Fig. 8

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Gravitational harmonics J2, J4 for Uranus (a) and Neptune (b) in case (ii) models (stars) and case (iv) models (dots). The colour of the dots indicates the parameter PZ. The colour of the stars indicates the H2 –H2O phase diagram used. Dark pink crosses show observed values. Light pink crosses are wind-corrected static J4 values (see text for details). In the case of Neptune, the V23 conv-1800 K and SFB-linear-4 GPa stars overlap. We note the change in units for J2 and J4 with respect to Table 1. Panels c and d show stars which are the same models as in (a) and (b), and circles: case (iii) models. This figure shows that a mixture of rocks (circles) in the deep interior below the 2000 K level, and water reduces the resulting |J4| values.
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