HATS-49 is 1,058 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this 4,405 K star; the first was found in 2020 by transit (HATSouth).
Fly there in 3DHATS-49 b goes round its star every 4.15 days, 21 times as often as Mercury goes round the Sun.
| Surface temperature | 4,405 K |
| Mass | 0.7133 solar masses |
| Radius | 0.6977 solar radii |
| Luminosity | 0.1641 times the Sun |
| Apparent magnitude | 14.988 |
| Age | about 10.5 billion years |
| Distance from the Sun | 1058.1 light-years (324.4 parsecs) |
| Position (J2000) | RA 6.6136°, Dec -56.3443° |
| Constellation | Phoenix |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| HATS-49 b | 4.15 days | 0.0452 AU | 8.5749 R⊕ | 112.19 M⊕ | Transit, 2020 |
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 4,405 K, 0.16 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.41 to 0.76 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 1,058 years ago, around AD 970.