Kepler-411 is 501 light-years from the Sun. The NASA Exoplanet Archive lists 4 planets around this K2 V star; the first was found in 2013 by transit (Kepler).
Fly there in 3DKepler-411 b goes round its star every 3.01 days, 29 times as often as Mercury goes round the Sun.
Kepler-411 is one of 2 stars in its system. The position of the other star is not catalogued, so only Kepler-411 and its planets are drawn.
| Spectral type | K2 V |
| Surface temperature | 4,974 K |
| Mass | 0.87 solar masses |
| Radius | 0.82 solar radii |
| Luminosity | 0.2636 times the Sun |
| Apparent magnitude | 12.448 |
| Age | about 0.212 billion years |
| Distance from the Sun | 501.2 light-years (153.7 parsecs) |
| Position (J2000) | RA 287.6057°, Dec 49.5234° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-411 b | 3.01 days | 0.0375 AU | 2.401 R⊕ | 25.6 M⊕ | Transit, 2013 |
| Kepler-411 c | 7.83 days | 0.0739 AU | 4.421 R⊕ | 26.4 M⊕ | Transit, 2016 |
| Kepler-411 e | 31.5 days | 0.186 AU | 3.28 R⊕ estimated | 10.8 M⊕ | Transit Timing Variations, 2018 |
| Kepler-411 d | 58.0 days | 0.279 AU | 3.319 R⊕ | 15.2 M⊕ | Transit, 2018 |
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.