The Kepler-62 system contains 5 exoplanets. It is located 981.32 light years away from the solar system.
| Mass | 0.69 solar masses |
| Radius | 0.64 solar radiae |
| Temperature | 4925 kelvin |
| Stellar Metallicity | -0.37 decimal exponent |
| Age | 7 billion years |
At more than 10 Earth masses, Kepler-62 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 | 9.000 Earth masses |
| Density | NaN grams per cubic centimeter |
| Radius | 1.310 Earth radiae |
| Semi-major Axis | 0.0553 AU |
| Eccentricity | 0 |
| Orbital Period | 5.715 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2013-05 |
| Reference | Borucki et al. 2013 |
| Mass | 4.000 Earth masses |
| Density | NaN grams per cubic centimeter |
| Radius | 0.540 Earth radiae |
| Semi-major Axis | 0.0929 AU |
| Eccentricity | 0 |
| Orbital Period | 12.442 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2013-05 |
| Reference | Borucki et al. 2013 |
At more than 10 Earth masses, Kepler-62 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 | 14.000 Earth masses |
| Density | NaN grams per cubic centimeter |
| Radius | 1.950 Earth radiae |
| Semi-major Axis | 0.12 AU |
| Eccentricity | 0 |
| Orbital Period | 18.164 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2013-05 |
| Reference | Borucki et al. 2013 |
At more than 10 Earth masses, Kepler-62 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 | 36.000 Earth masses |
| Density | NaN grams per cubic centimeter |
| Radius | 1.610 Earth radiae |
| Semi-major Axis | 0.427 AU |
| Eccentricity | 0 |
| Orbital Period | 122.387 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2013-05 |
| Reference | Borucki et al. 2013 |
At more than 10 Earth masses, Kepler-62 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 | 35.000 Earth masses |
| Density | NaN grams per cubic centimeter |
| Radius | 1.410 Earth radiae |
| Semi-major Axis | 0.718 AU |
| Eccentricity | 0 |
| Orbital Period | 267.291 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2013-05 |
| Reference | Borucki et al. 2013 |