Life in the dark - Potential urability of the moons of rogue planets

Open Access

Table 1

Parameter space used for modeling the SN II explosion. The table lists stellar, planetary, and moon parameters for the simulations.

	Parameter	$e_{p}^{(0)} = 0$ $e_{\rm{p}}^{(0)} = 0$	$e_{p}^{(0)} \neq 0$ $e_{\rm{p}}^{(0)} \ne 0$	$e_{m}^{(0)} \neq 0$ $e_{\rm{m}}^{(0)} \ne 0$	$n_{m}^{(0)} : n_{res}^{(0)}$ $n_{\rm{m}}^{(0)}:n_{{\rm{res}}}^{(0)}$
Stars	M_ej (M_⊙)	8
	(M_n M_⊙)	2
	v_max (km s⁻¹)	1000; 10000			10000
Planets	M_p (M_Jup)	0.01; 0.1; 1; 10
	$a_{p}^{(0)} (CsE)$ $a_{\rm{p}}^{(0)}({\rm{CsE}})$	[5.14:200]^*	13.95		[5.14:200]^∗
	$e_{p}^{(0)}$ $e_{\rm{p}}^{(0)}$	0	0.1; 0.2; 0.4; 0.6; 0.8	0
	$f_{p}^{(0)} (^{°})$ $f_{\rm{p}}^{(0)}\left( {^^\circ } \right)$	0	0, 90, 180, 270	0
Moons	M_m (M_p)	2.5 × 10⁻⁵
	$a_{m}^{(0)} (R_{p})$ $a_{\rm{m}}^{(0)}\left( {{R_{\rm{p}}}} \right)$	5.89; 9.39; 14.97; 26.33			9.39
	$e_{m}^{(0)}$ $e_{\rm{m}}^{(0)}$	0		10⁻⁴; 10⁻³ ; 10⁻²; 10⁻¹	0
	$f_{m}^{(0)} (^{\circ})$ $f_{\rm{m}}^{(0)}\left( {^ \circ } \right)$	0; 90; 180; 270
	M_res (M_m)	–			0.5; 1; 2
	Res.	–			2:1; 3:1; 3:2

Notes. ^(*) Logarithmic sampling of 12 points on the indicated interval.

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