The star
The star
Kepler-148
- Type
- orange dwarf
- Surface
- ≈ 5,272 K
- Size
- 0.85 × the Sun
- Mass
- 0.86 × the Sun
- Brightness
- 0.414 × the Sun
- Habitable zone
- 0.497–1.19 AU
The planets
Kepler-148
Kepler-148 b
- Year
- 1.73 days
- Distance from star
- 0.028 AU
- Mass
- 3.9 Earths
- Size
- 1.8 × Earth
- Temperature
- ≈ 1284 K (+1011 °C)
- Found
- 2014, transit (Kepler)
Kepler-148
Kepler-148 c
- Year
- 4.18 days
- Distance from star
- 0.05 AU
- Mass
- 13 Earths
- Size
- 3.6 × Earth
- Temperature
- ≈ 957 K (+684 °C)
- Found
- 2014, transit (Kepler)
Kepler-148
Kepler-148 d
- Year
- 51.85 days
- Distance from star
- 0.261 AU
- Mass
- 56 Earths
- Size
- 8.7 × Earth
- Temperature
- ≈ 413 K (+140 °C)
- Found
- 2016, transit (Kepler)
Masses found by the wobble method are minimums, because the orbit's tilt is unknown. Temperatures are equilibrium estimates for a bare planet, before any atmosphere.
How we know
The shadow
The planet passes in front of its star and dims it by a fraction of a percent, every orbit. The dip gives the planet's size and year.
Sources
- Planet and star parameters: NASA Exoplanet Archive, Planetary Systems Composite Parameters, retrieved 1 Nov 2026. This research has made use of the NASA Exoplanet Archive, which is operated by the California Institute of Technology, under contract with NASA under the Exoplanet Exploration Program.
- Position: HYG Database v4.1 (CC BY-SA 4.0).
- Habitable zone: a simple estimate from the star's brightness (√L × 0.95 to 1.67 AU), shown as a guide.