Volatiles in fourteen interplanetary dust particles: A comparison with CI and CM chondrites

Details Volatiles in fourteen interplanetary dust particles: A comparison with CI and CM chondrites Volatiles in fourteen interplanetary dust particles: A comparison with CI and CM chondrites

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993lpi....24..239b&link_type=abstract

In Lunar and Planetary Inst., Twenty-fourth Lunar and Planetary Science Conference. Part 1: A-F p 239-240 (SEE N94-12015 01-91)

Computer Science

Abundance, Carbonaceous Chondrites, Interplanetary Dust, Meteoritic Composition, Mass Spectrometers, Volatility

Scientific paper

In 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.

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