Dynamical stability analysis of the HD 202206 system and constraints to the planetary orbits

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Table 5:

Orbital parameters of an orbit close to the center of libration of the 5:1 mean motion resonance.
Param.	S3	Inner	Outer
a	[AU]	0.8050	2.5113
i	[deg]	90	90
e		0.439	0.071
$M+\omega$	[deg]	239.25	247.30
$\omega$	[deg]	161.81	78.19
$\Omega$	[deg]	0	0
m	[ ${M}_{\rm Jup}$ ]	16.59	2.179
Date	[JD-2 400 000]	53 000.00
$\sqrt {\chi _{\rm r}^2}$		1.553

Notes. This orbit was obtained from S2 (Table 2) at the sixth iteration. We expect that the actual system will be closer to this orbit as dissipative processes will have dampened the resonant mode.

Source LaTeX | All tables | In the text

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