The Kepler-169 system contains 5 exoplanets. It is located 1325.92 light years away from the solar system.
| Mass | 0.84 solar masses |
| Radius | 0.76 solar radiae |
| Temperature | 4997 kelvin |
| Stellar Metallicity | 0.05 decimal exponent |
| Age | 13.8 billion years |
At 1.507 Earth masses, Kepler-169 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 | 1.510 Earth masses |
| Density | 5.750 grams per cubic centimeter |
| Radius | 1.130 Earth radiae |
| Semi-major Axis | 0.04 AU |
| Eccentricity | 0 |
| Orbital Period | 3.251 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 1.927 Earth masses, Kepler-169 c 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 | 1.920 Earth masses |
| Density | 5.960 grams per cubic centimeter |
| Radius | 1.210 Earth radiae |
| Semi-major Axis | 0.062 AU |
| Eccentricity | 0 |
| Orbital Period | 6.195 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 2.099 Earth masses, Kepler-169 d 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 | 0.075 AU |
| Eccentricity | 0 |
| Orbital Period | 8.348 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-169 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 | 5.480 Earth masses |
| Density | 2.830 grams per cubic centimeter |
| Radius | 2.200 Earth radiae |
| Semi-major Axis | 0.105 AU |
| Eccentricity | 0 |
| Orbital Period | 13.767 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-169 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 | 7.180 Earth masses |
| Density | 2.300 grams per cubic centimeter |
| Radius | 2.580 Earth radiae |
| Semi-major Axis | 0.359 AU |
| Eccentricity | 0 |
| Orbital Period | 87.090 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 |