Table 4
System parameters of K2-32 obtained from the joint light curve and radial velocity analysis with PASTIS.
Planet parameters | K2-32 e | K2-32 b | K2-32 c | K2-32 d |
---|---|---|---|---|
Orbital period P [d] | 4.34934 ± 0.00039 | 8.99200 ± 0.00008 | ![]() |
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T0 [BJD - 2 400 000] | ![]() |
56900.92676 ± 0.00031 | ![]() |
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RV semi-amplitude K [m s−1] | ![]() |
5.22 ± 0.60 | ![]() |
1.53 ± 0.58 |
Orbital inclination i [°] | 89.0 ± 0.7 | ![]() |
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89.4 ± 0.1 |
Planet-to-star radius ratio k | ![]() |
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Orbital eccentricity e | ![]() |
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Argument of periastron ω [°] | ![]() |
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System scale a∕R⋆ | ![]() |
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Impact parameter b | 0.22 ± 0.16 | ![]() |
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Transit duration T14 [h] | ![]() |
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Semi-major axis a [AU] | ![]() |
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Planet mass M [M⊕] | ![]() |
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8.1 ± 2.4 | 6.7 ± 2.5 |
Planet radius R [R⊕] | ![]() |
5.299 ± 0.191 | ![]() |
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Planet bulk density ρ [g cm−3] | ![]() |
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Mean Eq. temperature Teq [K] | ![]() |
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Day-side temperature Teq, d [K] | ![]() |
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Notes. Stellar parameters from Table 3 (derived from PASTIS and not from the spectral analysis). We assumed R⊙ = 695 508 km, M⊙ = 1.98842 × 1030 kg, R⊕ = 6 378 137 m, M⊕ = 5.9736 × 1024 kg and 1 AU = 149 597 870.7 km. The temperatures were derived assuming a zero albedo. The day-side temperature was computed assuming tidally synchronized rotation.
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