Table 1
Main physical and orbital parameters of the HAT-P-11 system.
Parameter(a) | Value | Reference |
---|---|---|
Stellar parameters | ||
Spectral class | K4 V | 1 |
M* (M⊙) | 0.86 ± 0.06 | 2 |
R⋆ (R⊙) | 0.76 ± 0.01 | 2 |
Teff (K) | 4780 ± 50 | 1 |
[Fe/H] | 0.31 ± 0.05 | 1 |
log g (log10, cgs) | ![]() |
3 |
Vsys (km s−1) | −63.24 ± 0.26 | 4 |
Distance (ly) | 123.17 ± 0.11 | 4 |
Age (Gyr) | ![]() |
2 |
H | 7.131 ± 0.021 | 5 |
Planetary parameters | ||
Mp (Mj) | 0.0787 ± 0.0048 | This work |
Rp (Rj) | 0.4466 ± 0.0059 | This work |
Mp (M⊕) | 25.0 ± 1.5 | This work |
Rp (R⊕) | 4.901 ± 0.065 | This work |
ρp (g cm−3) | 1.172 ± 0.085 | This work |
Teq (K) | ![]() |
This work |
Porb (days) | 4.887802443 ± 0.000000034 | 6 |
T0 (BJDtdb) | 2454 957.8132067 ± 0.0000053 | 6 |
i (deg) | 89.027 ± 0.068 | This work |
e | ![]() |
This work |
ωp (deg) | ![]() |
This work |
a (au) | 0.0532 ± 0.0010 | This work |
Kp (km s−1) | 123.4 ± 9.9 | This work |
Notes. (a)The symbols of the parameters listed in the table have the following meanings: M⋆ – stellar mass; R⋆ – stellar radius; Teff – stellar effective temperature; [Fe/H] – stellar metallicity; log g – logarithm of stellar surface gravity; Vsys – systemic radial velocity; H – apparent magnitude in the photometric H band; Mp – planetary mass; Rp – planetary radius; ρp – planetary mean density; Teq – planetary equilibrium temperature computed at the planet-to-star distance during the secondary eclipse, assuming an inefficient (full) heat re-distribution for the derived geometrical albedo ; Porb – orbital period; T0 – transit epoch; i – orbital inclination; e – orbital eccentricity; ωp – planetary argument of periastron; a – orbital semi-major axis; Kp -planetary radial-velocity semi-amplitude.
References. 1. Bakos et al. (2010); 2. Lundkvist et al. (2016); 3. Stassun et al. (2019); 4. Gaia Collaboration (2018); 5. Cutri et al. (2003); 6. Huber et al. (2017).
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