HATS-67 is 3,132 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this 6,594 K star; the first was found in 2018 by transit (HATSouth).
Fly there in 3DHATS-67 b goes round its star every 38.6 hours, 55 times as often as Mercury goes round the Sun.
| Surface temperature | 6,594 K |
| Mass | 1.435 solar masses |
| Radius | 1.441 solar radii |
| Luminosity | 3.52 times the Sun |
| Apparent magnitude | 13.698 |
| Age | about 0.51 billion years |
| Distance from the Sun | 3131.5 light-years (960.1 parsecs) |
| Position (J2000) | RA 180.2088°, Dec -46.1364° |
| Constellation | Centaurus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| HATS-67 b | 38.6 hours | 0.0303 AU | 18.887 R⊕ | 460.85 M⊕ | Transit, 2018 |
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 6,594 K, 3.5 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.70 to 2.95 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 3,132 years ago, around 1100 BC.