Kepler-334 is 1,391 light-years from the Sun. The NASA Exoplanet Archive lists 3 planets around this 5,828 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-334 b goes round its star every 5.47 days, 16 times as often as Mercury goes round the Sun.
| Surface temperature | 5,828 K |
| Mass | 1.022 solar masses |
| Radius | 1.068 solar radii |
| Luminosity | 1.136 times the Sun |
| Apparent magnitude | 12.834 |
| Age | about 2.75 billion years |
| Distance from the Sun | 1391.4 light-years (426.6 parsecs) |
| Position (J2000) | RA 287.1406°, Dec 47.1151° |
| Constellation | Lyra |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-334 b | 5.47 days | 0.0610 AU | 1.12 R⊕ | 1.46 M⊕ estimated | Transit, 2014 |
| Kepler-334 c | 12.8 days | 0.107 AU | 1.43 R⊕ | 2.63 M⊕ estimated | Transit, 2014 |
| Kepler-334 d | 25.1 days | 0.168 AU | 1.41 R⊕ | 2.57 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 5,828 K, 1.1 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.01 to 1.78 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 1,391 years ago, around AD 630.