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Ancient Stardust in the Laboratory

DEC 01, 1997
As it collapsed to form the Solar System, material in the solar nebula was churned up and homogenized. But not everything was lost in the mix …
Thomas J. Bernatowicz
Robert M. Walker

A mazingly, individual grains of dust from stars that existed before the Sun was born have made their way to Earth in meteorites. When subjected to a battery of cutting‐edge laboratory techniques, these tiny grains provide thrilling new insights into such topics as the dynamics of supernova explosions, the age and chemical evolution of the Galaxy, fundamental nuclear physics and processes in the outer envelopes of stars. The path from dust grain to astrophysical insight is the subject of this article.

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References

  1. 1. For a recent account of the history and status of nucleosynthesis theory, see D. Arnett, Supernovae and Nucleosynthesis, Princeton U.P., Princeton, N.J. (1996).

  2. 2. A detailed account of this new field can be found in Astrophysical Implications of the Laboratory Study of Presolar Materials, T. Bernatowicz, E. Zinner, eds., AIP Conf. Proc. 402, AIP Press, Woodbury, N.Y. (1997).

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More about the authors

Thomas J. Bernatowicz, Washington University, St. Louis, Missouri.

Robert M. Walker, Washington University.

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This Content Appeared In
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Volume 50, Number 12

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