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Table 4.
Comparison involving masses and radii derived by different authors for HD 219134 system.
| HD 219134 | L approach | R approach | (1) | (2) | (3) | |
|---|---|---|---|---|---|---|
| Star | R⋆ [R⊙] |
 |
0.7774 ± 0.0050 | 0.778 ± 0.005 | 0.778 ± 0.005 | 0.77 ± 0.02 |
| M⋆ [M⊙] |
 |
 |
0.81 ± 0.03 | 0.78 ± 0.02 |  |
|
| Planet b | Rp [R⊕] |
 |
 |
1.602 ± 0.055 | 1.606 ± 0.086 | |
| P = 3.1 days | Mp [M⊕] | 4.62 ± 0.14 | 4.68 ± 0.17 | 4.74 ± 0.19 | 4.36 ± 0.44 | 3.8 ± 0.3 |
| Planet c | Rp [R⊕] |
 |
1.511 ± 0.046 | 1.511 ± 0.047 | ||
| P = 6.8 days | Mp [M⊕] |  |
4.27 ± 0.21 | 4.36 ± 0.22 | 2.78 ± 0.65 (c) | 3.5 ± 0.6 |
| Planet d | Mp sin ip [M⊕] |  |
15.80 ± 0.56 | 16.17 ± 0.64 | 8.94 ± 1.13 (c) | 21.3 ± 1.3 |
| P = 46.9 days (a) | ||||||
| Planet f | Mp sin ip [M⊕] |  |
 |
7.30 ± 0.40 | 8.9 ± 1.0 | |
| P = 22.7 days (b) | ||||||
Notes.
References. (1): Gillon et al. (2017); (2): Motalebi et al. (2015); (3): Vogt et al. (2015).
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