TOI-5120 b
Also written TOI-5120b, TOI 5120b, TOI 5120 b
TOI-5120 b is close to a twin of Jupiter in size and mass, about 1.23 times Jupiter's mass and 0.97 times its width, but it circles its star every 24.9 days at 0.17 astronomical units (one astronomical unit is the Earth–Sun distance). NASA's TESS satellite flagged it as a candidate from a regular dip in the starlight, called a transit, as the planet crossed in front of its star. A team led by E. Knudstrup confirmed it in 2026 by measuring the star's slight wobble with two spectrographs, the Tull coudé spectrograph at McDonald Observatory and FIES on the Nordic Optical Telescope, monitoring it from 2022 to 2025. Combining the two methods gives both the planet's size and its mass.
TOI-5120
- Type
- G-type (Yellow (Sun-like))
- Temperature
- 5,763 K
- Radius
- 1.42 ☉
- Mass
- 1.12 ☉
- Known planets
- 1 (this one)
- Luminosity
- 2.17 ☉
Published by the NASA Exoplanet Archive. This world’s temperature and habitability score are computed from this star’s measured luminosity, not from a stand-in for its class.
Gas Giant
Physical Properties
Orbital Environment
Atmosphere
Elemental Composition
Surface Characteristics
No solid surface - thick gaseous envelope with possible rocky core deep withinHow TerraForge built this world
TOI-5120 b, from the NASA Exoplanet Archive (found 2026). Measured: 391 Earth masses, 0.172 AU, a 5763 K G-type star. Composition inferred from a mass of 391 Earths, which is giant territory whatever its 0.30x density suggests, with an assumed 24-hour day — rotation cannot be measured for exoplanets.




