The Kepler-1130 system contains 3 exoplanets. It is located 813.25 light years away from the solar system.
| Mass | 0.9 solar masses |
| Radius | 0.81 solar radiae |
| Temperature | 5403 kelvin |
| Stellar Metallicity | -0.06 decimal exponent |
| Age | 1.58 billion years |
At less than 1.5 Earth masses, Kepler-1130 b is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
| Mass | 0.437 Earth masses |
| Density | 4.690 grams per cubic centimeter |
| Radius | 0.800 Earth radiae |
| Semi-major Axis | 0.0595 AU |
| Eccentricity | 0 |
| Orbital Period | 5.453 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 less than 1.5 Earth masses, Kepler-1130 c is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
| Mass | 0.422 Earth masses |
| Density | 4.660 grams per cubic centimeter |
| Radius | 0.792 Earth radiae |
| Semi-major Axis | 0.0423 AU |
| Eccentricity | 0 |
| Orbital Period | 3.267 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 |
At less than 1.5 Earth masses, Kepler-1130 d is a terrestrial planet, much like the terrestrial planets we find in our solar system, namely Mercury, Venus, Earth and Mars.
| Mass | 0.202 Earth masses |
| Density | 4.140 grams per cubic centimeter |
| Radius | 0.645 Earth radiae |
| Semi-major Axis | 0.0506 AU |
| Eccentricity | 0 |
| Orbital Period | 4.272 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 |