Kepler-374 is 4,128 light-years from the Sun. The NASA Exoplanet Archive lists 3 planets around this 5,977 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-374 b goes round its star every 45.5 hours, 46 times as often as Mercury goes round the Sun.
| Surface temperature | 5,977 K |
| Mass | 1.033 solar masses |
| Radius | 0.911 solar radii |
| Luminosity | 1.881 times the Sun |
| Apparent magnitude | 14.701 |
| Age | about 8.51 billion years |
| Distance from the Sun | 4127.9 light-years (1265.6 parsecs) |
| Position (J2000) | RA 294.1379°, Dec 42.3704° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-374 b | 45.5 hours | 0.0290 AU | 1.03 R⊕ | 1.08 M⊕ estimated | Transit, 2014 |
| Kepler-374 c | 3.28 days | 0.0420 AU | 1.1 R⊕ | 1.37 M⊕ estimated | Transit, 2014 |
| Kepler-374 d | 5.03 days | 0.0560 AU | 1.31 R⊕ | 2.27 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 5,977 K, 1.9 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.29 to 2.26 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 4,128 years ago, around 2100 BC.