Kepler-82 is 2,950 light-years from the Sun. The NASA Exoplanet Archive lists 5 planets around this G star; the first was found in 2012 by transit (Kepler).
Fly there in 3DKepler-82 d goes round its star every 2.38 days, 37 times as often as Mercury goes round the Sun.
| Spectral type | G |
| Surface temperature | 5,401 K |
| Mass | 0.91 solar masses |
| Radius | 0.898 solar radii |
| Luminosity | 0.653 times the Sun |
| Apparent magnitude | 15.131 |
| Age | about 1.41 billion years |
| Distance from the Sun | 2949.5 light-years (904.3 parsecs) |
| Position (J2000) | RA 292.8734°, Dec 42.9662° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-82 d | 2.38 days | 0.0340 AU | 1.77 R⊕ | 885.1 M⊕ | Transit, 2014 |
| Kepler-82 e | 5.90 days | 0.0630 AU | 2.47 R⊕ | 254.02 M⊕ | Transit, 2014 |
| Kepler-82 b | 26.4 days | 0.168 AU | 4.07 R⊕ | 12.15 M⊕ | Transit, 2012 |
| Kepler-82 c | 51.5 days | 0.263 AU | 5.34 R⊕ | 13.9 M⊕ | Transit, 2012 |
| Kepler-82 f | 75.7 days | 0.340 AU | 4.84 R⊕ estimated | 20.9 M⊕ | Transit Timing Variations, 2019 |
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.