
TOI-3714 b
Also written TOI-3714b, TOI 3714b, TOI 3714 b
- Mass
- 222.00 × Earth
- Radius
- 11.30 × Earth
- Gravity
- 1.74 g
- Surface (est.)
- 755 K
- Year
- 2.1 days
- From Earth
- 369 ly
- Mass
- 222.00 × Earth
- Radius
- 11.30 × Earth
- Gravity
- 1.74 g
- Surface (est.)
- 755 K
- Year
- 2.1 days
- From Earth
- 369 ly
TOI-3714 system
- Type
- M-type (Red Dwarf)
- Spectral type
- M2
- Temperature
- 3,660 K
- Radius
- 0.51 ☉
- Mass
- 0.53 ☉
- Planets
- 1
- Luminosity
- 0.0392 ☉
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-3714 b0.027 AUYou are here222 M⊕Star and planets drawn to scale: the star is 4.9 times as wide as TOI-3714 b, so only its edge is in view. Orbits spaced as in the star system view.
TOI-3714 b, from the NASA Exoplanet Archive (found 2022). Measured: 222 Earth masses, 0.027 AU, a 3660 K M-type star. Composition inferred from a mass of 222 Earths, which is giant territory whatever its 0.15x density suggests, with a day locked to its 2.1-day year, as anything orbiting this close would be.
Surface. No solid surface - thick gaseous envelope with possible rocky core deep within
Hydrogen and helium dominated with trace methane and ammonia
Hydrogen-rich atmosphere typical of gas giants


