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Mineralogy and Petrology of Yamato 86029: A New Type of Carbonaceous ChondriteY-86029 resembles CI chondrites. Its matrix is very fine-grained. Olivine shows evidence of shock, which has rarely been observed in carbonaceous chondrites. Y-86029 experienced aqueous and thermal alteration during or after accretion in parent body. Additional information is contained in the original extended abstract.
Document ID
20010045199
Document Type
Conference Paper
Authors
Tonui, E. (NASA Johnson Space Center Houston, TX United States)
Zolensky, M. E. (NASA Johnson Space Center Houston, TX United States)
Date Acquired
August 20, 2013
Publication Date
January 1, 2001
Publication Information
Publication: Lunar and Planetary Science XXXII
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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