Kepler-193 is 3,291 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 6,335 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-193 b goes round its star every 11.4 days, 8 times as often as Mercury goes round the Sun.
| Surface temperature | 6,335 K |
| Mass | 1.051 solar masses |
| Radius | 1.147 solar radii |
| Luminosity | 1.258 times the Sun |
| Apparent magnitude | 14.712 |
| Age | about 0.3 billion years |
| Distance from the Sun | 3291.2 light-years (1009.1 parsecs) |
| Position (J2000) | RA 296.4986°, Dec 46.5772° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-193 b | 11.4 days | 0.106 AU | 2.39 R⊕ | 6.3 M⊕ estimated | Transit, 2014 |
| Kepler-193 c | 50.7 days | 0.286 AU | 2.75 R⊕ | 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 6,335 K, 1.3 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 1.03 to 1.80 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 3,291 years ago, around 1300 BC.