HAT-P-49 is 1,143 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this F3 star; the first was found in 2014 by transit (HATNet).
Fly there in 3DHAT-P-49 b goes round its star every 2.69 days, 33 times as often as Mercury goes round the Sun.
| Spectral type | F3 |
| Surface temperature | 6,820 K |
| Mass | 2.22 solar masses |
| Radius | 2.06 solar radii |
| Luminosity | 6.516 times the Sun |
| Apparent magnitude | 10.205 |
| Age | about 1.5 billion years |
| Distance from the Sun | 1142.7 light-years (350.4 parsecs) |
| Position (J2000) | RA 305.4413°, Dec 26.6927° |
| Constellation | Vulpecula |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| HAT-P-49 b | 2.69 days | 0.0438 AU | 17.822 R⊕ | 699.23 M⊕ | Transit, 2014 |
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 6,820 K, 6.5 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 2.28 to 3.95 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 1,143 years ago, around AD 880.