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

Open Access

Fig. 1

Typical configuration and notations for a rotating system made of L = 2 differentiated layers: the core (C) as layer 1, and the envelope (E) as layer 2. The polar radius is R_pol ≡ Z₂ and the equatorial radius is R_eq ≡ R₂. All layers rotate at the same rate Ω around the Z-axis.

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