The Kepler-529 system contains 3 exoplanets. It is located 2606.01 light years away from the solar system.
Mass | 1.07 solar masses |
Radius | 1.14 solar radiae |
Temperature | 6087 kelvin |
Stellar Metallicity | -0.1 decimal exponent |
Age | 3.98 billion years |
At 4.134 Earth masses, Kepler-529 b is a so called Super Earth. Super Earths could be terrestrial worlds like Earth, but they could also be ocean worlds or terrestrial worlds wrapped in a substantial atmosphere, in which case some refer to them as Mini Neptunes.
Mass | 4.120 Earth masses |
Density | 3.520 grams per cubic centimeter |
Radius | 1.860 Earth radiae |
Semi-major Axis | 0.0309 AU |
Eccentricity | 0 |
Orbital Period | 1.980 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 |
With a mass below 5 Earth masses, a density of 3.2, and a semi-major axis of 0.1075 astronomical units, Kepler-529 c could, potentially, be an ocean world - a planet with no dry land.
Mass | 4.660 Earth masses |
Density | 3.200 grams per cubic centimeter |
Radius | 2.000 Earth radiae |
Semi-major Axis | 0.1075 AU |
Eccentricity | 0 |
Orbital Period | 12.835 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-529 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 | 8.220 Earth masses |
Density | 2.070 grams per cubic centimeter |
Radius | 2.795 Earth radiae |
Semi-major Axis | 0.2134 AU |
Eccentricity | 0 |
Orbital Period | 35.866 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 |