Kepler-619 is 2,938 light-years from the Sun. The NASA Exoplanet Archive lists 3 planets around this 5,980 K star; the first was found in 2016 by transit (Kepler).
Fly there in 3DKepler-619 c goes round its star every 29.0 hours, 73 times as often as Mercury goes round the Sun.
| Surface temperature | 5,980 K |
| Mass | 1.09 solar masses |
| Radius | 1.11 solar radii |
| Luminosity | 0.912 times the Sun |
| Apparent magnitude | 14.84 |
| Age | about 3.47 billion years |
| Distance from the Sun | 2937.6 light-years (900.7 parsecs) |
| Position (J2000) | RA 290.8491°, Dec 48.4160° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-619 c | 29.0 hours | 0.0222 AU | 1.69 R⊕ | 3.5 M⊕ estimated | Transit, 2016 |
| Kepler-619 b | 5.40 days | 0.0601 AU | 3.16 R⊕ | 10.1 M⊕ estimated | Transit, 2016 |
| Kepler-619 d | 11.7 days | 0.102 AU | 4.17 R⊕ | 16.2 M⊕ estimated | Transit, 2023 |
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 5,980 K, 0.91 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.90 to 1.57 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 2,938 years ago, around 900 BC.