Development of a C/H/O/N/S chemical network: Experimental benchmark, application to exoplanets, and identification of key C/S coupling pathways

Open Access

Table 2

Exoplanets simulated in this study and the input parameters.

Planet name	Planet type	Star type	D (au)	R (R_J)	T (K)	K_zz (cm²/s)	g (m/s²)	M (solar)
GJ 436 b	Warm Neptune	M3V	0.029	0.38	1094	10⁸	12.6	10
GJ 1214 b	Warm Neptune	M4.5V	0.014	0.24	1054	3 × 10⁷ × P^−0.4	8.93	100
HD 189733 b	Hot Jupiter	K2V	0.031	1.14	1470	profile	21.5	1
HD 209458 b	Hot Jupiter	F9V	0.047	1.38	1671	profile	9.54	1
WASP-39 b	Hot Jupiter	G8	0.048	1.31	1604	profile	4.26	10
WASP-107 b	Warm Neptune	K6	0.055	0.94	1051	10¹⁰	2.6	10

Notes. The parameter D denotes the distance to the host star, R the planet radius, T the temperature at 1 bar, K_zz the eddy diffusion coefficient, and M the metallicity relative to solar abundances.

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