Broad bounds on Earth’s accretion and core formation constrained by geochemical models
By John Frederick Rudge, T. Kleine, B. Bourdon. 2010
194 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Geophysics, Paleontology
View Paper: https://www.semanticscholar.org/paper/01ea9a8a56d3b7c01d78a4afdf4105b73f99656f
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Citations in the corpus
- Heterogeneous accretion, composition and core–mantle differentiation of the Earth (2011, methodology): “…of the largest differentiated impactors only partially equilibrated with silicate liquid in magma oceans, which is in agreement with a recent fluid dynamics study (Dahl and Stevenson, 2010) and with Hf-W isotopic data (Halliday, 2004; Nimmo and Agnor, 2006; Nimmo et al., 2010; Rudge et al., 2010).”
- Evidence for Mo isotope fractionation in the solar nebula and during planetary differentiation (2014, methodology): “Data reduction of the data obtained on the Neptune was made off-line using the “double-spike toolbox” (Rudge et al., 2009), which employs MATLAB’s non-linear equation solving routine for the iteration. To ensure that both routines yielded consistent results, some of the Nu1700 data were reduced usin”
- Solidus and liquidus profiles of chondritic mantle: Implication for melting of the Earth across its history (2011, background): “It seems that the siderophile pattern of the mantle can be reproduced under non-equilibrium conditions assuming oxygen fugacity conditions higher than previously thought and embryos that have equilibrated at excessively hightemperatures (450 K above liquidus of chondritic mantle) (Rudge et al., 2010”
- The Non-carbonaceous–Carbonaceous Meteorite Dichotomy (2020, methodology): “W systematics of the BSE are compatible with a lower degree of core-mantle reequilibration (Nimmo et al. 2010; Rudge et al. 2010), and so the accretion of CC planetesimals to Earth would be consistent with the Hf–”
- Accretion and differentiation of the terrestrial planets with implications for the compositions of early-formed Solar System bodies and accretion of water (2014, background): “, 2011) and is of major importance for interpreting W isotopic anomalies in terms of the timing of planetary core formation (e.g. Nimmo and Agnor, 2006; Nimmo et al., 2010; Rudge et al., 2010).”