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Table 6
System parameters for WASP-68.
General information | ||
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RA (J2000) | 20 20 22.98 | |
Dec (J2000) | –19 18 52.9 | |
V | 10.7 | |
K | 8.9 | |
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Stellar parameters from spectroscopic analysis | ||
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Teff (K) | 5910 ± 60 | |
log g⋆ [cgs] | 4.17 ± 0.11 | |
[Fe/H] | 0.22 ± 0.08 | |
ξt (km s-1) | 1.4 ± 0.1 | |
vmac (km s-1) | 2.6 ± 0.3 | |
v sin i⋆ (km s-1) | 2.3 ± 0.8 | |
Sp. type | G0 | |
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Parameters from MCMC analyses | ||
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Jump parameters | e ≥ 0 | e = 0 (adopted) |
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Planet/star area ratio (Rp/R⋆)2 [%] | 0.57 ± 0.03 |
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b′ = acosip/R⋆ [R⋆] |
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Transit width W [d] |
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T0 [HJDTDB] |
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Orbital period P [d] | 5.084299 ± 0.000015 | 5.084298 ± 0.000015 |
RV K2 [ms-1d1/3] | 168.2 ± 3.3 |
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RV slope [ms-1y-1] | 14 ± 2 | 14 ± 2 |
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0 (fixed) |
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0 (fixed) |
c 1,I + z | 0.79 ± 0.04 |
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c 2,I + z | –0.31 ± 0.02 | −0.31 ± 0.03 |
c 1, Ic | 0.84 ± 0.03 | 0.84 ± 0.02 |
c 2, Ic | −0.29 ± 0.02 | −0.29 ± 0.02 |
Effective temperature Teff[K]a | 5911 ± 60 |
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Metallicity [Fe/H] [dex]a | 0.22 ± 0.08 | 0.22 ± 0.08 |
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Deduced stellar parameters | ||
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Mean density ρ⋆ [ρ⊙] |
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Surface gravity log g⋆ [cgs] |
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Mass M⋆ [M⊙] | 1.23 ± 0.03 | 1.24 ± 0.03 |
Radius R⋆ [R⊙] |
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Luminosity L⋆ [L⊙] |
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u 1,I + z | 0.25 ± 0.02 |
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u 2,I + z | 0.28 ± 0.01 | 0.28 ± 0.01 |
u 1, Ic | 0.28 ± 0.01 | 0.28 ± 0.01 |
u 2, Ic | 0.28 ± 0.01 | 0.28 ± 0.01 |
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Deduced planet parameters | ||
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RV K [ms-1] | 97.9 ± 1.9 | 97.9 ± 1.9 |
Planet/star radius ratio Rp/R⋆ | 0.075 ± 0.002 | 0.075 ± 0.002 |
btr [R⋆] |
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boc [R⋆] |
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Toc [HJDTDB] | 2456067.444 ± 0.029 | 2456067.406 ± 0.001 |
Scaled semi-major axis a/R⋆ |
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Orbital semi-major axis a [AU] |
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Orbital inclination ip [deg] |
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88.1 ± 1.3 |
Orbital eccentricity e | ![]() |
0 (fixed) |
Argument of periastron ω [deg] |
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– |
Mean density ρp [ρJup] |
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Surface gravity log gp [cgs] |
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Mass Mp [MJup] | 0.95 ± 0.03 | 0.95 ± 0.03 |
Radius Rp [RJup] |
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Roche limit aR[AU]b |
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a/aR |
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Equilibrium temperature Teq[K]c |
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Irradiation [erg s-1cm-2] |
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Notes. The values given for the parameters derived from our MCMC analyses are medians and 1σ limits of the marginalized posterior probability distributions.
(b)
Using aR = 2.46 Rp(M⋆/Mp)1/3 (Chandrasekhar 1987).
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