Pre-solar grains in meteorites and interplanetary dust: an overview

Details Pre-solar grains in meteorites and interplanetary dust: an overview Pre-solar grains in meteorites and interplanetary dust: an overview

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007hia....14..341o&link_type=abstract

Highlights of Astronomy, Volume 14, p. 341-344

Astronomy and Astrophysics

Astronomy

Meteors, Meteoroids, Stars: Agb And Post-Agb, Supernovae: General, Dust, Extinction, Ism: Evolution, Ism: General

Scientific paper

Small amounts of pre-solar grains have survived in the matrices of primitive meteorites and interplanetary dust particles. Their detailed study in the laboratory with modern analytical tools provides highly accurate and detailed information with regard to stellar nucleosynthesis and evolution, grain formation in stellar atmospheres, and Galactic Chemical Evolution. Their survival puts constraints on conditions they were exposed to in the interstellar medium and in the Early Solar System.

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