Kepler-382 is 3,051 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 5,600 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-382 b goes round its star every 5.26 days, 17 times as often as Mercury goes round the Sun.
| Surface temperature | 5,600 K |
| Mass | 1.002 solar masses |
| Radius | 0.945 solar radii |
| Luminosity | 1.398 times the Sun |
| Apparent magnitude | 14.907 |
| Age | about 7.08 billion years |
| Distance from the Sun | 3051.0 light-years (935.4 parsecs) |
| Position (J2000) | RA 299.1362°, Dec 45.8700° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-382 b | 5.26 days | 0.0550 AU | 1.32 R⊕ | 2.3 M⊕ estimated | Transit, 2014 |
| Kepler-382 c | 12.2 days | 0.0970 AU | 1.59 R⊕ | 3.15 M⊕ estimated | Transit, 2014 |
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.
For a star of 5,600 K, 1.4 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.14 to 2.01 AU. None of its known planets orbits inside it. The zone says how much starlight arrives, not whether a planet has water or air. The edges follow Kopparapu et al. (2014), as the 3D view draws them.
The light you see left 3,051 years ago, around 1000 BC.