Kepler-370 is 3,809 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 5,852 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-370 b goes round its star every 4.58 days, 19 times as often as Mercury goes round the Sun.
| Surface temperature | 5,852 K |
| Mass | 0.982 solar masses |
| Radius | 0.9 solar radii |
| Luminosity | 1.014 times the Sun |
| Apparent magnitude | 15.467 |
| Age | about 6.03 billion years |
| Distance from the Sun | 3809.3 light-years (1167.9 parsecs) |
| Position (J2000) | RA 292.1711°, Dec 40.9162° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-370 b | 4.58 days | 0.0540 AU | 1.59 R⊕ | 3.15 M⊕ estimated | Transit, 2014 |
| Kepler-370 c | 19.0 days | 0.140 AU | 1.91 R⊕ | 4.31 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 5,852 K, 1.0 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.95 to 1.68 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 3,809 years ago, around 1800 BC.