Distance from Earth: 135.0 parsecs (440.3 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⊕
8,766 km
Mass
4.50 M⊕
2.69E25 kg
Orbital Period
0.99 days
0.003 years
Eq. Temperature
1664 K
1391°C
Orbital Semi-major Axis
0.0182 AU
Density
9.30 g/cm³
1.38x Earth
4.50x Earth
0.003x Earth
Star Temperature
5,063 K
Star Radius
0.84 R☉
Star Mass
0.82 M☉
Planets in System
2
Stars in System
1
1664 K is outside the range for liquid water (180-310 K).
1.38 Earth radii suggests a rocky composition.
Receives 1,273.00x 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.
Eccentricity
Unknown
Insolation Flux
1,273.00 S⊕
Earth flux = 1.0
5.78x Earth