Discovery Method
Transit
Consistent across records
Host star K2-110 • 2.59 R⊕ • 13.86 d orbit
Records
9
archive rows
Discovery
2017
Transit
Radius
2.59 R⊕
default parameter set
Mass
15.90 M⊕
default parameter set
K2-110
638 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
K2-110
Stable across source rows
Discovery Method
Transit
Consistent across records
Discovery Year
2017
Stable across source rows
Orbital Period
13.86 day
13.86 to 13.86
Semi-Major Axis
0.10 au
0.10 to 0.10
Radius
2.59 Rearth
2.50 to 2.59
Mass
15.90 Mearth
15.90 to 17
Density
5.02 g/cm**3
5.02 to 5.70
Equilibrium Temperature
638 K
571 to 640
Scale Comparison
Current adopted radius: 2.59 R⊕ • circles scaled linearly by radius
Earth
1.0 R⊕ baseline
K2-110 b
2.59 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 |
|---|---|---|---|---|---|---|---|---|
| 2017 | Transit | K2 | 0.95 m Kepler Telescope | 13.86 day | 2.50 Rearth | — | — | Petigura et al. 2018 |
| 2017 | Transit | K2 | 0.95 m Kepler Telescope | 13.86 day | 2.55 Rearth | — | — | Kruse et al. 2019 |
| 2017 | Transit | K2 | 0.95 m Kepler Telescope | 13.86 day | 2.56 Rearth | 17 Mearth | 571 K | Howard et al. 2025 |
| 2017 | Transit | K2 | 0.95 m Kepler Telescope | 13.86 day | — | — | — | Barros et al. 2016 |
| 2017 | Transit | K2 | 0.95 m Kepler Telescope | 13.86 day | — | — | — | Pope et al. 2016 |
| 2017 | Transit | K2 | 0.95 m Kepler Telescope | 13.86 day | 2.59 Rearth | 15.90 Mearth | 638 K | Bonomo et al. 2023 |
| 2017 | Transit | K2 | 0.95 m Kepler Telescope | 13.86 day | 2.52 Rearth | — | — | Mayo et al. 2018 |
| 2017 | Transit | K2 | 0.95 m Kepler Telescope | 13.86 day | 2.56 Rearth | — | 575 K | Livingston et al. 2018 |
| 2017 | Transit | K2 | 0.95 m Kepler Telescope | 13.86 day | 2.59 Rearth | 16.70 Mearth | 640 K | Osborn et al. 2017 |