Kepler-26 is 1,094 light-years from the Sun. The NASA Exoplanet Archive lists 4 planets around this M0 V star; the first was found in 2011 by transit (Kepler).
Fly there in 3DKepler-26 d goes round its star every 3.54 days, 25 times as often as Mercury goes round the Sun.
| Spectral type | M0 V |
| Surface temperature | 3,914 K |
| Mass | 0.544 solar masses |
| Radius | 0.512 solar radii |
| Luminosity | 0.087 times the Sun |
| Apparent magnitude | 15.853 |
| Age | about 2.95 billion years |
| Distance from the Sun | 1093.6 light-years (335.3 parsecs) |
| Position (J2000) | RA 284.9411°, Dec 46.5665° |
| Constellation | Lyra |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-26 d | 3.54 days | 0.0390 AU | 1.07 R⊕ | 1.24 M⊕ estimated | Transit, 2014 |
| Kepler-26 b | 12.3 days | 0.0855 AU | 2.78 R⊕ | 5.12 M⊕ | Transit, 2011 |
| Kepler-26 c | 17.3 days | 0.107 AU | 2.72 R⊕ | 6.2 M⊕ | Transit, 2011 |
| Kepler-26 e | 46.8 days | 0.220 AU | 2.41 R⊕ | 6.39 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.