Science. 1980 Sep 26;209(4464):1512-4. doi: 10.1126/science.209.4464.1512.
Five carbynes (triply bonded allotropes of carbon) have been found by electron diffraction in the Allende and Murchison carbonaceous chondrites: carbon VI, VIII, X, XI, and (tentatively) XII. From the isotopic composition of the associated noble-gas components, it appears that the carbynes in Allende (C3V chondrite) are local condensates from the solar nebula, whereas at least two carbynes in Murchison (C2 chondrite) are of exotic, presolar origin. They may be dust grains that condensed in stellar envelopes and trapped isotopically anomalous matter from stellar nucleosynthesis.
在阿伦德和默奇森碳质球粒陨石中,通过电子衍射发现了五种碳炔(三重键合的碳同素异形体):碳 VI、VIII、X、XI 和(暂定)XII。根据伴生稀有气体成分的同位素组成,似乎阿伦德(C3V 球粒陨石)中的碳炔是太阳星云中的局部凝结物,而默奇森(C2 球粒陨石)中的至少两种碳炔则具有外来的、太阳前体的起源。它们可能是在恒星包层中凝结并捕获了恒星核合成中同位素异常物质的尘埃颗粒。