Isotopic compositions of cometary matter returned by Stardust.

نویسندگان

  • Kevin D McKeegan
  • Jerome Aléon
  • John Bradley
  • Donald Brownlee
  • Henner Busemann
  • Anna Butterworth
  • Marc Chaussidon
  • Stewart Fallon
  • Christine Floss
  • Jamie Gilmour
  • Matthieu Gounelle
  • Giles Graham
  • Yunbin Guan
  • Philipp R Heck
  • Peter Hoppe
  • Ian D Hutcheon
  • Joachim Huth
  • Hope Ishii
  • Motoo Ito
  • Stein B Jacobsen
  • Anton Kearsley
  • Laurie A Leshin
  • Ming-Chang Liu
  • Ian Lyon
  • Kuljeet Marhas
  • Bernard Marty
  • Graciela Matrajt
  • Anders Meibom
  • Scott Messenger
  • Smail Mostefaoui
  • Sujoy Mukhopadhyay
  • Keiko Nakamura-Messenger
  • Larry Nittler
  • Russ Palma
  • Robert O Pepin
  • Dimitri A Papanastassiou
  • François Robert
  • Dennis Schlutter
  • Christopher J Snead
  • Frank J Stadermann
  • Rhonda Stroud
  • Peter Tsou
  • Andrew Westphal
  • Edward D Young
  • Karen Ziegler
  • Laurent Zimmermann
  • Ernst Zinner
چکیده

Hydrogen, carbon, nitrogen, and oxygen isotopic compositions are heterogeneous among comet 81P/Wild 2 particle fragments; however, extreme isotopic anomalies are rare, indicating that the comet is not a pristine aggregate of presolar materials. Nonterrestrial nitrogen and neon isotope ratios suggest that indigenous organic matter and highly volatile materials were successfully collected. Except for a single (17)O-enriched circumstellar stardust grain, silicate and oxide minerals have oxygen isotopic compositions consistent with solar system origin. One refractory grain is (16)O-enriched, like refractory inclusions in meteorites, suggesting that Wild 2 contains material formed at high temperature in the inner solar system and transported to the Kuiper belt before comet accretion.

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عنوان ژورنال:
  • Science

دوره 314 5806  شماره 

صفحات  -

تاریخ انتشار 2006