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The present understanding of the formation and evolution of the earliest bodies in the Solar System is based in large part on geochemical and isotopic evidences contained within meteorites.

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    Date Created
    2012
    Resource Type
  • Text
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    Note
    • Partial requirement for: Ph.D., Arizona State University, 2012
      Note type
      thesis
    • Includes bibliographical references (p. 211-225)
      Note type
      bibliography
    • Field of study: Geological sciences

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    by Matthew E. Sanborn

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