Distance from Earth: 1,418.8 parsecs (4,627.4 light years)
The transit method detects planets by measuring the periodic dimming of a star's brightness as a planet passes in front of it. NASA's Kepler and TESS missions have used this technique to discover the majority of known exoplanets. The depth of the brightness dip reveals the planet's size relative to its star, while the period between transits gives the orbital period.
Radius
22.31 R⊕
142,137 km
Mass
266.97 M⊕
1.59E27 kg
Orbital Period
8.60 days
0.024 years
Eq. Temperature
1729 K
1456°C
Orbital Semi-major Axis
0.0948 AU
Density
0.13 g/cm³
22.31x Earth
266.97x Earth
0.024x Earth
Star Temperature
6,161 K
Star Radius
3.21 R☉
Star Mass
1.54 M☉
Planets in System
1
Stars in System
1
1729 K is outside the range for liquid water (180-310 K).
22.31 Earth radii suggests a non-rocky composition.
This planet orbits outside the estimated habitable zone of its star.
Habitability assessments are rough estimates based on limited available data. True habitability depends on many additional factors including atmospheric composition, magnetic field presence, tidal locking, and stellar activity. These assessments should not be considered definitive.
Eccentricity
0.1140
Insolation Flux
Unknown
Earth flux = 1.0
6.00x Earth