Impact of rotation on synthetic mass–radius relationships of two-layer rocky planets and water worlds

Open Access

Fig. I.1

Mean coefficients $⟨ c_{1}^{'} ⟩ \pm Δ_{1}$ $\langle c_1' \rangle \pm \Delta_1$ (top) and $⟨ c_{2}^{'} ⟩ \pm Δ_{2}$ $\langle c_2' \rangle \pm \Delta_2$ (bottom) of the mass-radius relationship for a two-layer IW planet versus the flattening parameter f, the fits (plain lines) and the absolute errors in fitting the means (dashed-lines, right axis).

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