Cosmochemical Estimates of Mantle Composition

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The composition of Mars (2019, methodology): “, 2008b) is used to constrain compositional models of the Earth by accepting these chondritic refractory element ratios (McDonough and Sun, 1995; Palme and O’Neill, 2014).”
The Nitrogen Budget of Earth (2015, background): “The Bulk Earth (BE) has 280 ppm K (Arevalo et al., 2009) and 0.6 ppm Rb (Palme and O'Neill, 2014).”
A reference Earth model for the heat‐producing elements and associated geoneutrino flux (2013, background): “…ng/g [ Javoy et al ., 2010; O ’ Neill and Palme , 2008], ~20 ng/g [ Allègre et al ., 1995; Hart and Zindler , 1986; Lyubetskaya and Korenaga , 2007a; 2007b; McDonough and Sun , 1995; Palme and O ’ Neill , 2003], and ~30 ng/g [ Anderson , 2007; Turcotte and Schubert , 2002; Turcotte et al ., 2001]).”
The Compositional Structure of the Asteroid Belt (2015, background): “No meteorite group or combination of groups can reproduce both the elemental and isotopic compositions of the Earth, the planet for which we have the best data (Palme and O'Neill, 2014; Halliday, 2014: Appendix Question D1).”
The condensation temperatures of the elements: A reappraisal (2019, background): “…1 shows the abundances of a large number of elements in the BSE, expressed relative to abundances in CI chondrites, (and normalized to Mg of 1.0) (Palme and O’Neill 2014) plotted vs. the temperature (Lodders 2003) at which 50% of the element would be condensed from a gas of solar composition at…”