HATS-30 is 1,116 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this G star; the first was found in 2016 by transit (HATSouth).
Fly there in 3DHATS-30 b goes round its star every 3.17 days, 28 times as often as Mercury goes round the Sun.
HATS-30 is one of 2 stars in its system. The position of the other star is not catalogued, so only HATS-30 and its planets are drawn.
| Spectral type | G |
| Surface temperature | 5,943 K |
| Mass | 1.093 solar masses |
| Radius | 1.061 solar radii |
| Luminosity | 1.25 times the Sun |
| Apparent magnitude | 12.283 |
| Age | about 2.3 billion years |
| Distance from the Sun | 1115.9 light-years (342.1 parsecs) |
| Position (J2000) | RA 5.6185°, Dec -59.9426° |
| Constellation | Tucana |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| HATS-30 b | 3.17 days | 0.0435 AU | 13.171 R⊕ | 224.39 M⊕ | Transit, 2016 |
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 5,943 K, 1.3 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.05 to 1.85 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 1,116 years ago, around AD 910.