Kunz J, Staudacher T, Allegre CJ
J. Kunz, Institut de Physique du Globe de Paris, Laboratoire de Geochimie et Cosmochimie, Centre National de la Recherche Scientifique URA 1758, 4 place Jussieu, F-75252 Paris Cedex 05, France. T. Staudacher, Institut de Physique du.
Science. 1998 May 8;280(5365):877-80. doi: 10.1126/science.280.5365.877.
Data from mid-ocean ridge basalt glasses indicate that the short-lived radionuclide plutonium-244 that was present during an early stage of the development of the solar system is responsible for roughly 30 percent of the fissiogenic xenon excesses in the interior of Earth today. The rest of the fissiogenic xenon can be ascribed to the spontaneous fission of still live uranium-238. This result, in combination with the refined determination of xenon-129 excesses from extinct iodine-129, implies that the accretion of Earth was finished roughly 50 million to 70 million years after solar system formation and that the atmosphere was formed by mantle degassing.
来自大洋中脊玄武岩玻璃的数据表明,在太阳系形成早期存在的短寿命放射性核素钚-244,是如今地球内部裂变成因氙过量的大约30%的来源。其余的裂变成因氙可归因于仍具放射性的铀-238的自发裂变。这一结果,结合对来自已灭绝碘-129的氙-129过量的精确测定,意味着地球的吸积在太阳系形成后约5000万至7000万年时完成,且大气是由地幔脱气形成的。