Verchovsky AB, Fisenko AV, Semjonova LF, Wright IP, Lee MR, Pillinger CT
A. B. Verchovsky, I. P. Wright, C. T. Pillinger, Planetary Sciences Research Institute, Open University, Walton Hall, Milton Keynes MK7 6AA, UK. A. V. Fisenko and L. F. Semjonova, Vernadsky Institute of Geochemistry and Analytical Chemistry, Russian.
Science. 1998 Aug 21;281(5380):1165-8.
Nanometer-size presolar diamonds from the Efremovka CV3 chondrite were physically separated into several grain size fractions by ultracentrifugation. 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.
通过超速离心法,将来自叶夫列莫夫卡CV3球粒陨石的纳米级前太阳钻石按物理方法分离成几个粒度级分。最粗的粒度级分中碳-12的富集程度最高;其他级分的碳同位素组成大致相似。对惰性气体的测量表明,其浓度随粒度减小而降低。这种效应归因于离子注入。这样的事件可能发生在产生钻石的超新星包层中,也可能发生在星际空间中;在任何一种情况下,能量高于某个阈值的离子都会完全穿过较小的钻石颗粒而不被捕获。氮的浓度随粒度变化很小,这表明氮进入钻石的机制不同。