The Kepler-335 system contains 2 exoplanets. It is located 4171.44 light years away from the solar system.
| Mass | 1.03 solar masses |
| Radius | 1.85 solar radiae |
| Temperature | 5877 kelvin |
| Stellar Metallicity | 0.278 decimal exponent |
| Age | 4.37 billion years |
At more than 10 Earth masses, Kepler-335 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 | 11.400 Earth masses |
| Density | 1.610 grams per cubic centimeter |
| Radius | 3.390 Earth radiae |
| Semi-major Axis | 0.075 AU |
| Eccentricity | 0 |
| Orbital Period | 6.562 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-335 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 | 9.640 Earth masses |
| Density | 1.830 grams per cubic centimeter |
| Radius | 3.070 Earth radiae |
| Semi-major Axis | 0.356 AU |
| Eccentricity | 0 |
| Orbital Period | 67.844 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 |