Kepler-175 is 4,280 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 6,064 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-175 b goes round its star every 11.9 days, 7 times as often as Mercury goes round the Sun.
| Surface temperature | 6,064 K |
| Mass | 0.969 solar masses |
| Radius | 1.01 solar radii |
| Luminosity | 1.563 times the Sun |
| Apparent magnitude | 15.225 |
| Age | about 3.39 billion years |
| Distance from the Sun | 4280.3 light-years (1312.3 parsecs) |
| Position (J2000) | RA 289.5532°, Dec 43.8761° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-175 b | 11.9 days | 0.105 AU | 2.56 R⊕ | 7.08 M⊕ estimated | Transit, 2014 |
| Kepler-175 c | 34.0 days | 0.213 AU | 3.1 R⊕ | 9.8 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 6,064 K, 1.6 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.17 to 2.05 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 4,280 years ago, around 2300 BC.