaceous and ordinary chondrites. These nodules are interpreted as fractionated distillation residues of primitive dust. However, the available data do not unambiguously rule out a condensation origin for at least some of these objects. Finally, the preservation of distinct diopside-hedenbergite rims on the spinel-rich bodies and the small grain size of many minerals in the CAI matrix material both suggest that the CAI accreted cool and had a relatively cool thermal history in the Kaba parent body.
Document ID
19860034124
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Fegley, B., Jr.
(MIT Cambridge, MA, United States)
Post, J. E.
(Harvard University Cambridge, MA, United States)
Date Acquired
August 12, 2013
Publication Date
November 1, 1985
Publication Information
Publication: Earth and Planetary Science Letters
Volume: 75
Issue: 4
ISSN: 0012-821X
Subject Category
Lunar And Planetary Exploration
Accession Number
86A18862
Funding Number(s)
CONTRACT_GRANT: NSF EAR-79-2005
CONTRACT_GRANT: NSF ATM-84-01232
Distribution Limits
Public
Copyright
Other

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