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Highly labile elementsCertain elements of high lability are very responsive to thermal processes, being either highly volatile during primary nebular condensation or highly mobile by postaccretionary metamorphic or shock heating. Data for highly labile elements indicate that different thermal processes were important in the genesis of each of the chondritic groups and a discussion of each is given. Contents of highly labile elements in a given group of contemporary falls differ from those of the same group that fell in Antarctica more than 0.1 Myr ago. This difference is due either to a time-dependent change in meteorite sources or, less likely, orbital variation of the meteorite flux to Earth.
Document ID
19890040126
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Lipschutz, Michael E.
(Purdue University West Lafayette, IN, United States)
Woolum, Dorothy S.
(California State University Fullerton, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1988
Subject Category
Lunar And Planetary Exploration
Accession Number
89A27497
Funding Number(s)
CONTRACT_GRANT: NAG9-48
CONTRACT_GRANT: NAG9-57
CONTRACT_GRANT: NSF DPP-84-15061
Distribution Limits
Public
Copyright
Other

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