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Table 1

Summary of stellar, input, and derived parameters of the WASP-189 system.

Fitted parameters
Mid-transit time (T0)
[BJDTT −2450 000]
Impact parameter (b)
Scaled semi-major axis (aR*)
Eclipse duration (T14) [h]
Occultation depth (dFocc) [ppm] 87.9 ± 4.3
Radius ratio (RpR*)
u+ = ua + ub
u = uaub
Stellar inclination I* [°]
Projected orbital obliquity λ [°]

Additional input parameters

RV amplitude (K) [km s−1] 0.182 ± 0.013
Planetary period (a) (P) [d] 2.7240330
Eccentricity (a) (e) 0

Stellar parameters

Stellar Mass (M*) [M] 2.030 ± 0.066
Stellar Radius (R*) [R] 2.36 ± 0.030
Stellar eff. temperature (Teff) [K] 8000 ± 80
Stellar surface gravity log g [ log g] 3.9 ± 0.2
Projected rotational velocity 93.1 ± 1.7
νsinI* [km s−1]
Microturbulent velocity 2.7 ± 0.3
νmic [km s−1]
Iron abundance [Fe/H] + 0.29 ± 0.13
System age [Myr] 730 ± 130

Derived parameters

Plan. radius (RP) [RJ ] 1.619 ± 0.021
Plan. mass (MP) [MJ ]
Plan. mean density (ρP) [ρJ ]
Plan. surface gravity (gP) [m s−2 ]
Orbital semi-major axis (a) [au] 0.05053 ± 0.00098
Orbital inclination (i) [°] 84.03 ± 0.14
True orbital obliquity Ψ [°] 85.4 ± 4.3
Dayside equilibrium temp. (b) (Teq) [K]
Brightness temp. (c) (Tb) [K]
Dayside temp. (d) (Tday) [K] 3435 ± 27

Notes. (a) Fixed. (b) , assuming immediate re-radiation (f = 2∕3) and zero albedo (AB = 0). (c) Assuming black body stellar and planetary SEDs. (d)Assuming a PHOENIX stellar model spectrum, Ag = 0, and inefficient energy circulation (ɛ = 0).

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