Kepler-32 is 1,056 light-years from the Sun. The NASA Exoplanet Archive lists 5 planets around this M1 V star; the first was found in 2011 by transit (Kepler).
Fly there in 3DKepler-32 f goes round its star every 17.8 hours, 118 times as often as Mercury goes round the Sun.
| Spectral type | M1 V |
| Surface temperature | 3,900 K |
| Mass | 0.58 solar masses |
| Radius | 0.53 solar radii |
| Luminosity | 0.051 times the Sun |
| Apparent magnitude | 16.36 |
| Age | about 5.6 billion years |
| Distance from the Sun | 1056.2 light-years (323.8 parsecs) |
| Position (J2000) | RA 297.8423°, Dec 46.5744° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-32 f | 17.8 hours | 0.0130 AU | 0.82 R⊕ | 1862.1 M⊕ | Transit, 2012 |
| Kepler-32 e | 2.90 days | 0.0330 AU | 1.5 R⊕ | 4.0818 M⊕ | Transit, 2012 |
| Kepler-32 b | 5.90 days | 0.0500 AU | 2.2 R⊕ | 1303 M⊕ | Transit, 2011 |
| Kepler-32 c | 8.75 days | 0.0900 AU | 2 R⊕ | 158.9 M⊕ | Transit, 2011 |
| Kepler-32 d | 22.8 days | 0.130 AU | 2.7 R⊕ | 39.909 M⊕ | Transit, 2012 |
Values are the NASA Exoplanet Archive’s composite parameters. A radius marked estimated comes from a mass–radius relation; a mass marked minimum is M sin i. Planet sizes and colours in the 3D view are renderings: none of these worlds has been photographed as more than a point of light.