The star
The star
Kepler-725
- Type
- G
- Surface
- ≈ 5,395 K
- Size
- 0.88 × the Sun
- Mass
- 0.95 × the Sun
- Brightness
- 0.486 × the Sun
- Habitable zone
- 0.535–1.28 AU
The planets
Kepler-725
Kepler-725 b
- Year
- 39.64 days
- Distance from star
- 0.224 AU
- Mass
- 1.6 Jupiters
- Size
- 11 × Earth
- Temperature
- ≈ 514 K (+241 °C)
- Found
- 2016, transit (Kepler)
Kepler-725
Kepler-725 c
- Year
- 207.54 days
- Distance from star
- 0.674 AU
- Mass
- 9.7 Earths
- Size
- 3.1 × Earth
- Temperature
- ≈ 268 K (-5 °C)
- Found
- 2025, transit timing variations (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.
Early and late
A known planet arrives early or late for its transits, betraying the pull of another, unseen planet.
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.