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Table 1

Physical properties of the extreme planetary system HD 196885, the stellar host (Aa), the binary companion (B) and the cir-cumprimary planet (Ab) based on the latest studies from Correia et al. (2008); Fischer et al. (2009); Chauvin et al. (2011); Gaia Collaboration (2021).

Primary star: HD 196885 Aa
Spectral type F8V
G (mag) 6.276973 ± 0.002767
V (mag) 6.385 ± 0.010
H (mag) 5.190 ± 0.023
Teff (K) 6340 ± 39
log(ɡ) (dex) 4.46 ± 0.02
Fe/H (dex) 0.29 ± 0.05
Distance (pc) 34.00 ± 0.04
µα (masyr−1) 71.915 ± 0.032
µδ (masyr−1) 89.318 ± 0.026
Age (Gyr) 1.5–3.5
MAa(M) 1.3 ± 0.1
log(L/L) 2.4 ± 0.1

Exoplanet: HD 196885 Ab

MAbsin(iAaAb) (MJup) 2.98 ± 0.05
PAaAb (yr) 3.63 ± 0.01
eAaAb 0.48 ± 0.02
ωAaAb (deg) 93.2 ± 3.0
tP,AaAb 2002.85 ± 0.02
aAaAb (au) 2.6 ± 0.1

Binary companion: HD 196885 B

Spectral type M1 ± 1
KB (mag) 6.398 ± 250
MB (MΘ) 0.45 ± 0.01
PAB (yr) 72.06 ± 4.59
eAB 0.42 ± 0.03
ωAB (deg) −118.1 ± 3.1
ΩAB (deg) 79.8 ± 0.1
iAB (deg) 116.8 ± 0.7
iP,AB 1985.59 ± 0.39
a AB (au) 21.00 ± 0.86

Notes. We consider below that the system is composed of the inner binary subsystem AaAb (composed by the primary star Aa and the exo-planet Ab), and the outer binary subsystem AB (composed by the center of mass of the inner orbit A and the companion star B).

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