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Implications for the evolution of chondrules from Agglomeratic olivine chondrulesThere is considerable evidence that chondrules formed by the melting of solid materials and, by default, the early solar nebula is the preferred location for chondrule formation. Agglomeratic olivine (AO) chondrules supply perhaps the most intriguing, direct evidence for chondrule formation from agglomeration of solids. We review the characteristics of AO chondrules and discuss their implications for understanding chondrule precursors and chondrule evolution.
Document ID
19950012920
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Weisberg, M. K.
(American Museum of Natural History New York, NY, United States)
Prinz, M.
(American Museum of Natural History New York, NY, 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
95N19335
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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