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Massive stars and short-lived radionuclides in the Solar System

Published online by Cambridge University Press:  16 November 2011

C. Charbonnel ,
T. Montmerle  and
M. Gounelle
M. Gounelle*
Affiliation:
Laboratoire de Minéralogie et de Cosmochimie du Muséum (LMCM), UMR 7202, MNHN & CNRS, 57 rue Cuvier, 75005 Paris, France
*
e-mail: [email protected]
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Abstract

Short-lived radionuclides (SLRs) are radioactive elements (T1/2 ≺ 200 Myr) which were present in the nascent solar system and are now extinct. While the initial abundance of SLRs with the longest half-lives (T1/2 ≻ 3 Myr) is compatible with the expectations of Galactic evolution models, others have a last-minute origin. 7Be, 10Be, 36Cl, and 41Ca probably originated within the protoplanetary disk from the irradiation of gas and dust by energetic particles accelerated by the protoSun. 26Al and 60Fe were probably synthesized by massive stars and added to interstellar gas which will eventually make up the bulk of our solar system. Identifying the detailed mechanisms of 26Al and 60Fe production and mixing will shed a light on the relationship between the Sun formation history and massive stars.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 51: Star Formation in the Local Universe – EES2010 , 2011 , pp. 289 - 297
Copyright
© EAS, EDP Sciences, 2011

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