Kepler-113 is 856 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 4,725 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-113 b goes round its star every 4.75 days, 19 times as often as Mercury goes round the Sun.
| Surface temperature | 4,725 K |
| Mass | 0.75 solar masses |
| Radius | 0.69 solar radii |
| Luminosity | 0.2655 times the Sun |
| Apparent magnitude | 13.655 |
| Age | about 6.89 billion years |
| Distance from the Sun | 855.7 light-years (262.3 parsecs) |
| Position (J2000) | RA 287.9979°, Dec 50.9442° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-113 b | 4.75 days | 0.0512 AU | 1.82 R⊕ | 11.7 M⊕ | Transit, 2014 |
| Kepler-113 c | 8.93 days | 0.0780 AU | 2.18 R⊕ | 8.7 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 4,725 K, 0.27 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.52 to 0.95 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 856 years ago, around 1170.