School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA.
Science. 2010 Jan 22;327(5964):449-51. doi: 10.1126/science.1180871. Epub 2009 Dec 31.
The 238U/235U isotope ratio has long been considered invariant in meteoritic materials (equal to 137.88). This assumption is a cornerstone of the high-precision lead-lead dates that define the absolute age of the solar system. Calcium-aluminum-rich inclusions (CAIs) of the Allende meteorite display variable 238U/235U ratios, ranging between 137.409 +/- 0.039 and 137.885 +/- 0.009. This range implies substantial uncertainties in the ages that were previously determined by lead-lead dating of CAIs, which may be overestimated by several million years. The correlation of uranium isotope ratios with proxies for curium/uranium (that is, thorium/uranium and neodymium/uranium) provides strong evidence that the observed variations of 238U/235U in CAIs were produced by the decay of extant curium-247 to uranium-235 in the early solar system, with an initial 247Cm/235U ratio of approximately 1.1 x 10(-4) to 2.4 x 10(-4).
在陨石物质中,238U/235U 同位素比值长期以来被认为是不变的(等于 137.88)。这一假设是高精度铅铅定年的基石,铅铅定年定义了太阳系的绝对年龄。Allende 陨石中的钙铝富包体 (CAI) 显示出可变的 238U/235U 比值,范围在 137.409 +/- 0.039 和 137.885 +/- 0.009 之间。这一范围意味着先前通过 CAI 的铅铅定年确定的年龄存在很大的不确定性,这些年龄可能高估了几百万年。铀同位素比值与锔/铀(即钍/铀和钕/铀)的相关性提供了强有力的证据,表明 CAI 中观察到的 238U/235U 变化是由现存的锔-247 在早期太阳系中衰变为铀-235 产生的,初始 247Cm/235U 比值约为 1.1 x 10(-4) 到 2.4 x 10(-4)。