WASP-167 is 1,381 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this F1 V star; the first was found in 2017 by transit (Multiple Observatories).
Fly there in 3DWASP-167 b goes round its star every 2.02 days, 44 times as often as Mercury goes round the Sun.
| Spectral type | F1 V |
| Surface temperature | 7,000 K |
| Mass | 1.59 solar masses |
| Radius | 1.79 solar radii |
| Luminosity | 7.895 times the Sun |
| Apparent magnitude | 10.517 |
| Age | about 1.29 billion years |
| Distance from the Sun | 1381.4 light-years (423.5 parsecs) |
| Position (J2000) | RA 196.0438°, Dec -35.5495° |
| Constellation | Centaurus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| WASP-167 b | 2.02 days | 0.0365 AU | 17.71 R⊕ | 2542.6 M⊕ | Transit, 2017 |
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 7,000 K, 7.9 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 2.49 to 4.30 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 1,381 years ago, around AD 640.