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

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Table 1

Data^⋆ for the modified EoS from Seager et al. (2007) according to Eq. (4).

	ρ_s, in g/cm³	K^-m	m	Index n	Exponent γ	$\frac{1 - n}{3 - n} \equiv β$ $\frac{1-n}{3-n} \equiv \beta$
Iron	8.30	1.034726 × 10^-6	0.528	1.11864	1.89393	-0.06306
Perovskite	4.10	0.463261 × 10^-6	0.541	1.17864	1.84842	-0.09809
Water	1.46	0.954465 × 10^-6	0.513	1.05338	1.94931	-0.02743

Notes. ^(*)The coefficient K is given in g/cm³ × (dyn/cm²)^-m, and assumes that P is in dyn/cm² (see note 1). Coefficients n and $γ = 1 + \frac{1}{n}$ $\gamma=1+\frac{1}{n}$ are computed in the limit of high pressures, i.e. $γ = \frac{1}{m}$ $\gamma=\frac{1}{m}$ .

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