C, N, and noble gas isotopes in grain size separates of presolar diamonds from Efremovka

被引:68
作者
Verchovsky, AB
Fisenko, AV
Semjonova, LF
Wright, IP
Lee, MR
Pillinger, CT
机构
[1] Open Univ, Planetary Sci Res Inst, Milton Keynes MK7 6AA, Bucks, England
[2] Russian Acad Sci, VI Vernadskii Inst Geochem & Analyt Chem, Moscow 117975, Russia
[3] Univ Edinburgh, Dept Geol & Geophys, Edinburgh EH9 3JW, Midlothian, Scotland
关键词
D O I
10.1126/science.281.5380.1165
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Nanometer-size presolar diamonds from the Efremovka CV3 chondrite were physically separated into several grain size fractions by uttracentrifugation. The coarsest size fraction is the most enriched in carbon-12; the others have broadly similar carbon isotopic compositions. Measurement of noble gases shows that their concentration decreases with decreasing grain size. This effect is attributed to ion implantation, Such an episode could occur in the envelope of a supernova that produced the diamonds, or in interstellar space; in either case, ions with energies above a certain threshold pass completely through the smaller diamond grains without being captured. Concentrations of nitrogen show only minor variations with grain size, indicating a different mechanism of incorporation into the diamonds.
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页码:1165 / 1168
页数:6
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