The Kepler-47 system contains 3 exoplanets. It is located 3343.16 light years away from the solar system.
| Mass | 0.96 solar masses |
| Radius | 0.94 solar radiae |
| Temperature | 5636 kelvin |
| Stellar Metallicity | -0.25 decimal exponent |
| Age | - billion years |
With a mass below 5 Earth masses, a density of 0.4, and a semi-major axis of 0.2877 astronomical units, Kepler-47 b could, potentially, be an ocean world - a planet with no dry land.
| Mass | 2.070 Earth masses |
| Density | 0.400 grams per cubic centimeter |
| Radius | 3.050 Earth radiae |
| Semi-major Axis | 0.2877 AU |
| Eccentricity | 0.021 |
| Orbital Period | 49.464 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2012-09 |
| Reference | Orosz et al. 2012 |
With a mass below 5 Earth masses, a density of 0.17, and a semi-major axis of 0.9638 astronomical units, Kepler-47 c could, potentially, be an ocean world - a planet with no dry land.
| Mass | 3.170 Earth masses |
| Density | 0.170 grams per cubic centimeter |
| Radius | 4.650 Earth radiae |
| Semi-major Axis | 0.9638 AU |
| Eccentricity | 0.044 |
| Orbital Period | 303.227 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2012-09 |
| Reference | Orosz et al. 2012 |
At more than 10 Earth masses, Kepler-47 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 | 19.020 Earth masses |
| Density | 0.300 grams per cubic centimeter |
| Radius | 7.040 Earth radiae |
| Semi-major Axis | 0.6992 AU |
| Eccentricity | 0.024 |
| Orbital Period | 187.366 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2019-05 |
| Reference | Orosz et al. 2019 |