HATS-36 is 2,793 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this G0 V star; the first was found in 2018 by transit (HATSouth).
Fly there in 3DHATS-36 b goes round its star every 4.18 days, 21 times as often as Mercury goes round the Sun.
| Spectral type | G0 V |
| Surface temperature | 5,950 K |
| Mass | 1.1 solar masses |
| Radius | 1.1 solar radii |
| Luminosity | 1.64 times the Sun |
| Apparent magnitude | 14.364 |
| Age | about 0.62 billion years |
| Distance from the Sun | 2793.3 light-years (856.4 parsecs) |
| Position (J2000) | RA 291.4787°, Dec -23.2028° |
| Constellation | Sagittarius |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| HATS-36 b | 4.18 days | 0.0523 AU | 12.92 R⊕ | 1022.1 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 5,950 K, 1.6 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.20 to 2.12 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 2,793 years ago, around 800 BC.