Kepler-49 is 1,015 light-years from the Sun. The NASA Exoplanet Archive lists 4 planets around this M1 V star; the first was found in 2012 by transit (Kepler).
Fly there in 3DKepler-49 d goes round its star every 2.58 days, 34 times as often as Mercury goes round the Sun.
| Spectral type | M1 V |
| Surface temperature | 4,096 K |
| Mass | 0.607 solar masses |
| Radius | 0.618 solar radii |
| Luminosity | 0.074 times the Sun |
| Apparent magnitude | 15.655 |
| Age | about 2.88 billion years |
| Distance from the Sun | 1015.1 light-years (311.2 parsecs) |
| Position (J2000) | RA 292.2945°, Dec 40.5918° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-49 d | 2.58 days | 0.0310 AU | 1.6 R⊕ | 235.98 M⊕ | Transit, 2014 |
| Kepler-49 b | 7.20 days | 0.0593 AU | 2.579 R⊕ | 9.77 M⊕ | Transit, 2012 |
| Kepler-49 c | 10.9 days | 0.0782 AU | 2.444 R⊕ | 8.38 M⊕ | Transit, 2012 |
| Kepler-49 e | 18.6 days | 0.116 AU | 1.56 R⊕ | 1.0381 M⊕ | 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.