Kepler-1322 is 4,404 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 5,488 K star; the first was found in 2016 by transit (Kepler).
Fly there in 3DKepler-1322 b goes round its star every 23.1 hours, 91 times as often as Mercury goes round the Sun.
| Surface temperature | 5,488 K |
| Mass | 0.9 solar masses |
| Radius | 0.87 solar radii |
| Luminosity | 0.7934 times the Sun |
| Apparent magnitude | 15.876 |
| Age | about 4.47 billion years |
| Distance from the Sun | 4404.2 light-years (1350.3 parsecs) |
| Position (J2000) | RA 293.2045°, Dec 45.4354° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-1322 b | 23.1 hours | 0.0183 AU | 1.61 R⊕ | 3.22 M⊕ estimated | Transit, 2016 |
| Kepler-1322 c | 6.46 days | 0.0652 AU | 2.1549 R⊕ | 5.29 M⊕ estimated | Transit, 2021 |
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 5,488 K, 0.79 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.86 to 1.53 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 4,404 years ago, around 2400 BC.