The Kepler-134 system contains 2 exoplanets. It is located 1091.96 light years away from the solar system.
| Mass | 1.06 solar masses |
| Radius | 1.18 solar radiae |
| Temperature | 5983 kelvin |
| Stellar Metallicity | -0.207 decimal exponent |
| Age | 3.55 billion years |
With a mass below 5 Earth masses, a density of 3.2, and a semi-major axis of 0.06 astronomical units, Kepler-134 b 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 | 0.06 AU |
| Eccentricity | 0 |
| Orbital Period | 5.317 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2014-03 |
| Reference | Rowe et al. 2014 |
At 2.127 Earth masses, Kepler-134 c 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 | 2.130 Earth masses |
| Density | 5.850 grams per cubic centimeter |
| Radius | 1.260 Earth radiae |
| Semi-major Axis | 0.092 AU |
| Eccentricity | 0 |
| Orbital Period | 10.106 days |
| Discovery Method | Transit |
| Discovery Facility | Kepler |
| Discovery Telescope | 0.95 m Kepler Telescope |
| Discovery Instrument | Kepler CCD Array |
| Discovery Date | 2014-03 |
| Reference | Rowe et al. 2014 |