Kepler-333 is 1,058 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this 4,259 K star; the first was found in 2014 by transit (Kepler).
Fly there in 3DKepler-333 b goes round its star every 12.6 days, 7 times as often as Mercury goes round the Sun.
Kepler-333 is one of 2 stars in its system. The position of the other star is not catalogued, so only Kepler-333 and its planets are drawn.
| Surface temperature | 4,259 K |
| Mass | 0.601 solar masses |
| Radius | 0.534 solar radii |
| Luminosity | 0.118 times the Sun |
| Apparent magnitude | 15.052 |
| Age | about 3.24 billion years |
| Distance from the Sun | 1058.1 light-years (324.4 parsecs) |
| Position (J2000) | RA 292.2861°, Dec 40.9135° |
| Constellation | Cygnus |
| Planet | Year | Orbit | Radius | Mass | Found |
|---|---|---|---|---|---|
| Kepler-333 b | 12.6 days | 0.0870 AU | 1.32 R⊕ | 28.2 M⊕ | Transit, 2014 |
| Kepler-333 c | 24.1 days | 0.135 AU | 1.11 R⊕ | 1.41 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.