Fig. 7

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Mass of water in the surface (condensed and vapour), mantle, and core reservoirs after 100 Myr of evolution for Earth (filled circles) and Mars (asterisks) as a function of the partition coefficient of water between metal melt and silicate melt. The measurement is given for H2 + O to reflect the H2O equivalent mass of the dissolved H in the core and the mantle. The best match to the surface water reservoir of Earth is found for high values of DH = 5 and DH = 8. Mars, on the other hand, loses all its surface water unless DH = 3 or less. The core reservoir mass falls with decreasing DH, particularly for Mars that has a smaller core than Earth. This hydrogen was outgassed as H2 from the martian mantle and subsequently lost to hydrodynamical escape. The mantles of Earth and Mars store significant H2 reservoirs that can later be outgassed as H2 and H2O in volcanism and after impacts. The symbols are displaced slightly horizontally to better distinguish them.
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