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Volumn 288, Issue 5471, 2000, Pages 1629-1631

Accretion of primitive planetesimals: Hf-W isotopic evidence from enstatite chondrites

Author keywords

[No Author keywords available]

Indexed keywords

ISOTOPE; TUNGSTEN;

EID: 0034595771     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.288.5471.1629     Document Type: Article
Times cited : (46)

References (33)
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    • note
    • All the samples were crushed with an aluminum oxide mortar under a laminar flow of high-efficiency particulate arresting (HEPA)-filtered air. Because of the very low W concentration in nonmetallic phases (mostly silicates and oxides), we treated all the nonmagnetic phases as a single fraction. Consequently, only three fractions-magnetic, bulk rock, and nonmagnetic-were analyzed, and the separation was performed with a hand magnet. Because abundant fine-grained silicates are intimately intergrown with the metal phases, mechanical separation is unable to provide a pure metallic fraction. Therefore, in addition to the bulk metal measurement some portions of the bulk metal separates from each sample were treated first with hot 6 M HCl to preferentially dissolve the metals. The solution was then decanted from the residue, and the residue was subsequently digested as another silicate/oxide-rich fraction with variable amounts of metal.
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    • note
    • We thank E, Hauri and K. Righter for their reviews; M. Johnson for technical assistance; R. Hewins, G. W. Lugmair, M. Prinz, B. Zanda, and G. J. Wasserburg for discussion; and M. Lindstrom, C. J. MacPherson, and M. Wadhwa for access to their meteorite collections at NASA, the Smithsonian Institution of Washington, and the Field Museum in Chicago. This work was supported by NSF and NASA.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.