The star
The star
Kepler-332
- Type
- orange dwarf
- Surface
- ≈ 4,955 K
- Size
- 0.72 × the Sun
- Mass
- 0.74 × the Sun
- Brightness
- 0.261 × the Sun
- Habitable zone
- 0.401–0.971 AU
The planets
Kepler-332
Kepler-332 b
- Year
- 7.63 days
- Distance from star
- 0.07 AU
- Mass
- 1.7 Earths
- Size
- 1.2 × Earth
- Temperature
- ≈ 703 K (+430 °C)
- Found
- 2014, transit (Kepler)
Kepler-332
Kepler-332 c
- Year
- 16.00 days
- Distance from star
- 0.114 AU
- Mass
- 1.3 Earths
- Size
- 1.1 × Earth
- Temperature
- ≈ 550 K (+277 °C)
- Found
- 2014, transit (Kepler)
Kepler-332
Kepler-332 d
- Year
- 34.21 days
- Distance from star
- 0.189 AU
- Mass
- 1.8 Earths
- Size
- 1.2 × Earth
- Temperature
- ≈ 427 K (+154 °C)
- Found
- 2014, 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.