
TOI-4336 A b
Also written TOI-4336 Ab, TOI 4336 Ab, TOI 4336 A b
- Mass
- 3.33 × Earth
- Radius
- 2.14 × Earth
- Gravity
- 0.73 g
- Surface (est.)
- 314 K
- Year
- 16.3 days
- From Earth
- 73.4 ly
- Mass
- 3.33 × Earth
- Radius
- 2.14 × Earth
- Gravity
- 0.73 g
- Surface (est.)
- 314 K
- Year
- 16.3 days
- From Earth
- 73.4 ly
TOI-4336 A system
- Type
- M-type (Red Dwarf)
- Spectral type
- M3.5 V
- Temperature
- 3,307 K
- Radius
- 0.326 ☉
- Mass
- 0.306 ☉
- Planets
- 2
- Luminosity
- 0.0110 ☉
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-4336 A b0.085 AUYou are here3.3 M⊕Star and planets drawn to scale: the star is 17 times as wide as TOI-4336 A 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-4336 A b, from the NASA Exoplanet Archive (found 2024). Measured: 3.33 Earth masses, 0.0849 AU, a 3307 K M-type star. Composition inferred from a measured bulk density of 0.34x Earth's, too low for bare rock at this size, suggesting a rocky core under roughly a 3% hydrogen/helium envelope by mass, with a day locked to its 16.3-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)



