Natural Variations in Comet-Aggregate Meteoroid Compositions

Mathematics – Logic

Scientific paper

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Aqueous Alteration, Ci Composition, Comet Nucleus, Comet Dust, Chemical Abundances, Differential Ablation, Interplanetary Dust Particles, Halley, Main Meteor Component, Meteoroids, Minerals, Leonids, Perseids, Solar Abundances, Wild 2

Scientific paper

Bulk compositions of aggregate meteoroids made of the originally accreted dust with its highly varied in mineral content and chemistry and considerable grain size variations do not have a chondritic bulk composition. Deviations from CI element abundances reflect indigenous variations within and among comet nuclei. These unmodified meteoroids that are heterogeneous in all their properties are fundamentally different from meteoroids with a CI bulk composition that are fine-grained, equigranular materials and chemically and mineralogically homogeneous. Collection and data reduction bias exists but the compositions of individual fast meteors are entirely constrained by the measured main component meteor abundances.

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