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Volatiles in fourteen interplanetary dust particles: A comparison with CI and CM chondritesIn an attempt to classify the nature of volatiles within interplanetary dust particles (IDP's), 14 IDP's using a laser microprobe/mass spectrometer (LM/MS) technique were studied. Volatile abundances and distributions found for the IDP's are compared with those measured for carbonaceous chondrites in order to determine if the IDP's are related to the parent bodies of these primitive meteorites.
Document ID
19940007660
Document Type
Conference Paper
Authors
Bustin, R. (Arkansas Coll. Batesville, AR, United States)
Gibson, E. K., Jr. (NASA Lyndon B. Johnson Space Center Houston, TX., United States)
Wentworth, S. J. (NASA Lyndon B. Johnson Space Center Houston, TX., United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1993
Publication Information
Publication: Lunar and Planetary Inst., Twenty-fourth Lunar and Planetary Science Conference. Part 1: A-F
Subject Category
ASTROPHYSICS
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19940007055Analytic PrimarySixth Annual Workshop on Space Operations Applications and Research (SOAR 1992), volume 219940007543Analytic PrimaryTwenty-fourth Lunar and Planetary Science Conference. Part 1: A-F