The TOI-1130 system contains 2 exoplanets. It is located 190.02 light years away from the solar system.
| Mass | 0.68 solar masses |
| Radius | 0.69 solar radiae |
| Temperature | 4250 kelvin |
| Stellar Metallicity | 0.2 decimal exponent |
| Age | 8.2 billion years |
At more than 10 Earth masses, TOI-1130 b 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 | 12.900 Earth masses |
| Density | 1.460 grams per cubic centimeter |
| Radius | 3.650 Earth radiae |
| Semi-major Axis | 0.04394 AU |
| Eccentricity | 0.22 |
| Orbital Period | 4.066 days |
| Discovery Method | Transit |
| Discovery Facility | Transiting Exoplanet Survey Satellite (TESS) |
| Discovery Telescope | 0.1 m TESS Telescope |
| Discovery Instrument | TESS CCD Array |
| Discovery Date | 2020-03 |
| Reference | Huang et al. 2020 |
At more than 50 Earth masses, TOI-1130 c is a gas giant, a planet whose mass is mostly made up of hydrogen and helium, like Jupiter and Saturn.
| Mass | 309.566 Earth masses |
| Density | 0.380 grams per cubic centimeter |
| Radius | 16.814 Earth radiae |
| Semi-major Axis | 0.07098 AU |
| Eccentricity | 0.047 |
| Orbital Period | 8.350 days |
| Discovery Method | Transit |
| Discovery Facility | Transiting Exoplanet Survey Satellite (TESS) |
| Discovery Telescope | 0.1 m TESS Telescope |
| Discovery Instrument | TESS CCD Array |
| Discovery Date | 2020-03 |
| Reference | Huang et al. 2020 |