The Kepler-60 system contains 3 exoplanets. It is located 3343.43 light years away from the solar system.
| Mass | 1.04 solar masses |
| Radius | 1.26 solar radiae |
| Temperature | 5905 kelvin |
| Stellar Metallicity | -0.09 decimal exponent |
| Age | 5 billion years |
At 4.191 Earth masses, Kepler-60 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 | 4.190 Earth masses |
| Density | 4.620 grams per cubic centimeter |
| Radius | 1.710 Earth radiae |
| Semi-major Axis | 0.0719 AU |
| Eccentricity | 0 |
| Orbital Period | 7.133 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2013-01 |
| Reference | Steffen et al. 2013 |
With a mass below 5 Earth masses, a density of 3.06, and a semi-major axis of 0.0835 astronomical units, Kepler-60 c could, potentially, be an ocean world - a planet with no dry land.
| Mass | 3.850 Earth masses |
| Density | 3.060 grams per cubic centimeter |
| Radius | 1.900 Earth radiae |
| Semi-major Axis | 0.0835 AU |
| Eccentricity | 0 |
| Orbital Period | 8.919 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2013-01 |
| Reference | Steffen et al. 2013 |
With a mass below 5 Earth masses, a density of 2.91, and a semi-major axis of 0.1012 astronomical units, Kepler-60 d could, potentially, be an ocean world - a planet with no dry land.
| Mass | 4.160 Earth masses |
| Density | 2.910 grams per cubic centimeter |
| Radius | 1.990 Earth radiae |
| Semi-major Axis | 0.1012 AU |
| Eccentricity | 0 |
| Orbital Period | 11.898 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2013-01 |
| Reference | Steffen et al. 2013 |