Kepler-149 is 1,863 light-years from the Sun. The NASA Exoplanet Archive lists 3 planets around this 5,381 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-149 b goes round its star every 29.2 days, 3 times as often as Mercury goes round the Sun.
| Surface temperature | 5,381 K |
| Mass | 1.013 solar masses |
| Radius | 0.953 solar radii |
| Luminosity | 0.7598 times the Sun |
| Apparent magnitude | 14.152 |
| Age | about 14 billion years |
| Distance from the Sun | 1862.5 light-years (571.0 parsecs) |
| Position (J2000) | RA 285.8537°, Dec 38.3841° |
| Constellation | Lyra |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-149 b | 29.2 days | 0.184 AU | 4.21 R⊕ | 16.5 M⊕ estimated | Transit, 2014 |
| Kepler-149 c | 55.3 days | 0.281 AU | 1.61 R⊕ | 3.22 M⊕ estimated | Transit, 2014 |
| Kepler-149 d | 160.0 days | 0.571 AU | 3.96 R⊕ | 14.9 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 5,381 K, 0.76 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.85 to 1.51 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 1,863 years ago, around AD 160.