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Microchondrules in ordinary chondrites: Implications for chondrule formationThe occurrence of numerous microchondrules in several matrix-rich clasts and chondrule rims as described in this article has important implications for the origin of chondrules. It implies that fine-grained materials existed in the immediate vicinity of the microchondrules when they formed and that the chondrule-formation mechanism must have been highly localized. Microchondrules on OC have been reported in two principal settings: (1) as rare individuals in the fine-grained matrices of many type-3 chondrites and in the clastic matrix of the Dimmitt H regolith breccia; and (2) as the predominant or exclusive chondrule size in a few unequilibrated clasts in LL3.4 Piancaldoli, the Rio Negro L regolith breccia, L3.7 Mezo-Madaras, and LL3.1 Krymka.
Document ID
19950012894
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Krot, A. N.
(Hawaii Univ. Manoa, HI., United States)
Rubin, A. E.
(California Univ. Los Angeles, CA, United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1994
Publication Information
Publication: Lunar and Planetary Inst., Papers Presented to the Conference on Chondrules and the Protoplanetary Disk
Subject Category
Astrophysics
Accession Number
95N19309
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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