Kepler-207 is 2,856 light-years from the Sun. The NASA Exoplanet Archive lists 3 planets around this 5,920 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-207 b goes round its star every 38.7 hours, 55 times as often as Mercury goes round the Sun.
| Surface temperature | 5,920 K |
| Mass | 1.313 solar masses |
| Radius | 1.588 solar radii |
| Luminosity | 3.422 times the Sun |
| Apparent magnitude | 13.164 |
| Age | about 3.63 billion years |
| Distance from the Sun | 2855.6 light-years (875.5 parsecs) |
| Position (J2000) | RA 290.0305°, Dec 42.1661° |
| Constellation | Lyra |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-207 b | 38.7 hours | 0.0290 AU | 1.57 R⊕ | 3.09 M⊕ estimated | Transit, 2014 |
| Kepler-207 c | 3.07 days | 0.0440 AU | 1.5 R⊕ | 2.86 M⊕ estimated | Transit, 2014 |
| Kepler-207 d | 5.87 days | 0.0680 AU | 3.31 R⊕ | 11 M⊕ estimated | Transit, 2014 |
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 5,920 K, 3.4 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.74 to 3.06 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 2,856 years ago, around 800 BC.