Kepler-607 is 1,693 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 5,196 K star; the first was found in 2016 by transit (Kepler).
Fly there in 3DKepler-607 b goes round its star every 15.3 hours, 138 times as often as Mercury goes round the Sun.
| Surface temperature | 5,196 K |
| Mass | 0.84 solar masses |
| Radius | 0.8 solar radii |
| Luminosity | 0.415 times the Sun |
| Apparent magnitude | 14.672 |
| Age | about 4.9 billion years |
| Distance from the Sun | 1693.1 light-years (519.1 parsecs) |
| Position (J2000) | RA 291.0571°, Dec 44.6323° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-607 b | 15.3 hours | 0.0137 AU | 0.87 R⊕ | 0.59 M⊕ estimated | Transit, 2016 |
| Kepler-607 c | 39.7 days | 0.215 AU | 2.76 R⊕ | 8.05 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 5,196 K, 0.41 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.63 to 1.14 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 1,693 years ago, around AD 330.