Open Access
Table C.11
Properties of the WASP-47 system
Parameter | Symbol | Value | Unit | Origin |
---|---|---|---|---|
Stellar parameters | ||||
Spectral type | G9 | Hellier et al. (2012) | ||
Stellar temperature | Teff | 5552 ± 75 | K | Vanderburg et al. (2017) |
Stellar mass | M* | 1 .040 ± 0.031 | M⊙ | Vanderburg et al. (2017) |
Stellar radius | R* | 1.137 ± 0.013 | R⊙ | Vanderburg et al. (2017) |
Stellar spin inclination | i* | ![]() |
deg | This work |
Stellar equatorial period | Peq | ![]() |
d | Bryant & Bayliss (2022) |
Stellar projected velocity | veq sin i* | ![]() |
km s−1 | Sanchis-Ojeda et al. (2015) |
Age | τ | ![]() |
Gyr | Almenara et al. (2016) |
Limb-darkening coefficients | u1 | 0.540 | Exofast | |
u2 | 0.209 | |||
Planet b parameters | ||||
Orbital period | P | 4.1591492 ± 0.0000006 | d | Bryant & Bayliss (2022) |
Transit epoch | T0 | 2457007.932103 ± 0.000019 | BJDtdb | Bryant & Bayliss (2022) |
Eccentricity | e | 0 (fixed) | Bryant & Bayliss (2022) | |
Argument of periastron | ω | 90 (fixed) | deg | Bryant & Bayliss (2022) |
Stellar reflex velocity | K | 140.84 ± 0.40 | m s−1 | Bryant & Bayliss (2022) |
Orbital inclination | i | ![]() |
deg | Bryant & Bayliss (2022) |
Projected spin-orbit angle | λ | 0 ± 24 | deg | Sanchis-Ojeda et al. (2015) |
3D spin-orbit angle | ψN | ![]() |
deg | This work |
ψS | ![]() |
deg | ||
ψ | ![]() |
deg | ||
Planet c parameters | ||||
Orbital period | P | 588.8 ± 2.0 | d | Bryant & Bayliss (2022) |
Inferior conjunction epoch | T0 | 2457763.1 ± 4.3 | BJDtdb | Bryant & Bayliss (2022) |
Eccentricity | e | 0.295 ± 0.016 | Bryant & Bayliss (2022) | |
Argument of periastron | ω | 112.0 ± 4.3 | deg | Bryant & Bayliss (2022) |
Stellar reflex velocity | K | 31.04 ± 0.40 | m s−1 | Bryant & Bayliss (2022) |
Planet d parameters | ||||
Orbital period | P | 9.03052118 ± 0.00000753 | d | This work |
Transit epoch | T0 | 2459426.5437 ± 0.0028 t | BJDTDB | This work |
Eccentricity | e | ![]() |
Bryant & Bayliss (2022) | |
Argument of periastron | ω | ![]() |
deg | Bryant & Bayliss (2022) |
Stellar reflex velocity | K | 4.26 ± 0.37 | m s−1 | Bryant & Bayliss (2022) |
Scaled separation | a/R* | ![]() |
Bryant & Bayliss (2022) | |
Orbital inclination | i | ![]() |
deg | Bryant & Bayliss (2022) |
Impact parameter | b | ![]() |
Bryant & Bayliss (2022) | |
Transit duration | T14 | 4.288 ± 0.039 | h | Vanderburg et al. (2017) |
Planet-to-star radius ratio | Rp/R* | 0.02876 ± 0.00017 | Bryant & Bayliss (2022) | |
Projected spin-orbit angle | Nondetection | deg | This work | |
Planet e parameters | ||||
Orbital period | P | 0.7895933 ± 0.0000044 | d | Bryant & Bayliss (2022) |
Transit epoch | T0 | 2457011.34862 ± 0.00030 | BJDtdb | Bryant & Bayliss (2022) |
Eccentricity | e | 0 (fixed) | Bryant & Bayliss (2022) | |
Argument of periastron | ω | 90 (fixed) | deg | Bryant & Bayliss (2022) |
Stellar reflex velocity | K | 4.55 ± 0.37 | m s−1 | Bryant & Bayliss (2022) |
Transit duration | T14 | 1.899 ± 0.013 | h | Vanderburg et al. (2017) |
† We caution that WASP-47 d displays strong TTV with an amplitude of ~6 min. We report here the mid-transit time calculated with a TTV model at the specific epoch of our RM observations (see Sect. 5.11).
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