Kepler-610 is 2,759 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 5,943 K star; the first was found in 2016 by transit (Kepler).
Fly there in 3DKepler-610 b goes round its star every 7.00 days, 13 times as often as Mercury goes round the Sun.
| Surface temperature | 5,943 K |
| Mass | 1.1 solar masses |
| Radius | 1.13 solar radii |
| Luminosity | 0.7756 times the Sun |
| Apparent magnitude | 14.816 |
| Age | about 3.55 billion years |
| Distance from the Sun | 2758.7 light-years (845.8 parsecs) |
| Position (J2000) | RA 293.1713°, Dec 45.0656° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-610 b | 7.00 days | 0.0719 AU | 4.19 R⊕ | 16.3 M⊕ estimated | Transit, 2016 |
| Kepler-610 c | 151.9 days | 0.559 AU | 3.3 R⊕ | 10.9 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 5,943 K, 0.78 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.83 to 1.46 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 2,759 years ago, around 700 BC.