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Volumn 284, Issue 5418, 1999, Pages 1348-1350

26Al in eucrite Piplia Kalan: Plausible heat source and formation chronology

Author keywords

[No Author keywords available]

Indexed keywords

ALUMINUM; MAGNESIUM;

EID: 0033591322     PISSN: 00368075     EISSN: None     Source Type: Journal    
DOI: 10.1126/science.284.5418.1348     Document Type: Article
Times cited : (139)

References (44)
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    • The sample was photo-documented with a JEOL scanning electron microscope at Washington University, St. Louis. Back-scattered electron image (BSE) photo-mosaics were created to be used as location maps and guides for ion probe isotopic analyses. Mineral chemistry was determined with a Cameca Camebax electron microprobe at Johnson Space Center, Houston, TX, operating at 15-kV accelerating potential and 40-nA beam current with counting time of 20 s for Al, Ca, Mn, and Fe and 40 s for Si, Ti, V, Cr, and Mg. Natural and synthetic crystalline standards were used for calibration.
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    • We thank V. K. Vaya and M. S. Sisodia of J.N.V. University, Jodhpur, for participating in the expedition for search of the Piplia Kalan meteorite fragments used in this study. We thank A. Shukla for help at various stages of this work. The assistance provided by P. Swan (Washington University, St. Louis) for photodocumentation of the section and V. Yang (Johnson Space Center, Houston) for electron microprobe analyses is appreciated. Comments from two referees helped to improve the quality of the paper.


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