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Isotopic compositions of cometary matter returned by Stardust.

Authors :
McKeegan KD
Aléon J
Bradley J
Brownlee D
Busemann H
Butterworth A
Chaussidon M
Fallon S
Floss C
Gilmour J
Gounelle M
Graham G
Guan Y
Heck PR
Hoppe P
Hutcheon ID
Huth J
Ishii H
Ito M
Jacobsen SB
Kearsley A
Leshin LA
Liu MC
Lyon I
Marhas K
Marty B
Matrajt G
Meibom A
Messenger S
Mostefaoui S
Mukhopadhyay S
Nakamura-Messenger K
Nittler L
Palma R
Pepin RO
Papanastassiou DA
Robert F
Schlutter D
Snead CJ
Stadermann FJ
Stroud R
Tsou P
Westphal A
Young ED
Ziegler K
Zimmermann L
Zinner E
Source :
Science (New York, N.Y.) [Science] 2006 Dec 15; Vol. 314 (5806), pp. 1724-8.
Publication Year :
2006

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 (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.

Details

Language :
English
ISSN :
1095-9203
Volume :
314
Issue :
5806
Database :
MEDLINE
Journal :
Science (New York, N.Y.)
Publication Type :
Academic Journal
Accession number :
17170292
Full Text :
https://doi.org/10.1126/science.1135992