Kepler-135 is 2,028 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 6,090 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-135 b goes round its star every 6.00 days, 15 times as often as Mercury goes round the Sun.
| Surface temperature | 6,090 K |
| Mass | 1.047 solar masses |
| Radius | 1.275 solar radii |
| Luminosity | 2.806 times the Sun |
| Apparent magnitude | 12.794 |
| Age | about 2.62 billion years |
| Distance from the Sun | 2028.2 light-years (621.8 parsecs) |
| Position (J2000) | RA 290.4951°, Dec 38.7955° |
| Constellation | Lyra |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-135 b | 6.00 days | 0.0670 AU | 1.81 R⊕ | 3.93 M⊕ estimated | Transit, 2014 |
| Kepler-135 c | 11.4 days | 0.103 AU | 1.16 R⊕ | 1.65 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 6,090 K, 2.8 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.56 to 2.73 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 2,028 years ago, around 100 BC.