Publication Date:
1998-10-17
Description:
Ultraviolet laser microprobe analyses of a calcium-aluminum-rich inclusion (CAI) from the Allende meteorite suggest that a line with a slope of exactly 1.00 on a plot of delta17O against delta18O represents the primitive oxygen isotope reservoir of the early solar nebula. Most meteorites are enriched in 17O and 18O relative to this line, and their oxygen isotope ratios can be explained by mass fractionation or isotope exchange initiating from the primitive reservoir. These data establish a link between the oxygen isotopic composition of the abundant ordinary chondrites and the primitive 16O-rich component of CAIs.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Young -- Russell -- New York, N.Y. -- Science. 1998 Oct 16;282(5388):452-5.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉E. D. Young, Department of Earth Sciences, University of Oxford, Parks Road, Oxford, OX1 3PR, UK. E-mail: ed.young@earth.ox.ac.uk S. S. Russell, Department of Mineralogy, Natural History Museum, Cromwell Road, London SW7 5BD, UK. E-mail: sar.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/9774267" target="_blank"〉PubMed〈/a〉
Print ISSN:
0036-8075
Electronic ISSN:
1095-9203
Topics:
Biology
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Chemistry and Pharmacology
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Computer Science
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Medicine
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Natural Sciences in General
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Physics
