
TOI-1422 c
Also written TOI-1422c, TOI 1422c, TOI 1422 c
- Mass
- 14.00 × Earth
- Radius
- 2.61 × Earth
- Gravity
- 2.06 g
- Surface (est.)
- 641 K
- Year
- 34.6 days
- From Earth
- 506 ly
- Mass
- 14.00 × Earth
- Radius
- 2.61 × Earth
- Gravity
- 2.06 g
- Surface (est.)
- 641 K
- Year
- 34.6 days
- From Earth
- 506 ly
TOI-1422 system
- Type
- G-type (Yellow (Sun-like))
- Spectral type
- G2 V
- Temperature
- 5,840 K
- Radius
- 1.02 ☉
- Mass
- 0.99 ☉
- Planets
- 2
- Luminosity
- 1.12 ☉
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.
TOI-1422 c0.20 AUYou are here14 M⊕Star and planets drawn to scale: the star is 43 times as wide as TOI-1422 c, so only its edge is in view. Orbits spaced as in the star system view.
Estimated: this planet doesn't transit its star, so its size is inferred, not measured
TOI-1422 c, from the NASA Exoplanet Archive (found 2025). Measured: 14 Earth masses, 0.205 AU, a 5840 K G-type star. Composition inferred from a estimated bulk density of 0.79x Earth's, modeled rather than measured since this isn't a transiting planet, too low for bare rock at this size, suggesting a rocky core under roughly a 4% hydrogen/helium envelope by mass, with an assumed 24-hour day — rotation cannot be measured for exoplanets.
Surface. No solid surface - a hydrogen-helium envelope wrapped around a rocky core (a sub-Neptune)
Deep hydrogen-helium envelope with photochemical haze
Hydrogen-rich atmosphere typical of gas giants



