Discovery Method
Transit
Consistent across records
Host star K2-265 • 1.71 R⊕ • 2.37 d orbit
Records
9
archive rows
Discovery
2018
Transit
Radius
1.71 R⊕
default parameter set
Mass
7.34 M⊕
default parameter set
K2-265
1366 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
K2-265
Stable across source rows
Discovery Method
Transit
Consistent across records
Discovery Year
2018
Stable across source rows
Orbital Period
2.37 day
2.37 to 2.37
Semi-Major Axis
0.03 au
0.03 to 0.03
Radius
1.71 Rearth
1.62 to 1.71
Mass
7.34 Mearth
4.60 to 7.34
Density
7.90 g/cm**3
5 to 7.90
Equilibrium Temperature
1366 K
1243.4 to 1366
Scale Comparison
Current adopted radius: 1.71 R⊕ • circles scaled linearly by radius
Earth
1.0 R⊕ baseline
K2-265 b
1.71 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 | 2.37 day | 1.66 Rearth | — | — | Mayo et al. 2018 |
| 2018 | Transit | K2 | 0.95 m Kepler Telescope | 2.37 day | 1.67 Rearth | — | — | Kruse et al. 2019 |
| 2018 | Transit | K2 | 0.95 m Kepler Telescope | 2.37 day | 1.71 Rearth | 6.54 Mearth | — | Lam et al. 2018 |
| 2018 | Transit | K2 | 0.95 m Kepler Telescope | 2.37 day | 1.62 Rearth | — | — | Crossfield et al. 2016 |
| 2018 | Transit | K2 | 0.95 m Kepler Telescope | 2.37 day | 1.68 Rearth | 4.60 Mearth | 1257 K | Howard et al. 2025 |
| 2018 | Transit | K2 | 0.95 m Kepler Telescope | 2.37 day | 1.63 Rearth | — | — | Vanderburg et al. 2016 |
| 2018 | Transit | K2 | 0.95 m Kepler Telescope | 2.37 day | 1.66 Rearth | — | 1243.4 K | ExoFOP |
| 2018 | Transit | K2 | 0.95 m Kepler Telescope | 2.37 day | 1.71 Rearth | 7.34 Mearth | 1366 K | Thygesen et al. 2023 |
| 2018 | Transit | K2 | 0.95 m Kepler Telescope | 2.37 day | — | — | — | Barros et al. 2016 |