Kepler-920 is 3,267 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 5,403 K star; the first was found in 2016 by transit (Kepler).
Fly there in 3DKepler-920 b goes round its star every 6.53 days, 13 times as often as Mercury goes round the Sun.
| Surface temperature | 5,403 K |
| Mass | 0.89 solar masses |
| Radius | 0.85 solar radii |
| Luminosity | 0.6563 times the Sun |
| Apparent magnitude | 15.492 |
| Age | about 4.37 billion years |
| Distance from the Sun | 3267.0 light-years (1001.7 parsecs) |
| Position (J2000) | RA 284.2969°, Dec 49.1586° |
| Constellation | Draco |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-920 b | 6.53 days | 0.0650 AU | 2.42 R⊕ | 6.44 M⊕ estimated | Transit, 2016 |
| Kepler-920 c | 100.8 days | 0.403 AU | 3.8 R⊕ | 13.8 M⊕ estimated | Transit, 2016 |
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 5,403 K, 0.66 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.79 to 1.40 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 3,267 years ago, around 1200 BC.