Kepler-35 is 5,933 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this 5,606 K star; the first was found in 2011 by transit (Kepler).
Fly there in 3DKepler-35 b takes 131.5 days to go round its star once.
Kepler-35 is one of 2 stars in its system. The position of the other star is not catalogued, so only Kepler-35 and its planets are drawn.
| Surface temperature | 5,606 K |
| Mass | 0.8877 solar masses |
| Radius | 1.0284 solar radii |
| Luminosity | 0.9397 times the Sun |
| Apparent magnitude | 15.863 |
| Distance from the Sun | 5933.3 light-years (1819.2 parsecs) |
| Position (J2000) | RA 294.4970°, Dec 46.6897° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-35 b | 131.5 days | 0.603 AU | 8.16 R⊕ | 40.363 M⊕ | Transit, 2011 |
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 5,606 K, 0.94 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.93 to 1.65 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 5,933 years ago, around 3900 BC.