Kepler-913 is 3,234 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 4,687 K star; the first was found in 2016 by transit (Kepler).
Fly there in 3DKepler-913 c goes round its star every 5.94 days, 15 times as often as Mercury goes round the Sun.
| Surface temperature | 4,687 K |
| Mass | 0.63 solar masses |
| Radius | 0.61 solar radii |
| Luminosity | 0.5228 times the Sun |
| Apparent magnitude | 15.522 |
| Age | about 5.62 billion years |
| Distance from the Sun | 3234.2 light-years (991.6 parsecs) |
| Position (J2000) | RA 297.5831°, Dec 41.9524° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-913 c | 5.94 days | 0.0699 AU | 3.8581 R⊕ | 14.2 M⊕ estimated | Transit, 2021 |
| Kepler-913 b | 10.3 days | 0.101 AU | 2.06 R⊕ | 4.9 M⊕ estimated | Transit, 2016 |
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 4,687 K, 0.52 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.73 to 1.33 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 3,234 years ago, around 1200 BC.