Coupled 142Nd–143Nd evidence for a protracted magma ocean in Mars
Author:
Publisher
Springer Science and Business Media LLC
Subject
Multidisciplinary
Link
http://www.nature.com/articles/nature06317.pdf
Reference32 articles.
1. Elkins-Tanton, L. T., Hess, P. C. & Parmentier, E. M. Possible formation of ancient crust on Mars through magma ocean processes. J. Geophys. Res. 110 E12S01 doi: 10.1029/2005JE002480 (2005)
2. Kiefer, W. S. Melting in the martian mantle: Shergottite formation and implications for present-day mantle convection on Mars. Meteorit. Planet. Sci. 38, 1815–1832 (2003)
3. Harper, C. L., Nyquist, L. E., Bansal, B., Wiesmann, H. & Shih, C.-Y. Rapid accretion and early differentiation of Mars indicated by 142Nd/144Nd in SNC meteorites. Science 267, 213–217 (1995)
4. Borg, L. E. & Draper, D. S. A petrogenetic model for the origin and compositional variation of the martian basaltic meteorites. Meteorit. Planet. Sci. 38, 1713–1731 (2003)
5. Foley, N. C. et al. The early differentiation history of Mars from 182W-142Nd isotope systematics in the SNC meteorites. Geochim. Cosmochim. Acta 69, 4557–4571 (2005)
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