The Kepler-616 system contains 3 exoplanets. It is located 3084.70 light years away from the solar system.
Mass | 0.98 solar masses |
Radius | 0.97 solar radiae |
Temperature | 5753 kelvin |
Stellar Metallicity | -0.02 decimal exponent |
Age | 3.89 billion years |
At more than 10 Earth masses, Kepler-616 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 | 6.480 Earth masses |
Density | 2.480 grams per cubic centimeter |
Radius | 2.430 Earth radiae |
Semi-major Axis | 0.0927 AU |
Eccentricity | 0 |
Orbital Period | 9.998 days |
Discovery Method | Transit |
Discovery Facility | Kepler |
Discovery Telescope | 0.95 m Kepler Telescope |
Discovery Instrument | Kepler CCD Array |
Discovery Date | 2016-05 |
Reference | Morton et al. 2016 |
At more than 10 Earth masses, Kepler-616 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 | 11.500 Earth masses |
Density | 1.590 grams per cubic centimeter |
Radius | 3.410 Earth radiae |
Semi-major Axis | 0.4024 AU |
Eccentricity | 0 |
Orbital Period | 90.411 days |
Discovery Method | Transit |
Discovery Facility | Kepler |
Discovery Telescope | 0.95 m Kepler Telescope |
Discovery Instrument | Kepler CCD Array |
Discovery Date | 2016-05 |
Reference | Morton et al. 2016 |
At more than 10 Earth masses, Kepler-616 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 | 7.520 Earth masses |
Density | 2.210 grams per cubic centimeter |
Radius | 2.653 Earth radiae |
Semi-major Axis | 0.2749 AU |
Eccentricity | 0 |
Orbital Period | 51.067 days |
Discovery Method | Transit |
Discovery Facility | Kepler |
Discovery Telescope | 0.95 m Kepler Telescope |
Discovery Instrument | Kepler CCD Array |
Discovery Date | 2022-02 |
Reference | Valizadegan et al. 2022 |