Harper C L, Nyquist L E, Bansal B, Wiesmann H, Shih C Y
Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA 02138.
Science. 1995 Jan 13;267(5195):213-7. doi: 10.1126/science.7809625.
Small differences in the ratio of neodymium-142 to neodymium-144 in early formed mantle reservoirs in planetary bodies are the result of in situ decay of the extinct radionuclide samarium-146 and can be used to constrain early planetary differentiation and therefore the time scale of planetary accretion. The martian meteorite Nakhla (approximately 1.3 billion years old), the type sample of the nakhlite subgroup of the Shergottite-Nakhlite-Chassigny (SNC) meteorites, exhibits a 59 +/- 13 parts per million excess in the ratio of neodymium-142 to neodymium-144 relative to normal neodymium. This anomaly records differentiation in the martian mantle before 4539 million years ago and implies that Mars experienced no giant impacts at any time later than 27 million years after the origin of the solar system.
行星天体早期形成的地幔储层中钕 - 142与钕 - 144的比例存在微小差异,这是灭绝放射性核素钐 - 146原位衰变的结果,可用于限制早期行星分化,进而确定行星吸积的时间尺度。火星陨石纳赫勒(约13亿年历史)是谢格特石 - 纳赫勒石 - 夏西尼陨石(SNC)中纳赫勒石亚群的典型样本,其钕 - 142与钕 - 144的比例相对于正常钕而言,有百万分之59±13的过剩。这一异常记录了45.39亿年前之前火星地幔的分化情况,意味着火星在太阳系起源后2700万年之后的任何时候都没有经历过巨大撞击。