Kepler-14 is 2,603 light-years from the Sun. The NASA Exoplanet Archive lists 1 planet around this 6,395 K star; the first was found in 2011 by transit (Kepler).
Fly there in 3DKepler-14 b goes round its star every 6.79 days, 13 times as often as Mercury goes round the Sun.
Kepler-14 is one of 2 stars in its system: the other is drawn where the Washington Double Star Catalog measures it on the sky.
| Surface temperature | 6,395 K |
| Mass | 1.512 solar masses |
| Radius | 2.048 solar radii |
| Luminosity | 6.295 times the Sun |
| Apparent magnitude | 12.003 |
| Age | about 2.2 billion years |
| Distance from the Sun | 2602.7 light-years (798.0 parsecs) |
| Position (J2000) | RA 287.7088°, Dec 47.3331° |
| Constellation | Lyra |
Kepler-14 B has no spectral type listed of magnitude 12.8, judged a true companion. In 2017 it was 0.3″ from Kepler-14, at position angle 145° (Washington Double Star Catalog, 19108+4720 KOI 98 AB): 239 AU on the sky at this distance. The true distance can only be larger. Its colour is estimated from its brightness.
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-14 b | 6.79 days | 0.0771 AU | 12.733 R⊕ | 2669.7 M⊕ | Transit, 2011 |
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.