Discovery Method
Transit
Consistent across records
Host star K2-237 • 16.06 R⊕ • 2.18 d orbit
Records
9
archive rows
Discovery
2018
Transit
Radius
16.06 R⊕
default parameter set
Mass
434.2 M⊕
default parameter set
K2-237
1759 K equilibrium
Canonical Summary
Values come from the archive's default parameter set. Missing values stay missing. Ranges and counts describe all source rows.
Selected source: Thygesen et al. 2023
Host Star
K2-237
Stable across source rows
Discovery Method
Transit
Consistent across records
Discovery Year
2018
Stable across source rows
Orbital Period
2.18 day
2.18 to 2.18
Semi-Major Axis
0.04 au
0.04 to 0.04
Radius
16.06 Rearth
16.06 to 18.49
Mass
434.2 Mearth
392.8 to 508.5
Density
0.58 g/cm**3
0.37 to 0.58
Equilibrium Temperature
1759 K
1654.4 to 1884
Scale Comparison
Current adopted radius: 16.06 R⊕ • circles scaled linearly by radius
Earth
1.0 R⊕ baseline
K2-237 b
16.06 R⊕
Jupiter
11.2 R⊕ reference
Provenance
Evidence Summary
Rows
9
Refs
9
Methods
1
| Year | Method | Facility | Telescope | Period | Radius | Mass | Eq. Temp | Reference |
|---|---|---|---|---|---|---|---|---|
| 2018 | Transit | K2 | 0.95 m Kepler Telescope | 2.18 day | 16.20 Rearth | 433.2 Mearth | 1828 K | Ikwut-Ukwa et al. 2020 |
| 2018 | Transit | K2 | 0.95 m Kepler Telescope | 2.18 day | 18.49 Rearth | 508.5 Mearth | 1884 K | Soto et al. 2018 |
| 2018 | Transit | K2 | 0.95 m Kepler Telescope | 2.18 day | — | — | — | Patel & Espinoza 2022 |
| 2018 | Transit | K2 | 0.95 m Kepler Telescope | 2.18 day | — | — | — | Kokori et al. 2022 |
| 2018 | Transit | K2 | 0.95 m Kepler Telescope | 2.18 day | — | — | — | Ivshina & Winn 2022 |
| 2018 | Transit | K2 | 0.95 m Kepler Telescope | 2.18 day | — | — | — | Kokori et al. 2023 |
| 2018 | Transit | K2 | 0.95 m Kepler Telescope | 2.18 day | 16.70 Rearth | — | 1654.4 K | ExoFOP |
| 2018 | Transit | K2 | 0.95 m Kepler Telescope | 2.18 day | 16.06 Rearth | 434.2 Mearth | 1759 K | Thygesen et al. 2023 |
| 2018 | Transit | K2 | 0.95 m Kepler Telescope | 2.18 day | 18.41 Rearth | 392.8 Mearth | 1838 K | Smith et al. 2019 |