Watching the Nasa sim, and others I've seen multiple times before, thought occurs that by re-liquifying much of the Earth after its initial formation, heavier elements which had otherwise been trapped in the crust / upper mantle might have re-mobilised and sunk deeper into the core.
I'm not sure of relative abundance of elements in the crusts of other rocky worlds, though at least generally Mars seems to have a greater prevalence of iron, and fewer of the lighter metals, in its own crust.
Arya Udry, Esteban Gazel, and Harry Y. McSween Jr., "Formation of Evolved Rocks at Gale Crater by Crystal Fractionation and Implications for Mars Crustal Composition", Journal of Geophysical Research: Planets 123 (2018), Issue 6, pp. 1525-1540. <https://doi.org/10.1029/2018JE005602>
Harry Y. McSween Jr.1,G. Jeffrey Taylor, and Michael B. Wyatt, "Elemental Composition of the Martian Crust", Science 324 (2009), Issue 5928, pp. 736-739. <https://science.sciencemag.org/content/324/5928/736>
(The fact that we now have geological studies of multiple specific regions of Mars delights me.)
I'm not sure of relative abundance of elements in the crusts of other rocky worlds, though at least generally Mars seems to have a greater prevalence of iron, and fewer of the lighter metals, in its own crust.
See: <https://earthscience.stackexchange.com/a/20711>
Citing:
Arya Udry, Esteban Gazel, and Harry Y. McSween Jr., "Formation of Evolved Rocks at Gale Crater by Crystal Fractionation and Implications for Mars Crustal Composition", Journal of Geophysical Research: Planets 123 (2018), Issue 6, pp. 1525-1540. <https://doi.org/10.1029/2018JE005602>
Harry Y. McSween Jr.1,G. Jeffrey Taylor, and Michael B. Wyatt, "Elemental Composition of the Martian Crust", Science 324 (2009), Issue 5928, pp. 736-739. <https://science.sciencemag.org/content/324/5928/736>
(The fact that we now have geological studies of multiple specific regions of Mars delights me.)