The Kepler-119 system contains 2 exoplanets. It is located 2289.60 light years away from the solar system.
| Mass | 0.92 solar masses |
| Radius | 0.84 solar radiae |
| Temperature | 5595 kelvin |
| Stellar Metallicity | 0.01 decimal exponent |
| Age | 3.63 billion years |
At more than 10 Earth masses, Kepler-119 b is an ice giant, a planet that is made up mostly of volatiles like water, amonia and methane, and enveloped by a dense hydrogen and helium atmosphere, much like Uranus and Neptune.
| Mass | 12.600 Earth masses |
| Density | 1.480 grams per cubic centimeter |
| Radius | 3.600 Earth radiae |
| Semi-major Axis | 0.035 AU |
| Eccentricity | 0 |
| Orbital Period | 2.422 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2014-03 |
| Reference | Rowe et al. 2014 |
At less than 1.5 Earth masses, Kepler-119 c is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
| Mass | 0.721 Earth masses |
| Density | 5.090 grams per cubic centimeter |
| Radius | 0.920 Earth radiae |
| Semi-major Axis | 0.049 AU |
| Eccentricity | 0 |
| Orbital Period | 4.125 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2014-03 |
| Reference | Rowe et al. 2014 |