The Solar System has a largely uniform isotopic composition but with tantalizing small variations. Geochemists are trying to ascertain the mechanisms and types of stars that produced this state of affairs.
This is a preview of subscription content
Access options
Subscribe to Journal
Get full journal access for 1 year
204,58 €
only 4,01 € per issue
Tax calculation will be finalised during checkout.
Buy article
Get time limited or full article access on ReadCube.
$32.00
All prices are NET prices.
References
Becker, H. & Walker, R. J. Nature 425, 152–155 (2003).
Suess, E. Rev. Astron. Astrophys. 3, 217–234 (1965).
Nittler, L. R. Earth Planet. Sci. Lett. 209, 259–273 (2003).
Nicolussi, G. K. et al. Astrophys. J. 504, 492–499 (1998).
Hartmann, L. Space Sci. Rev. 92, 55–68 (2000).
Weidenschilling, S. J. Mon. Not. R. Astron. Soc. 180, 57–70 (1977).
Lugmair, G. W. & Shukolyukov, A. Geochim. Cosmochim. Acta 62, 2863–2886 (1998).
Schönbächler, M. et al. Earth Planet. Sci. Lett. (in the press).
Yin, Q., Jacobsen, S. B. & Yamashiti, K. Nature 415, 881–883 (2002).
Dauphas, N., Marty, B. & Reisberg, L. Astrophys. J. 565, 640–644 (2001).
Author information
Affiliations
Rights and permissions
About this article
Cite this article
Halliday, A. Inside the cosmic blender. Nature 425, 137–139 (2003). https://doi.org/10.1038/425137a
Issue Date:
DOI: https://doi.org/10.1038/425137a