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

Open Access

Table 4

Relative core size, q, calculated from Eq. (33) for LHS 1140 b in different spin states f ∈ {0,0.1,0.2}, assuming a two-layer planet.

	f	(x₀, y₀)	C₁	C₂	C₃	C₄
IW	0	0.641	0.647	0.613	0.634	0.668
	0.10	0.703	0.708	0.676	0.696	0.729
	0.20	0.771	0.776	0.746	0.765	0.795

IP	0	q^σ < 0	q^σ < 0	q^σ < 0	q^σ < 0	q^σ < 0^‡
	0.0681^⋆	0
	0.0636^†	0
	0.10	0.3277	0.364	q^σ < 0	0.280	0.466
	0.20	0.5638	0.580	0.470	0.547	0.637

PW	0	0.937	0.946	0.894	0.927	0.979
	0.0962^⋆	1
	0.10	q^σ > 1	q^σ > 1	0.964	0.994	q^σ > 1
	0.20	q^σ > 1	q^σ > 1	q^σ > 1	q^σ > 1	q^σ > 1

Notes. ^*Single-layer limit of Eq. (33). ^†from Eq. (18). ^‡Tiny core solution with the DROP code.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.