The Kepler-175 system contains 2 exoplanets. It is located 4280.28 light years away from the solar system.
| Mass | 1.12 solar masses |
| Radius | 1.01 solar radiae |
| Temperature | 6064 kelvin |
| Stellar Metallicity | 0.1 decimal exponent |
| Age | 3.39 billion years |
At more than 10 Earth masses, Kepler-175 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 | 7.080 Earth masses |
| Density | 2.320 grams per cubic centimeter |
| Radius | 2.560 Earth radiae |
| Semi-major Axis | 0.105 AU |
| Eccentricity | 0 |
| Orbital Period | 11.904 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-175 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 | 9.800 Earth masses |
| Density | 1.810 grams per cubic centimeter |
| Radius | 3.100 Earth radiae |
| Semi-major Axis | 0.213 AU |
| Eccentricity | 0 |
| Orbital Period | 34.035 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 |