Kepler-92 is 1,559 light-years from the Sun. The NASA Exoplanet Archive lists 3 planets around this 5,883 K star; the first was found in 2013 by transit (Kepler).
Fly there in 3DKepler-92 b goes round its star every 13.7 days, 6 times as often as Mercury goes round the Sun.
| Surface temperature | 5,883 K |
| Mass | 1.21 solar masses |
| Radius | 1.7 solar radii |
| Luminosity | 3.616 times the Sun |
| Apparent magnitude | 11.671 |
| Age | about 3.98 billion years |
| Distance from the Sun | 1559.0 light-years (478.0 parsecs) |
| Position (J2000) | RA 289.0861°, Dec 41.5630° |
| Constellation | Lyra |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-92 b | 13.7 days | 0.122 AU | 3.51 R⊕ | 64.3 M⊕ | Transit, 2013 |
| Kepler-92 c | 26.7 days | 0.191 AU | 2.6 R⊕ | 6.1 M⊕ | Transit, 2013 |
| Kepler-92 d | 49.4 days | 0.287 AU | 2.067 R⊕ | 11.867 M⊕ minimum | Transit, 2015 |
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 5,883 K, 3.6 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.80 to 3.16 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 1,559 years ago, around AD 470.