Discovery Method
Transit
Consistent across records
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ExoplanetDetail
K2-25 b
Host star K2-25 • 3.44 R⊕ • 3.48 d orbit
Records
8
archive rows
Discovery
2015
Transit
Radius
3.44 R⊕
default parameter set
Mass
24.50 M⊕
default parameter set
K2-25
494 K equilibrium
Canonical Summary
Adopted planet values from the default parameter set
Values come from the archive's default parameter set. Missing values stay missing. Ranges and counts describe all source rows.
Selected source: Stefansson et al. 2020
Host Star
K2-25
Stable across source rows
Discovery Year
2015
Stable across source rows
Orbital Period
3.48 day
3.48 to 3.48
Semi-Major Axis
0.03 au
single adopted value
Radius
3.44 Rearth
3.43 to 4.21
Mass
24.50 Mearth
single adopted value
Equilibrium Temperature
494 K
447.8 to 494
Scale Comparison
Radius against familiar reference worlds
Current adopted radius: 3.44 R⊕ • circles scaled linearly by radius
Earth
1.0 R⊕ baseline
K2-25 b
3.44 R⊕
Jupiter
11.2 R⊕ reference
Provenance
Underlying measurements and references
Evidence Summary
Rows
8
Refs
8
Methods
1
Discoverystable
Facilitystable
Periodstable
Radiusdisputed
Massstable
Eq. Tempdisputed
| Year | Method | Facility | Telescope | Period | Radius | Mass | Eq. Temp | Reference |
|---|---|---|---|---|---|---|---|---|
| 2015 | Transit | K2 | 0.95 m Kepler Telescope | 3.48 day | — | — | — | Rizzuto et al. 2017 |
| 2015 | Transit | K2 | 0.95 m Kepler Telescope | 3.48 day | 3.44 Rearth | 24.50 Mearth | 494 K | Stefansson et al. 2020 |
| 2015 | Transit | K2 | 0.95 m Kepler Telescope | 3.48 day | 4.21 Rearth | — | 447.8 K | ExoFOP |
| 2015 | Transit | K2 | 0.95 m Kepler Telescope | 3.48 day | — | — | — | Kokori et al. 2023 |
| 2015 | Transit | K2 | 0.95 m Kepler Telescope | — | — | — | — | Gaidos et al. 2020 |
| 2015 | Transit | K2 | 0.95 m Kepler Telescope | 3.48 day | 3.45 Rearth | — | — | Thao et al. 2020 |
| 2015 | Transit | K2 | 0.95 m Kepler Telescope | 3.48 day | 3.43 Rearth | — | — | Mann et al. 2016 |
| 2015 | Transit | K2 | 0.95 m Kepler Telescope | 3.48 day | — | — | — | Kokori et al. 2022 |