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PubMed · 11543337

Tracking the organic refractory component from interstellar dust to comets.

J M Greenberg·A Li
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Abstract

The abundance and composition of complex organic (carbonaceous) material in the interstellar dust is followed as the dust evolves in its cyclic evolution between diffuse and dense clouds. Interstellar extinction, laboratory and space analog experiments, dust infrared absorption spectra, the cosmic abundance of the condensible atoms, and space and ground-based observations of comet dust are used to impose constraints on the organic dust component as mantles on silicate cores.

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CarbonCarbonatesCosmic DustExobiologyExtraterrestrial EnvironmentHydrocarbonsIceMeteoroidsOrganic ChemicalsPolycyclic Aromatic HydrocarbonsSilicatesSpectrum AnalysisJournal ArticleResearch Support, Non-U.S. Gov't

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J M Greenberg, A Li. 1999. Tracking the organic refractory component from interstellar dust to comets.. https://doi.org/10.1016/s0273-1177(99)00091-5

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