The interstellar connection to solar system bodies

Computer Science – Emerging Technologies

Scientific paper

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Comets, Interstellar Matter, Meteoritic Composition, Solar System, Stellar Evolution, Astronomical Models, Comet Nuclei, Cosmic Dust, Interstellar Gas, Planetary Nebulae, Protoplanets, Solar System, Comets, Meteorites, Protoplanets, Origin, Formation, Nebula, Interplanetary Dust, Idps, Dust, Models, Comet Nuclei, Comae, Diagrams, Gases, Samples, Extraterrestrial, Laboratory Studies, Composition, Sampling

Scientific paper

Solar system bodies such as comets and meteorites are examined for interstellar signatures which may ultimately indicate what the protoplanetary nebula conditions were at the time the bodies formed. This involves retracing the sequence starting with a dense interstellar cloud, through the accretion disk phase of the protoplanetary nebula to the various steps in the aggregation process and finally to the physical and chemical metamorphic processes in the final body during the subsequent 4.55 billion years. Models of interstellar dust and comets which aid in such analysis are presented.

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