Kepler-433 is 6,126 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this 6,360 K star; the first was found in 2015 by transit (Kepler).
Fly there in 3DKepler-433 b goes round its star every 5.33 days, 16 times as often as Mercury goes round the Sun.
| Surface temperature | 6,360 K |
| Mass | 1.46 solar masses |
| Radius | 2.26 solar radii |
| Luminosity | 7.586 times the Sun |
| Apparent magnitude | 14.717 |
| Age | about 2.67 billion years |
| Distance from the Sun | 6126.2 light-years (1878.3 parsecs) |
| Position (J2000) | RA 297.5936°, Dec 40.9773° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-433 b | 5.33 days | 0.0679 AU | 16.25 R⊕ | 896.24 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 6,360 K, 7.6 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 2.53 to 4.40 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 6,126 years ago, around 4100 BC.