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3 known planets · 1,049 light years

Kepler-52

Kepler-52 is a orange dwarf (M0 V) 1,049 light years away, with 3 confirmed planets. Distances and orbital speeds are to scale; the star and planets are enlarged so you can see them.

Day 0
habitable zone (estimate)planet orbits

Green band: where liquid water could exist on a planet's surface. Drag to turn the system, pinch or scroll to zoom.

The star

The star

Kepler-52

Type
M0 V
Surface
≈ 4,075 K
Size
0.52 × the Sun
Mass
0.54 × the Sun
Brightness
0.101 × the Sun
Habitable zone
0.257–0.649 AU

The planets

Kepler-52

Kepler-52 b

Year
7.88 days
Distance from star
0.0637 AU
Mass
1.4e+02 Earths
Size
2.1 × Earth
Temperature
≈ 553 K (+280 °C)
Found
2012, transit (Kepler)
Too hot
Kepler-52

Kepler-52 c

Year
16.39 days
Distance from star
0.104 AU
Mass
45 Earths
Size
1.8 × Earth
Temperature
≈ 433 K (+160 °C)
Found
2012, transit (Kepler)
Too hot
Kepler-52

Kepler-52 d

Year
36.45 days
Distance from star
0.182 AU
Mass
89 Earths
Size
1.9 × Earth
Temperature
≈ 332 K (+59 °C)
Found
2014, transit (Kepler)
Outside the habitable zone

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

  1. 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.
  2. Position: HYG Database v4.1 (CC BY-SA 4.0).
  3. Habitable zone: a simple estimate from the star's brightness (√L × 0.95 to 1.67 AU), shown as a guide.
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