Kepler-267 is 864 light-years from the Sun. The NASA Exoplanet Archive lists 3 planets around this M1 V star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-267 b goes round its star every 3.35 days, 26 times as often as Mercury goes round the Sun.
| Spectral type | M1 V |
| Surface temperature | 4,258 K |
| Mass | 0.541571 solar masses |
| Radius | 0.555 solar radii |
| Luminosity | 0.059 times the Sun |
| Apparent magnitude | 16.69 |
| Age | about 3.06 billion years |
| Distance from the Sun | 864.3 light-years (265.0 parsecs) |
| Position (J2000) | RA 299.8306°, Dec 47.1576° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-267 b | 3.35 days | 0.0370 AU | 1.98 R⊕ | 37.9 M⊕ | Transit, 2014 |
| Kepler-267 c | 6.88 days | 0.0600 AU | 2.13 R⊕ | 5.18 M⊕ estimated | Transit, 2014 |
| Kepler-267 d | 28.5 days | 0.154 AU | 2.27 R⊕ | 5.77 M⊕ estimated | Transit, 2014 |
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 4,258 K, 0.059 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.25 to 0.46 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 864 years ago, around 1160.