The Kepler-150 system contains 5 exoplanets. It is located 2906.35 light years away from the solar system.
| Mass | 0.94 solar masses |
| Radius | 0.94 solar radiae |
| Temperature | 5560 kelvin |
| Stellar Metallicity | -0.02 decimal exponent |
| Age | 4.57 billion years |
At 2.099 Earth masses, Kepler-150 b is a so called Super Earth. Super Earths could be terrestrial worlds like Earth, but they could also be ocean worlds or terrestrial worlds wrapped in a substantial atmosphere, in which case some refer to them as Mini Neptunes.
| Mass | 2.100 Earth masses |
| Density | 5.910 grams per cubic centimeter |
| Radius | 1.250 Earth radiae |
| Semi-major Axis | 0.044 AU |
| Eccentricity | 0 |
| Orbital Period | 3.428 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 more than 10 Earth masses, Kepler-150 c 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 | 13.200 Earth masses |
| Density | 1.440 grams per cubic centimeter |
| Radius | 3.690 Earth radiae |
| Semi-major Axis | 0.073 AU |
| Eccentricity | 0 |
| Orbital Period | 7.382 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 more than 10 Earth masses, Kepler-150 d 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 | 8.200 Earth masses |
| Density | 2.070 grams per cubic centimeter |
| Radius | 2.790 Earth radiae |
| Semi-major Axis | 0.104 AU |
| Eccentricity | 0 |
| Orbital Period | 12.561 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 more than 10 Earth masses, Kepler-150 e 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 | 9.910 Earth masses |
| Density | 1.790 grams per cubic centimeter |
| Radius | 3.120 Earth radiae |
| Semi-major Axis | 0.189 AU |
| Eccentricity | 0 |
| Orbital Period | 30.827 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 more than 10 Earth masses, Kepler-150 f 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 | 12.900 Earth masses |
| Density | 1.470 grams per cubic centimeter |
| Radius | 3.640 Earth radiae |
| Semi-major Axis | 1.24 AU |
| Eccentricity | NaN |
| Orbital Period | 637.209 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2017-04 |
| Reference | Schmitt et al. 2017 |