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- W323725 abstract "Meteorites and interplanetary dust particles contain presolar stardust grains: solid samples of stars that can be studied in the laboratory. We review the role of these grains for the sciences of nucleosynthesis, stellar evolution, grain condensation, and chemical and dynamic evolution of the Galaxy. We explain what stardust is, prediscovery ideas about it, how it is collected and recognized, and how evidence of thermal condensation and measured isotopic abundance ratios places individual grains into related families. Unique scientific information derives primarily from the high precision ( in some cases 1%) of the measured isotopic ratios of large numbers of elements in single stardust grains. To clarify the new scientific scope, we focus on three of the stardust families: mainstream SiC grains from asymptotic giant branch carbon stars, oxide grains from oxygen-rich red giants, and carbide grains condensed within interiors of young expanding supernovae. Stardust science is just now reaching maturity and will remain an increasingly significant aspect of nucleosynthesis applications." @default.
- W323725 created "2016-06-24" @default.
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- W323725 date "2004-01-01" @default.
- W323725 modified "2023-09-27" @default.
- W323725 title "Presolar Stardust Grains" @default.
- W323725 hasPublicationYear "2004" @default.
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