
TOI-426 b
Also written TOI-426b, TOI 426b, TOI 426 b
- Mass
- 6.70 × Earth
- Radius
- 2.19 × Earth
- Gravity
- 1.40 g
- Surface (est.)
- 1,783 K
- Year
- 31.7 hrs
- From Earth
- 372 ly
- Mass
- 6.70 × Earth
- Radius
- 2.19 × Earth
- Gravity
- 1.40 g
- Surface (est.)
- 1,783 K
- Year
- 31.7 hrs
- From Earth
- 372 ly
TOI-426 system
- Type
- G-type (Yellow (Sun-like))
- Spectral type
- G2 V
- Temperature
- 5,750 K
- Radius
- 0.99 ☉
- Mass
- 1 ☉
- Planets
- 2
- Luminosity
- 0.951 ☉
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.
Star and planets drawn to scale: the star is 49 times as wide as TOI-426 b, so only its edge is in view. Orbits spaced as in the star system view.
Sub-Neptune, likely · its density could also fit a water world
TOI-426 b is an extremely irradiated sub-Neptune, between Earth and Neptune in size, that circles its Sun-like star every 1.32 days and receives about 1,700 times the light Earth gets from the Sun. The star, also known as HD 34390, is about 370 light-years away. The planet is about 2.2 times Earth's width and about 6.7 times its mass.
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 giantsPhysical Properties
Time Dilation
Clocks run 19.7 seconds per year slower than deep space — about 26 minutes over a lifetimeElemental Composition
How TerraForge built this world
TOI-426 b, from the NASA Exoplanet Archive (found 2026). Measured: 6.7 Earth masses, 0.0237 AU, a 5750 K G-type star. Composition inferred from a measured bulk density of 0.64x Earth's, too low for bare rock at this size, suggesting a rocky core under roughly a 2% hydrogen/helium envelope by mass, with a day locked to its 1.3-day year, as anything orbiting this close would be.




