Isotopic compositions of cometary matter returned by stardust

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. JacobsenAnton 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

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

331 Citations (Scopus)

Abstract

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 17O-enriched circumstellar stardust grain, silicate and oxide minerals have oxygen isotopic compositions consistent with solar system origin. One refractory grain is 16O-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.

Original languageEnglish
Pages (from-to)1724-1728
Number of pages5
JournalScience
Volume314
Issue number5806
DOIs
Publication statusPublished - 15 Dec 2006
Externally publishedYes

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