
TOI-406.01
Also written TOI 406.01
- Mass
- 6.57 × Earth
- Radius
- 2.08 × Earth
- Gravity
- 1.52 g
- Surface (est.)
- 370 K
- Year
- 13.2 days
- From Earth
- 101 ly
- Mass
- 6.57 × Earth
- Radius
- 2.08 × Earth
- Gravity
- 1.52 g
- Surface (est.)
- 370 K
- Year
- 13.2 days
- From Earth
- 101 ly
TOI-406 system
- Type
- M-type (Red Dwarf)
- Spectral type
- M3
- Temperature
- 3,392 K
- Radius
- 0.41 ☉
- Mass
- 0.408 ☉
- Planets
- 2
- Luminosity
- 0.0193 ☉
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-406.010.081 AUYou are here6.6 M⊕Star and planets drawn to scale: the star is 22 times as wide as TOI-406.01, 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-406.01, from the NASA Exoplanet Archive (found 2024). Measured: 6.57 Earth masses, 0.0809 AU, a 3392 K M-type star. Composition inferred from a measured bulk density of 0.73x 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 13.2-day year, as anything orbiting this close would be.
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 (partially stripped by slow rotation)



