Kepler-292 is 3,446 light-years from the Sun. The NASA Exoplanet Archive lists 5 planets around this 5,299 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-292 b goes round its star every 2.58 days, 34 times as often as Mercury goes round the Sun.
| Surface temperature | 5,299 K |
| Mass | 0.865 solar masses |
| Radius | 0.826 solar radii |
| Luminosity | 0.4604 times the Sun |
| Apparent magnitude | 16.303 |
| Age | about 5.13 billion years |
| Distance from the Sun | 3445.8 light-years (1056.5 parsecs) |
| Position (J2000) | RA 295.7662°, Dec 42.4243° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-292 b | 2.58 days | 0.0350 AU | 1.32 R⊕ | 2.3 M⊕ estimated | Transit, 2014 |
| Kepler-292 c | 3.72 days | 0.0450 AU | 1.47 R⊕ | 2.76 M⊕ estimated | Transit, 2014 |
| Kepler-292 d | 7.06 days | 0.0680 AU | 2.23 R⊕ | 5.6 M⊕ estimated | Transit, 2014 |
| Kepler-292 e | 12.0 days | 0.0970 AU | 2.67 R⊕ | 7.61 M⊕ estimated | Transit, 2014 |
| Kepler-292 f | 20.8 days | 0.141 AU | 2.35 R⊕ | 6.12 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 5,299 K, 0.46 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.66 to 1.19 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 3,446 years ago, around 1400 BC.