HATS-24 is 1,612 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this F V star; the first was found in 2017 by transit (HATSouth).
Fly there in 3DHATS-24 b goes round its star every 32.4 hours, 65 times as often as Mercury goes round the Sun.
| Spectral type | F V |
| Surface temperature | 6,125 K |
| Mass | 1.07 solar masses |
| Radius | 1.12 solar radii |
| Luminosity | 1.549 times the Sun |
| Apparent magnitude | 12.915 |
| Age | about 3.7 billion years |
| Distance from the Sun | 1611.8 light-years (494.2 parsecs) |
| Position (J2000) | RA 268.8907°, Dec -61.7474° |
| Constellation | Pavo |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| HATS-24 b | 32.4 hours | 0.0238 AU | 15.637 R⊕ | 718.3 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 6,125 K, 1.5 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.16 to 2.03 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 1,612 years ago, around AD 410.