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Volumn 312, Issue 5774, 2006, Pages 727-730

Interstellar chemistry recorded in organic matter from primitive meteorites

Author keywords

[No Author keywords available]

Indexed keywords

EXTRATERRESTRIAL ATMOSPHERES; HYDROGEN INORGANIC COMPOUNDS; ISOTOPES; MOLECULES; PLANETARY SURFACE ANALYSIS; SOLAR RADIATION;

EID: 33646444068     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1123878     Document Type: Article
Times cited : (329)

References (32)
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    • note
    • See supporting material on Science Online.
  • 19
    • 33646448650 scopus 로고    scopus 로고
    • note
    • 15N ∼2500‰) have been found in CB and CH chondrites [e.g., (29)]. However, the origin of these anomalies is unknown and their carriers may be secondary phases.
  • 22
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    • J. Bradley et al., Science 307, 244 (2005).
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  • 23
    • 33646447768 scopus 로고    scopus 로고
    • note
    • 13C = -113 ± 14‰), a composition closely similar to a putative interstellar C grain reported in an IDP (9). All other observed C anomalies originate from presolar SiC grains (15) embedded in the samples.
  • 31
    • 0032513360 scopus 로고    scopus 로고
    • R. Meier et ol., Science 279, 1707 (1998).
    • (1998) Science , vol.279 , pp. 1707
    • Meier, R.1
  • 32
    • 33646462815 scopus 로고    scopus 로고
    • note
    • Supported by grants from NASA's Cosmochemistry and Origins of the Solar System program (C.M.O'D.A., L.R.N.) and by the NASA Astrobiology Institute. We thank the NASA Meteorite Working Group for the Antarctic meteorites, M. Zolensky for providing the Tagish Lake sample, G. Cody for sample preparation assistance, E. Gröner for technical assistance with NanoSIMS, and two anonymous reviewers for their helpful constructive comments. A.F.Y. thanks B. Minarik for support through a NSF Research Experience for Undergraduates program at the Carnegie Institution of Washington.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.