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ON TYPE III PLESSITE IN CHONDRITES

 

作者: Reed Knox,  

 

期刊: Meteoritics  (WILEY Available online 1980)
卷期: Volume 15, issue 1  

页码: 25-29

 

ISSN:0026-1114

 

年代: 1980

 

DOI:10.1111/j.1945-5100.1980.tb00170.x

 

出版商: Blackwell Publishing Ltd

 

数据来源: WILEY

 

摘要:

Questions are raised concerning the possible sources of heat necessary for converting martensite to coarse Type III plessite in ordinary chondrites.It is suggested that the unusual Type III plessite in the Kingfisher, Oklahoma black chondrite was formed by partial homogenization of preexisting Type III plessite as a result of shock reheating of the metal into the γ field of the Fe‐Ni phase diagram, rather than by decomposition of shock reheated prior martensite in the α + γ field, as originally proposed by Taylor and Heymann.Because martensite is sporadically distributed within Kingfisher plessite it is suggested that microstructures of this kind be called Type II‐III pl

 

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