Open Access
Table 1
Parameters of the WASP-69 system.
Parameter | Symbol (Unit) | Value | Reference |
---|---|---|---|
Stellar parameters | |||
Apparent magnitude | mv | 9.87 | Høg et al. (2000) |
Luminosity | L⋆ (L⊙) | 0.33 | This work |
Distance | d (pc) | 50.3 | Sousa et al. (2021) |
Stellar age | Age (Gyr) | 1–2.6 | This work |
Stellar mass | M⋆ (M⊙) | 0.83 ± 0.05 | This work |
Stellar radius | R⋆ (R⊙) | 0.801 ± 0.015 | This work |
Effective temperature | Teff (K) | 4792 ± 158 | This work |
Metallicity | [Fe/H] (dex) | 0.35 ± 0.07 | This work |
Turbulent velocity | Vturb (km s−1) | 0.55 ± 0.008 | This work |
Surface gravity(1) | log g⋆ (cgs) | 4.16 ± 0.037 | This work |
Surface gravity(2) | log g⋆ (cgs) | 4.57 ± 0.037 | This work |
Activity indicator | log ![]() |
−4.597 ± 0.001 | This work |
Limb-darkening coefficient | u1 | 0.2669 | This work |
Limb-darkening coefficient | u2 | 0.2657 | This work |
Spin inclination | i⋆ (deg) | ![]() |
This work |
Equatorial rotation period | Peq (days) | 23.07 ± 0.16 | Anderson et al. (2014) |
Projected rotational velocity | vsini⋆ (km s−1) | 1.54 ± 0.05 | This work |
Stellar RV semi-amplitude | K⋆ (m s−1) | 38.1 ± 2.4 | Anderson et al. (2014) |
Planetary parameters | |||
Planet mass | Mp (M⊕) | 82.58 ± 5.37 | This work |
Planet mass | Mp (MJup) | 0.26 ± 0.02 | This work |
Planet radius | Rp (R⊕) | 11.21 ± 0.22 | This work |
Planet radius | Rp (RJup) | 1.00 ± 0.02 | This work |
Equilibrium temperature(3) | Teq (K) | 971 ± 33 | This work |
Projected spin-orbit angle | λ (deg) | 0.05 ± 1.10 | This work |
3D spin-orbit angle(4) | ψ (deg) | ![]() |
This work |
Mid-transit time | Tc (BJDTDB) | 2455748.83428 ± 0.00013 | This work |
Orbital period | P (d) | 3.86813881 ± 0.00000013 | This work |
Transit duration (t1 to t4) | t14 (h) | 2.1869 ± 0.0053 | This work |
Orbital semi-major axis | a (R⋆) | 12.17 ± 0.07 | This work |
Orbital semi-major axis | a (AU) | 0.0453 ± 0.0008 | This work |
Orbit inclination | ip (deg) | 86.79 ± 0.04 | This work |
Eccentricity | e | 0 (fixed) | This work |
Periastron argument | ω | 90 (fixed) | This work |
Notes. (1)surface gravity from spectroscopy; (2)surface gravity calibrated with Mortier et al. (2014) and adopted in the this study; (3)assuming a null albedo; (4)the 3D spin–orbit angle is combined over the two degenerate configurations for the stellar inclination (see text).
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