Discovery Method
Transit
Consistent across records
Host star Kepler-78 • 1.20 R⊕ • 0.36 d orbit
Records
8
archive rows
Discovery
2013
Transit
Radius
1.20 R⊕
default parameter set
Mass
1.68 M⊕
default parameter set
Kepler-78
2223 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
Kepler-78
Stable across source rows
Discovery Method
Transit
Consistent across records
Discovery Year
2013
Stable across source rows
Orbital Period
0.36 day
0.35 to 0.36
Semi-Major Axis
9.01e-3 au
single adopted value
Radius
1.20 Rearth
1.12 to 1.23
Mass
1.68 Mearth
1.68 to 8
Density
5.33 g/cm**3
5.26 to 6
Equilibrium Temperature
2223 K
2223 to 2250
Scale Comparison
Current adopted radius: 1.20 R⊕ • circles scaled linearly by radius
Earth
1.0 R⊕ baseline
Kepler-78 b
1.20 R⊕
Jupiter
11.2 R⊕ reference
Provenance
Evidence Summary
Rows
8
Refs
8
Methods
1
| Year | Method | Facility | Telescope | Period | Radius | Mass | Eq. Temp | Reference |
|---|---|---|---|---|---|---|---|---|
| 2013 | Transit | Kepler | 0.95 m Kepler Telescope | 0.36 day | — | — | — | Iglesias-Marzoa et al. 2015 |
| 2013 | Transit | Kepler | 0.95 m Kepler Telescope | 0.36 day | 1.20 Rearth | 1.69 Mearth | — | Howard et al. 2013 |
| 2013 | Transit | Kepler | 0.95 m Kepler Telescope | 0.36 day | 1.16 Rearth | 8 Mearth | — | Sanchis-Ojeda et al. 2013 |
| 2013 | Transit | Kepler | 0.95 m Kepler Telescope | 0.35 day | 1.17 Rearth | 1.86 Mearth | 2250 K | Pepe et al. 2013 |
| 2013 | Transit | Kepler | 0.95 m Kepler Telescope | 0.36 day | 1.20 Rearth | 1.87 Mearth | — | Grunblatt et al. 2015 |
| 2013 | Transit | Kepler | 0.95 m Kepler Telescope | 0.36 day | 1.12 Rearth | 1.97 Mearth | — | Stassun et al. 2017 |
| 2013 | Transit | Kepler | 0.95 m Kepler Telescope | 0.35 day | 1.23 Rearth | 1.77 Mearth | — | Dai et al. 2019 |
| 2013 | Transit | Kepler | 0.95 m Kepler Telescope | 0.36 day | 1.20 Rearth | 1.68 Mearth | 2223 K | Bonomo et al. 2023 |