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Volumn 273, Issue 5276, 1996, Pages 757-762

Evidence for widespread 26Al in the solar nebula and constraints for nebula time scales

Author keywords

[No Author keywords available]

Indexed keywords

ALUMINUM; ALUMINUM 26; MAGNESIUM; MAGNESIUM 26; MAGNESIUM 28; UNCLASSIFIED DRUG;

EID: 0029663501     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.273.5276.757     Document Type: Article
Times cited : (207)

References (41)
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    • note
    • Samples were examined with a JEOL 840a scanning electron microscope at the Smithsonian Institution. Location maps were constructed from backscattered electron (BSE) photomosaics of entire thin sections. X-ray maps were made using a Fisons/Kevex Sigma energy-dispersive x-ray analysis system attached to the SEM.
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    • Mineral chemistry was analyzed using an ARL-SEMQ automated 9-spectrometer electron microprobe at the Smithsonian, operated at 15 kV accelerating potential and 0.15 μA beam current. Counting times were 40 seconds. Natural and synthetic crystalline materials were used as calibration standards. Data were corrected for matrix, absorption, and atomic number effects using a phi-rho-z program.
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    • note
    • The bulk composition of each chondrule was calculated by combining a point-count mode with analyzed mineral compositions and appropriate mineral densities. Area fraction is assumed to be equivalent to volume fraction.
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    • note
    • 24Mg of terrestrial standards as measured on the Caltech ion probe (36).
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    • note
    • 1-5) that encloses subordinate spinel (FeO up to 2%), blocky ∼2-4-μm-sized perovskite grains,
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    • T. D. Swindle, A. M. Davis, C. M. Hohenberg, G. J. MacPherson, L. E. Nyquist, in (28), p. 77
    • T. D. Swindle, A. M. Davis, C. M. Hohenberg, G. J. MacPherson, L. E. Nyquist, in (28), p. 77.
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    • thesis, California Institute of Technology
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    • note
    • We thank A. M. Davis and an anonymous reviewer for comments that significantly improved this paper. This research was supported by NASA grants NAGW 3553 (G.J.M.) and NACW 3297 (G.J.W.). This is Caltech contribution no. 5679 (934).


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.