Kepler-313 is 3,521 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 5,727 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-313 b goes round its star every 15.0 days, 6 times as often as Mercury goes round the Sun.
| Surface temperature | 5,727 K |
| Mass | 1.114 solar masses |
| Radius | 1.536 solar radii |
| Luminosity | 2.051 times the Sun |
| Apparent magnitude | 14.304 |
| Age | about 7.08 billion years |
| Distance from the Sun | 3520.5 light-years (1079.4 parsecs) |
| Position (J2000) | RA 298.2949°, Dec 48.7754° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-313 b | 15.0 days | 0.125 AU | 2.53 R⊕ | 6.94 M⊕ estimated | Transit, 2014 |
| Kepler-313 c | 32.3 days | 0.208 AU | 2.57 R⊕ | 7.13 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 5,727 K, 2.1 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.37 to 2.41 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 3,521 years ago, around 1500 BC.