Distance from Earth: 30.5 parsecs (99.5 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
1.67 R⊕
10,652 km
Mass
4.82 M⊕
2.88E25 kg
Orbital Period
11.06 days
0.030 years
Eq. Temperature
326 K
53°C
Orbital Semi-major Axis
0.0610 AU
Density
5.60 g/cm³
1.67x Earth
4.82x Earth
0.030x Earth
Star Temperature
3,185 K
Star Radius
0.28 R☉
Star Mass
0.25 M☉
Planets in System
1
Stars in System
2
326 K is outside the range for liquid water (180-310 K).
1.67 Earth radii suggests a rocky composition.
Receives 1.80x 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
0.0000
Insolation Flux
1.80 S⊕
Earth flux = 1.0
1.13x Earth