The hydrology of carbonaceous chondrite parent bodies and the evolution of planet progenitors

By E. Young. Philosophical Transactions of the Royal Society of London. Series A: Mathematical, Physical and Engineering Sciences, 2001

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Ceres’ evolution and present state constrained by shape data (2010, background): “It is more widely believed that the silicates were aqueously altered and metasomatized in the early planetesimals as a result of hydrothermal activity (e.g., Wilson et al., 1999; Young, 2001).”
A model for planetesimal meltdown by 26Al and its implications for meteorite parent bodies (2006, background): “…of planetesimals by 26Al have dealt with the sub-solidus thermal (and aqueous) metamorphism of chondritic parent bodies (e.g., Miyamoto 1991; Ghosh et al. 1999, 2003; Cohen and Coker 2000; Young 2001; LaTourrette and Wasserburg 1998), a few studies have explored the melting of planetesimals.”
Accretion and differentiation of the terrestrial planets with implications for the compositions of early-formed Solar System bodies and accretion of water (2014, background): “Models for the hydrology of the parent bodies of these rocks indicate that the 21 parent bodies had excesses of water relative to that required to form hydrated minerals and that large reservoirs of water were retained within them (Young et al. 1999; Young 2001; Palguta et al. 2010).”