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ShareJune 16, 2009 — The interstellar stuff that became incorporated into the planets and life on Earth has younger cosmic roots than theories predict, according to the University of Chicago postdoctoral scholar Philipp Heck and his international team of colleagues.
Heck and his colleagues examined 22 interstellar grains from the Murchison meteorite for their analysis. Dying sun-like stars flung the Murchison grains into space more than 4.5 billion years ago, before the birth of the solar system. Scientists know the grains formed outside the solar system because of their exotic composition.
"The concentration of neon, produced during cosmic-ray irradiation, allows us to determine the time a grain has spent in interstellar space," Heck said. His team determined that 17 of the grains spent somewhere between three million and 200 million years in interstellar space, far less than the theoretical estimates of approximately 500 million years. Only three grains met interstellar duration expectations (two grains yielded no reliable age).
"The knowledge of this lifetime is essential for an improved understanding of interstellar processes, and to better contain the timing of formation processes of the solar system," Heck said. A period of intense star formation that preceded the sun's birth may have produced large quantities of dust, thus accounting for the timing discrepancy, according to the research team.
Funding sources for the research include the National Aeronautics and Space Administration, Swiss National Science Foundation, the Australian National University, and the Brazilian National Council for Scientific and Technological Development.
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The above story is reprinted from materials provided by University of Chicago, via EurekAlert!, a service of AAAS.
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Journal Reference:
- Philipp R. Heck, Frank Gyngard, Ulrich Ott, Matthias M. M. Meier, Janaína N. Ávila, Sachiko Amari, Ernst K. Zinner, Roy S. Lewis, Heinrich Baur, and Rainer Wieler. Interstellar Residence Times of Presolar SiC Dust Grains from the Murchison Carbonaceous Meteorite. The Astrophysical Journal, 2009; 698 (2): 1155 DOI: 10.1088/0004-637X/698/2/1155
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