Kepler-385 is 4,673 light-years from the Sun. The NASA Exoplanet Archive lists 3 planets around this 6,326 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-385 b goes round its star every 10.0 days, 9 times as often as Mercury goes round the Sun.
| Surface temperature | 6,326 K |
| Mass | 0.992 solar masses |
| Radius | 1.126 solar radii |
| Luminosity | 1.392 times the Sun |
| Apparent magnitude | 15.76 |
| Age | about 3.31 billion years |
| Distance from the Sun | 4672.5 light-years (1432.6 parsecs) |
| Position (J2000) | RA 294.3385°, Dec 50.3365° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-385 b | 10.0 days | 0.0970 AU | 2.73 R⊕ | 12.8 M⊕ | Transit, 2014 |
| Kepler-385 c | 15.2 days | 0.127 AU | 3.04 R⊕ | 13.2 M⊕ | Transit, 2014 |
| Kepler-385 d | 56.4 days | 0.287 AU | 2.6186 R⊕ | 7.36 M⊕ estimated | Transit, 2020 |
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.