Kepler-616 is 3,085 light-years from the Sun. The NASA Exoplanet Archive lists 3 planets around this 5,753 K star; the first was found in 2016 by transit (Kepler).
Fly there in 3DKepler-616 b goes round its star every 10.00 days, 9 times as often as Mercury goes round the Sun.
| Surface temperature | 5,753 K |
| Mass | 0.98 solar masses |
| Radius | 0.97 solar radii |
| Luminosity | 0.7736 times the Sun |
| Apparent magnitude | 15.021 |
| Age | about 3.89 billion years |
| Distance from the Sun | 3084.7 light-years (945.8 parsecs) |
| Position (J2000) | RA 294.9891°, Dec 46.8383° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-616 b | 10.00 days | 0.0927 AU | 2.43 R⊕ | 6.48 M⊕ estimated | Transit, 2016 |
| Kepler-616 d | 51.1 days | 0.275 AU | 2.653 R⊕ | 7.52 M⊕ estimated | Transit, 2021 |
| Kepler-616 c | 90.4 days | 0.402 AU | 3.41 R⊕ | 11.5 M⊕ estimated | 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 5,753 K, 0.77 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.84 to 1.48 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 3,085 years ago, around 1100 BC.