Early Earth evolution: new insight from Sm and Nd isotopes in meteoritic inclusions
Abstract:
On the basis of nucleosynthethic anomalies in Sm and Nd isotopes [4], the ordinary (O) and enstatite (E) chondrites remain potential candidates for the Earth’s building blocks. OC have an average deficit of -18±3 ppm relative to modern terrestrial 142Nd/144Nd, whereas EC range from the OC to the terrestrial values [4-6]. Sm stable isotope compositions of the analyzed CAIs indicate that galactic cosmic rays did not affect the 142Nd/144Nd compositions, but deficits are found in the pure p-process 144Sm nuclide (-240 to -290 ppm/ standard). These deficits may translate to 142Nd deficits of a few ppm. NWA 6991 CAI 146Sm-142Nd internal isochron passes through a 142Nd/144Nd ratio of -6 ±6 ppm relative to the terrestrial standard at a chondritic 147Sm/144Nd of 0.1960. We note that this value is identical to the enstatite chondrite average and the 142Nd/144Nd ratio of the lunar mantle, as defined recently by [7] using a chondritic Sm/Nd and Lu/Hf for the bulk Moon. While the determination of the Sm-Nd reference parameters for the bulk Earth is still contentious, the difference in 142Nd/144Nd between modern terrestrial rocks and meteorites analyzed so far is <10ppm.
[1] Bouvier and Wadhwa (2010) Nat. Geosc. 3, 637. [2] Boyet et al. (2010) Earth Planet. Sci. Lett. 291, 172. [3] Kinoshita et al. (2012) Science 335, 1614. [4] Carlson et al. (2007) Science 316, 1175. [5] Boyet and Carlson (2005) Science 309, 576. [6] Gannoun et al. (2011) Proc. Nat. Acad. Sc. 108, 7693. [7] Sprung et al. (2013) Earth Planet. Sci. Lett. 380, 77.
