WASP-135 is 973 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this G5 V star; the first was found in 2015 by transit (SuperWASP).
Fly there in 3DWASP-135 b goes round its star every 33.6 hours, 63 times as often as Mercury goes round the Sun.
| Spectral type | G5 V |
| Surface temperature | 5,675 K |
| Mass | 0.98 solar masses |
| Radius | 0.96 solar radii |
| Luminosity | 0.4724 times the Sun |
| Apparent magnitude | 13.181 |
| Age | about 0.6 billion years |
| Distance from the Sun | 972.6 light-years (298.2 parsecs) |
| Position (J2000) | RA 267.2849°, Dec 29.8790° |
| Constellation | Hercules |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| WASP-135 b | 33.6 hours | 0.0243 AU | 14.572 R⊕ | 603.88 M⊕ | Transit, 2015 |
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 5,675 K, 0.47 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.66 to 1.16 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 973 years ago, around 1050.