Unique Meteorite from Early Amazonian Mars: Water-Rich Basaltic Breccia Northwest Africa 7034

  • Carl B. Agee
    Institute of Meteoritics, University of New Mexico, Albuquerque, NM 87131, USA.
  • Nicole V. Wilson
    Institute of Meteoritics, University of New Mexico, Albuquerque, NM 87131, USA.
  • Francis M. McCubbin
    Institute of Meteoritics, University of New Mexico, Albuquerque, NM 87131, USA.
  • Karen Ziegler
    Institute of Meteoritics, University of New Mexico, Albuquerque, NM 87131, USA.
  • Victor J. Polyak
    Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, NM 87131, USA.
  • Zachary D. Sharp
    Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, NM 87131, USA.
  • Yemane Asmerom
    Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, NM 87131, USA.
  • Morgan H. Nunn
    Department of Chemistry and Biochemistry, University of California, San Diego, La Jolla, CA 92093, USA.
  • Robina Shaheen
    Department of Chemistry and Biochemistry, University of California, San Diego, La Jolla, CA 92093, USA.
  • Mark H. Thiemens
    Department of Chemistry and Biochemistry, University of California, San Diego, La Jolla, CA 92093, USA.
  • Andrew Steele
    Geophysical Lab, Carnegie Institution of Washington, Washington, DC 20005, USA.
  • Marilyn L. Fogel
    Geophysical Lab, Carnegie Institution of Washington, Washington, DC 20005, USA.
  • Roxane Bowden
    Geophysical Lab, Carnegie Institution of Washington, Washington, DC 20005, USA.
  • Mihaela Glamoclija
    Geophysical Lab, Carnegie Institution of Washington, Washington, DC 20005, USA.
  • Zhisheng Zhang
    Department of Chemistry and Biochemistry, University of California, San Diego, La Jolla, CA 92093, USA.
  • Stephen M. Elardo
    Institute of Meteoritics, University of New Mexico, Albuquerque, NM 87131, USA.

書誌事項

公開日
2013-02-15
DOI
  • 10.1126/science.1228858
公開者
American Association for the Advancement of Science (AAAS)

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説明

<jats:title>So Different and So Similar</jats:title> <jats:p> Most known meteorites from Mars fit into one class. <jats:bold> Agee <jats:italic>et al.</jats:italic> </jats:bold> (p. <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6121" page="780" related-article-type="in-this-issue" vol="339" xlink:href="10.1126/science.1228858">780</jats:related-article> , published online 3 January; see the Perspective by <jats:bold> <jats:related-article xmlns:xlink="http://www.w3.org/1999/xlink" ext-link-type="doi" issue="6121" page="771" related-article-type="in-this-issue" vol="339" xlink:href="10.1126/science.1232490">Humayun</jats:related-article> </jats:bold> ) describe a meteorite, NWA 7034, which shares some characteristics with other martian meteorites but does not fit within the usual classification. NWA 7034 matches the composition of Mars' surface but is also richer in water than other martian meteorites, and has different oxygen isotope composition, which suggests the existence of multiple oxygen isotopic reservoirs within Mars. Its radiometric age of 2.1 billion years makes it a unique sample of the Amazonian period on Mars. </jats:p>

収録刊行物

  • Science

    Science 339 (6121), 780-785, 2013-02-15

    American Association for the Advancement of Science (AAAS)

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