Kepler-375 is 4,041 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 5,826 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-375 b goes round its star every 12.1 days, 7 times as often as Mercury goes round the Sun.
| Surface temperature | 5,826 K |
| Mass | 0.891 solar masses |
| Radius | 0.837 solar radii |
| Luminosity | 0.6874 times the Sun |
| Apparent magnitude | 15.643 |
| Age | about 0.4 billion years |
| Distance from the Sun | 4040.5 light-years (1238.8 parsecs) |
| Position (J2000) | RA 288.6179°, Dec 48.0984° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-375 b | 12.1 days | 0.101 AU | 1.45 R⊕ | 2.7 M⊕ estimated | Transit, 2014 |
| Kepler-375 c | 20.0 days | 0.141 AU | 2.65 R⊕ | 7.51 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 5,826 K, 0.69 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.79 to 1.38 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 4,041 years ago, around 2000 BC.