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

Published online by Cambridge University Press:  01 August 2006

Ulrich Ott  and
Peter Hoppe
Ulrich Ott
Affiliation:
Max-Planck-Institut für Chemie, Joh.-J.-Becherweg 27, D-55128 Mainz, Germany email: ott@mpch-mainz.mpg.de, hoppe@mpch-mainz.mpg.de
Peter Hoppe
Affiliation:
Max-Planck-Institut für Chemie, Joh.-J.-Becherweg 27, D-55128 Mainz, Germany email: ott@mpch-mainz.mpg.de, hoppe@mpch-mainz.mpg.de
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Abstract

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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.

Keywords

meteorsmeteoroidsstars: AGB and post-AGBsupernovae: generaldustextinctionISM: evolutionISM: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Highlights of Astronomy 14: Highlights of Astronomy , August 2006 , pp. 341 - 344
Copyright
Copyright © International Astronomical Union 2007

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