Kepler-365 is 3,389 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 6,012 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-365 b goes round its star every 10.7 days, 8 times as often as Mercury goes round the Sun.
| Surface temperature | 6,012 K |
| Mass | 1.02 solar masses |
| Radius | 1.048 solar radii |
| Luminosity | 1.294 times the Sun |
| Apparent magnitude | 14.771 |
| Age | about 4 billion years |
| Distance from the Sun | 3388.7 light-years (1039.0 parsecs) |
| Position (J2000) | RA 295.6266°, Dec 49.1304° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-365 b | 10.7 days | 0.0980 AU | 2.04 R⊕ | 4.82 M⊕ estimated | Transit, 2014 |
| Kepler-365 c | 17.8 days | 0.137 AU | 1.64 R⊕ | 3.33 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 1.07 to 1.87 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 3,389 years ago, around 1400 BC.