Kepler-167 is 1,115 light-years from the Sun. The NASA Exoplanet Archive lists 4 planets around this K4 star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-167 b goes round its star every 4.39 days, 20 times as often as Mercury goes round the Sun.
Kepler-167 is one of 2 stars in its system. The position of the other star is not catalogued, so only Kepler-167 and its planets are drawn.
| Spectral type | K4 |
| Surface temperature | 4,884 K |
| Mass | 0.777 solar masses |
| Radius | 0.749 solar radii |
| Luminosity | 0.289 times the Sun |
| Apparent magnitude | 14.284 |
| Age | about 7.1 billion years |
| Distance from the Sun | 1115.2 light-years (341.9 parsecs) |
| Position (J2000) | RA 292.6585°, Dec 38.3456° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-167 b | 4.39 days | 0.0483 AU | 1.718 R⊕ | 3.6 M⊕ estimated | Transit, 2014 |
| Kepler-167 c | 7.41 days | 0.0684 AU | 1.674 R⊕ | 3.44 M⊕ estimated | Transit, 2014 |
| Kepler-167 d | 21.8 days | 0.140 AU | 1.238 R⊕ | 2.06 M⊕ estimated | Transit, 2016 |
| Kepler-167 e | 2.9 years | 1.883 AU | 10.16 R⊕ | 321.01 M⊕ | 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 4,884 K, 0.29 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.54 to 0.97 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 1,115 years ago, around AD 910.