
TOI-6002 b
Also written TOI-6002b, TOI 6002b, TOI 6002 b
- Mass
- 3.36 × Earth
- Radius
- 1.65 × Earth
- Gravity
- 1.23 g
- Surface (est.)
- 326 K
- Year
- 10.9 days
- From Earth
- 104 ly
- Mass
- 3.36 × Earth
- Radius
- 1.65 × Earth
- Gravity
- 1.23 g
- Surface (est.)
- 326 K
- Year
- 10.9 days
- From Earth
- 104 ly
TOI-6002 system
- Type
- M-type (Red Dwarf)
- Spectral type
- M3.5+/-0.5
- Temperature
- 3,229 K
- Radius
- 0.243 ☉
- Mass
- 0.21 ☉
- Planets
- 1
- Luminosity
- 5.82e-3 ☉
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-6002 b0.057 AUYou are here3.4 M⊕Star and planets drawn to scale: the star is 16 times as wide as TOI-6002 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 rocky world
TOI-6002 b, from the NASA Exoplanet Archive (found 2024). Measured: 3.36 Earth masses, 0.0572 AU, a 3229 K M-type star. Composition inferred from a measured bulk density of 0.75x Earth's, too low for bare rock at this size, suggesting a rocky core under roughly a 0.8% hydrogen/helium envelope by mass, with a day locked to its 10.9-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)


