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Contact: Steve Koppes
s-koppes@uchicago.edu
773-702-8366
University of Chicago

Meteorite grains divulge Earth's cosmic roots

IMAGE: This is University of Chicago postdoctoral scientist Philipp Heck with a sample of the Allende meteorite. The dark portions of the meteorite contain dust grains that formed before the birth...

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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).

IMAGE: Philipp Heck with the Chicago Center for Cosmochemistry's time-of-flight mass spectrometer, which can reveal the chemical composition of minute experimental samples. Heck and his associates used a magnetic sector mass...

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"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.

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Citation: "Interstellar Residence Times of Presolar Dust Grains from the Murchison Carbonaceous Meteorite," Astrophysical Journal, June 20, 2009, Vol. 698, Issue 12, pages 1155-1164

Authors: Philipp R. Heck, University of Chicago Department of Geophysical Sciences and Chicago Center for Cosmochemistry

Frank Gyngard, Laboratory for Space Sciences and Physics Department, Washington University, St. Louis

Ulrich Ott, Max Planck Institute for Chemistry, Mainz, Germany

Matthias M.M. Meier, Institute of Isotope Geology and Mineral Resources, Zurich, Switzerland

Janaína N. Ávila, Research School of Earth Sciences and Planetary Science Institute, Australian National University, Canberra

Sachiko Amari, Laboratory for Space Sciences and Physics Department, Washington University, St. Louis

Ernest K. Zinner, Laboratory for Space Sciences and Physics Department, Washington University, St. Louis

Roy S. Lewis, Enrico Fermi Institute and the Chicago Center for Cosmochemistry, University of Chicago

Heinrich Baur, Institute of Isotope Geology and Mineral Resources, Zurich, Switzerland

Rainer Wieler, Institute of Isotope Geology and Mineral Resources, Zurich, Switzerland

Funding sources: 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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