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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
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
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
Accession Number
Distribution Limits
Work of the US Gov. Public Use Permitted.

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