Distance from Earth: 35.7 parsecs (116.4 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
1.38 R⊕
8,805 km
Mass
3.28 M⊕
1.96E25 kg
Orbital Period
2.16 days
0.006 years
Eq. Temperature
796 K
523°C
Orbital Semi-major Axis
0.0266 AU
Density
6.82 g/cm³
Eccentricity
0.0150
Insolation Flux
66.66 S⊕
Earth flux = 1.0
1.38x Earth
3.28x Earth
0.006x Earth
2.76x Earth
Star Temperature
3,664 K
Star Radius
0.54 R☉
Star Mass
0.54 M☉
Planets in System
4
Stars in System
1
796 K is outside the range for liquid water (180-310 K).
1.38 Earth radii suggests a rocky composition.
Receives 66.66x Earth's insolation, outside the habitable zone.
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.