Kepler-341 is 3,415 light-years from the Sun. The NASA Exoplanet Archive lists 4 planets around this 6,012 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-341 b goes round its star every 5.20 days, 17 times as often as Mercury goes round the Sun.
| Surface temperature | 6,012 K |
| Mass | 0.976 solar masses |
| Radius | 1.024 solar radii |
| Luminosity | 1.34 times the Sun |
| Apparent magnitude | 14.739 |
| Age | about 9.12 billion years |
| Distance from the Sun | 3415.0 light-years (1047.0 parsecs) |
| Position (J2000) | RA 289.8616°, Dec 43.4727° |
| Constellation | Lyra |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-341 b | 5.20 days | 0.0600 AU | 1.18 R⊕ | 1.76 M⊕ estimated | Transit, 2014 |
| Kepler-341 c | 8.01 days | 0.0800 AU | 1.7 R⊕ | 3.53 M⊕ estimated | Transit, 2014 |
| Kepler-341 d | 27.7 days | 0.182 AU | 1.85 R⊕ | 4.08 M⊕ estimated | Transit, 2014 |
| Kepler-341 e | 42.5 days | 0.242 AU | 1.99 R⊕ | 4.62 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 6,012 K, 1.3 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.08 to 1.90 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 3,415 years ago, around 1400 BC.