Crustal recycling, mantle dehydration, and the thermal evolution of Mars

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Thermochemical evolution of Mercury's interior (2013, background): “The solidus of the mantle residue is increased linearly with the degree of depletion [Morschhauser et al., 2011], and we assume a total maximum solidus change of 150 K between undepleted and depleted peridotite, i.e., harzburgite [Maaløe, 2004], at a maximum melt fraction of 40%.”
Outgassing History and Escape of the Martian Atmosphere and Water Inventory (2015, methodology): “The partition coefficient of water is most likely close to 0.01 (Katz et al. 2003), and melt fractions obtained from numerical models average around 5 − 10 % (Hauck et al. 2002; Morschhauser et al. 2011).”
Very recent and wide‐spread basaltic volcanism on Mars (2011, background): “…models predicting zones of partial melt underneath or an enhanced heat flow at Tharsis [e.g., Schumacher and Breuer, 2007; Grott and Breuer, 2010; Morschhauser et al., 2011], the observed young volcanic ages have been reported for very localized phenomena only, e.g., the platy terrain of…”