Science. 1971 May 21;172(3985):837-40. doi: 10.1126/science.172.3985.837.
The mass spectrum of xenon from spontaneous fission in a laboratory sample of plutonium-244 is precisely what meteoriticists predicted it would be; this discovery completes a web of proof that this nuclide is a bona fide extinct radioactivity of galactic origin, that r-process nucleosynthesis was ongoing in the galaxy at the time of the birth of the sun, and that the early meteoritic abundances of plutonium-244, heretofore tentative, can be utilized with confidence in models for the chronology of galactic nucleosynthesis. The search for an explanation for anomalous fission-like xenon in carbonaceous chondrites can now be narrowed.
实验室中钚-244 自发裂变产生的氙的质谱,与陨石学家所预测的完全吻合;这一发现完成了一系列证明,即这种核素是一种真正来自银河系的已灭绝放射性同位素,在太阳诞生时,银河系中正在进行 r 过程核合成,而此前暂定的早期陨石中钚-244 的丰度,可以在银河系核合成年代学模型中被自信地使用。现在,可以缩小对碳质球粒陨石中异常类裂变氙的解释的搜索范围。