Table 3
Minimum mass values for planets above the radius gap.
| Planet above Radius gap | Radius (R⊕) | P orb (days) | Measured mass (M⊕) | Minimum mass prediction from each planet bel ow 2 R⊕ (M⊕) | |||
|---|---|---|---|---|---|---|---|
| Kepler-102e | 2.22 | 16.15 | 8.93 | Kepler-102 b LM | Kepler-102c 0.12 | Kepler-102 d 2.73 | Kepler-102 f No Solution |
| Kepler-68 c | 0.93 | 9.6 | 5.97 | Kepler-68 b 3.75 | Kepler-68 d Radius unknown | ||
| Kepler-49 d | Kepler-49 e | ||||||
| Kepler-49 b | 2.69 | 7.2 | − | 1.0 | 1.0 | ||
| Kepler-49 c | 2.58 | 10.91 | − | LM | LM | ||
| Kepler-125 b | 2.37 | 4.16 | − | Kepler-125 c 1.0 | |||
| Kepler-11 b | |||||||
| Kepler-11 c | 2.87 | 13.03 | 2.9 | No Solution | |||
| Kepler-11 d | 3.12 | 22.69 | 7.3 | 4.51 | |||
| Kepler-11 e | 4.19 | 31.99 | 9.53 | 2.02 | |||
| Kepler-11 f | 2.49 | 46.69 | 1.99 | 1.59 | |||
| Kepler-11 g | 3.67 | 118.38 | 301.9 | 0.33 | |||
| HD 3167 b | |||||||
| HD 3167 c | 3.02 | 29.85 | 9.78 | 0.13 | |||
| Kepler-10 b | |||||||
| Kepler-10 c | 2.35 | 45.29 | 7.36 | LM | |||
| Kepler-20 b | Kepler-20 e | Kepler-20 f | |||||
| Kepler-20 c | 3.05 | 10.85 | 12.75 | 3.49 | 0.35 | 2.839 | |
| Kepler-20 d | 2.74 | 77.61 | 10.06 | 0.23 | LM | 0.23 | |
| K2-3 b | 2.17 | 10.05 | 6.47 | K2-3 c No Solution | K2-3 d No Solution | ||
| Kepler-9 d | |||||||
| Kepler-9 b | 8.20 | 19.22 | 43.5 | 0.997 | |||
| Kepler-9 c | 8.29 | 38.97 | 29.9 | 0.769 | |||
| Kepler-18 b | |||||||
| Kepler-18 c | 5.48 | 7.6 | 17.20 | 5.36 | |||
| Kepler-18 d | 6.97 | 14.86 | 16.29 | 2.14 | |||
| Kepler-126 b | Kepler-126c | ||||||
| Kepler-126 d | 2.51 | 100.28 | − | 0.3* | 0.96* | ||
| Kepler-127 b | Kepler-127d | ||||||
| Kepler-127 c | 2.39 | 29.39 | − | − | 1.79* | ||
| Kepler-218 b | |||||||
| Kepler-218 c | 3.13 | 44.70 | − | 1.0* | |||
| Kepler-218 d | 2.66 | 124.5 | − | LM | |||
Notes. The planets listed in the left half of the table are above the radius gap and have an observed mass listed in column 4. These can be compared to their minimum mass predicted from the planets below the period gap (right hand section of the table). Systems marked “No Solution” are not compatible with the photoevaporation model. Note that the mass values in the right half of the table are predictions for the mass of planets in the left half, not masses of the planets in the right half. Minimum mass values with an asterisk had estimated solar mass values used in the calculation. Planets that do not constrain the minimum mass are marked LM. The minimum masses are estimated using the Owen & Campos Estrada (2020) code.
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