Heterogeneous accretion, composition and core–mantle differentiation of the Earth

By D. Rubie, D. Frost, U. Mann, Y. Asahara, F. Nimmo, K. Tsuno, P. Kegler, A. Holzheid, H. Palme. 2011

431 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/c0c12a3c9b0f67dc1173b7f1cd9df362ca67611a

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

In Geophysics

Citations in the corpus

A hydrogen-based oxidation mechanism relevant to planetary formation (2013, background): “Both Earth and the Moon must have been below the IW buffer during their early history growth due to transient mixing between iron metal cores and silicate mantles during the Giant impact (Deguen et al., 2011; Frost et al., 2008; Jones and Palme, 2000; Rubie et al., 2011; Wood et al., 1990).”
Magma oceans in the inner solar system (2012, background): “Thus, chemical equilibration or disequilibrium processes between silicate and core metals likely occurred at several pressures and at several times during the growth of a terrestrial planet (Figure 1) (Rubie et al. 2011).”
Building Terrestrial Planets (2012, background): “Wood et al. (2008) and Rubie et al. (2011) showed that the oxidation state of Earth increased progressively as Earth was growing.”
Origins of building blocks of life: A review (2017, background): “It has been argued that, at the time of accretion and core formation of the Earth, the magma ocean on Earth could have been very reducing, with the oxygen fugacity being 2e4 log units below the IW buffer (Wood et al., 2006; Rubie et al., 2011; Scaillet and Gaillard, 2011).”
Accretion and differentiation of the terrestrial planets with implications for the compositions of early-formed Solar System bodies and accretion of water (2014, methodology): “By modeling the compositions of equilibrated metal and silicate for every impact event, we track and store the evolving mantle and core compositions of all embryos and proto-planets in the N-body simulation as accretion proceeds (Rubie et al. 2011).”