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Volumn 274, Issue 5294, 1996, Pages 1876-1879

Hf-W isotopic evidence for rapid accretion and differentiation in the early solar system

Author keywords

[No Author keywords available]

Indexed keywords

IRON; METAL; RADIOISOTOPE; SILICATE; TUNGSTEN;

EID: 0030474925     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.274.5294.1876     Document Type: Article
Times cited : (136)

References (35)
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    • 180Os.
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    • 4.
  • 16
    • 12644290234 scopus 로고    scopus 로고
    • note
    • 184W ratio in the reservoir from which the metal was segregated would increase at a faster rate than the ratio in chondritic parent bodies. The main conclusion from our data is that these maximum time differences are short.
  • 17
  • 27
    • 0024258764 scopus 로고
    • J. F. Kerridge and M. S. Matthews, Eds. Univ. of Arizona Press, Tucson
    • T. D. Swindle and F. A. Podosek, in Meteorites and the Early Solar System, J. F. Kerridge and M. S. Matthews, Eds. (Univ. of Arizona Press, Tucson, 1988), pp. 1127-1146.
    • (1988) Meteorites and the Early Solar System , pp. 1127-1146
    • Swindle, T.D.1    Podosek, F.A.2
  • 35
    • 12644278287 scopus 로고    scopus 로고
    • note
    • We thank D. Peacor, E. J. Essene, R. Van der Voo, G. J. MacPherson, P. Pellas, and R. Hutchison for permission to access their meteorite collections. We also thank the reviewers for their comments, C. J. Allègre, C. Göpel, and M. W. Johnson for their assistance, and T. R. Ireland, R. J. Walker, and G. J. Wasserburg for discussion. This work was supported by NSF, DOE, NASA, and the University of Michigan.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.