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Table 6
Dynamical configuration of the Kepler-402 planetary system according to Rowe et al. (2014).
| Planet | b | c | d | e |
|---|---|---|---|---|
| Radius (R⊕) | 1.22 ± 0.24 | 1.56 ± 0.35 | 1.38 ± 0.27 | 1.46 ± 0.29 |
| Period (days) | 4.029 | 6.125 | 8.921 | 11.243 |
| Period ratio to inner planet | ∖ | 1.520 | 1.457 | 1.260 |
| (p, q, r) of 3BR(a) | (3, 5, 8) | (5, 11, 16) | ||
| Normalized B-values of 3BR(b) | 6.09 × 10−3 | 1.05 × 10−2 |
Notes. (a) Same definition as Table 5. (b) The non-adjacent planets b, c, and e are close to (7, 8, 15) 3BR with a small normalized B-value of 9.25 × 10−7.
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