Kepler-413 is 2,764 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this 4,700 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-413 b goes round its star every 66.3 days, 1.3 times as often as Mercury goes round the Sun.
Kepler-413 is one of 2 stars in its system. The position of the other star is not catalogued, so only Kepler-413 and its planets are drawn.
| Surface temperature | 4,700 K |
| Mass | 0.82 solar masses |
| Radius | 0.7761 solar radii |
| Luminosity | 0.3716 times the Sun |
| Apparent magnitude | 15.885 |
| Distance from the Sun | 2764.3 light-years (847.5 parsecs) |
| Position (J2000) | RA 288.5107°, Dec 51.1624° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-413 b | 66.3 days | 0.355 AU | 4.347 R⊕ | 67 M⊕ | 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 4,700 K, 0.37 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.61 to 1.12 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 2,764 years ago, around 700 BC.