Kepler-435 is 4,627 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this 6,161 K star; the first was found in 2015 by transit (Kepler).
Fly there in 3DKepler-435 b goes round its star every 8.60 days, 10 times as often as Mercury goes round the Sun.
| Surface temperature | 6,161 K |
| Mass | 1.538 solar masses |
| Radius | 3.21 solar radii |
| Luminosity | 13.46 times the Sun |
| Apparent magnitude | 13.704 |
| Age | about 2.25 billion years |
| Distance from the Sun | 4627.4 light-years (1418.8 parsecs) |
| Position (J2000) | RA 292.2873°, Dec 43.1973° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-435 b | 8.60 days | 0.0948 AU | 22.31 R⊕ | 266.97 M⊕ | Transit, 2015 |
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 6,161 K, 13 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 3.41 to 5.95 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 4,627 years ago, around 2600 BC.