Discovery Method
Transit
Consistent across records
Host star K2-36 • 3.20 R⊕ • 5.34 d orbit
Records
9
archive rows
Discovery
2016
Transit
Radius
3.20 R⊕
default parameter set
Mass
7.90 M⊕
default parameter set
K2-36
854 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: Bonomo et al. 2023
Host Star
K2-36
Stable across source rows
Discovery Method
Transit
Consistent across records
Discovery Year
2016
Stable across source rows
Orbital Period
5.34 day
5.34 to 5.34
Semi-Major Axis
0.06 au
0.05 to 0.06
Radius
3.20 Rearth
2.41 to 3.58
Mass
7.90 Mearth
7.80 to 26
Density
1.30 g/cm**3
1.30 to 9.40
Equilibrium Temperature
854 K
772 to 854
Scale Comparison
Current adopted radius: 3.20 R⊕ • circles scaled linearly by radius
Earth
1.0 R⊕ baseline
K2-36 c
3.20 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 |
|---|---|---|---|---|---|---|---|---|
| 2016 | Transit | K2 | 0.95 m Kepler Telescope | 5.34 day | 3.58 Rearth | — | — | Mayo et al. 2018 |
| 2016 | Transit | K2 | 0.95 m Kepler Telescope | 5.34 day | 2.41 Rearth | 26 Mearth | 772 K | Howard et al. 2025 |
| 2016 | Transit | K2 | 0.95 m Kepler Telescope | 5.34 day | 3.20 Rearth | 7.80 Mearth | 788 K | Damasso et al. 2019 |
| 2016 | Transit | K2 | 0.95 m Kepler Telescope | 5.34 day | 3.12 Rearth | — | — | Duck et al. 2021 |
| 2016 | Transit | K2 | 0.95 m Kepler Telescope | 5.34 day | 3.20 Rearth | 7.90 Mearth | 854 K | Bonomo et al. 2023 |
| 2016 | Transit | K2 | 0.95 m Kepler Telescope | 5.34 day | — | — | — | Barros et al. 2016 |
| 2016 | Transit | K2 | 0.95 m Kepler Telescope | 5.34 day | 2.80 Rearth | — | 793 K | Sinukoff et al. 2016 |
| 2016 | Transit | K2 | 0.95 m Kepler Telescope | 5.34 day | 2.65 Rearth | — | — | Crossfield et al. 2016 |
| 2016 | Transit | K2 | 0.95 m Kepler Telescope | 5.34 day | 2.82 Rearth | — | — | Vanderburg et al. 2016 |