Kepler-192 is 2,126 light-years from the Sun. The NASA Exoplanet Archive lists 3 planets around this 5,479 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-192 d goes round its star every 6.47 days, 14 times as often as Mercury goes round the Sun.
| Surface temperature | 5,479 K |
| Mass | 1.028 solar masses |
| Radius | 1.007 solar radii |
| Luminosity | 0.8048 times the Sun |
| Apparent magnitude | 14.308 |
| Age | about 2.95 billion years |
| Distance from the Sun | 2125.5 light-years (651.7 parsecs) |
| Position (J2000) | RA 287.9179°, Dec 45.5929° |
| Constellation | Lyra |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-192 d | 6.47 days | 0.0686 AU | 1.02 R⊕ | 1.04 M⊕ estimated | Transit, 2016 |
| Kepler-192 b | 9.93 days | 0.0900 AU | 2.74 R⊕ | 7.95 M⊕ estimated | Transit, 2014 |
| Kepler-192 c | 21.2 days | 0.150 AU | 2.79 R⊕ | 8.2 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 5,479 K, 0.80 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.87 to 1.54 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 2,126 years ago, around 100 BC.