The Kepler-1530 system is known to contain 2 exoplanets in orbit around it. It is located 1597.76 light years away from the solar system.
| Mass | 0.92 solar masses |
| Radius | 0.88 solar radiae |
| Temperature | 5477 kelvin |
| Stellar Metallicity | 0.03 Decimal exponent |
| Age | 4.27 billion years |
At 3.339 Earth masses, Kepler-1530 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. No Super Earths are known to exist in our solar system, but if it exists, the so-called Planet Nine could very well be a super Earth, as it is hypothesized to have a mass between five and ten Earth masses.
| Mass | 3.330 Earth masses |
| Density | 4.150 Grams per cubic centimeter |
| Radius | 1.640 Earth radiae |
| Semi-major Axis | 0.0371 AU |
| Eccentricity | 0 |
| Orbital Period | 2.590 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 3.371 Earth masses, Kepler-1530 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. No Super Earths are known to exist in our solar system, but if it exists, the so-called Planet Nine could very well be a super Earth, as it is hypothesized to have a mass between five and ten Earth masses.
| Mass | 3.360 Earth masses |
| Density | 4.110 Grams per cubic centimeter |
| Radius | 1.650 Earth radiae |
| Semi-major Axis | 0.06 AU |
| Eccentricity | 0 |
| Orbital Period | 5.323 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 |