Trace element content of chondritic cosmic dust: Volatile enrichments, thermal alterations, and the possibility of contamination

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Atmospheric Entry, Atmospheric Heating, Chemical Composition, Interplanetary Dust, Trace Elements, Abundance, Chondrites, Contamination, Temperature Effects, X Ray Fluorescence

Scientific paper

Trace element abundances in 51 chondritic Interplanetary Dust Particles (IDP's) were measured by Synchrotron X-Ray Fluorescence (SXRF). The data allow us to determine an average composition of chondritic IDP's and to examine the questions of volatile loss during the heating pulse experienced on atmospheric entry and possible element addition due to contamination during atmospheric entry, stratospheric residence, and curation.

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