Distance from Earth: 32.8 parsecs (106.8 light years)
The radial velocity (Doppler) method detects the slight wobble a planet induces in its host star as both bodies orbit their common center of mass. By measuring tiny shifts in the star's spectral lines, astronomers can infer the planet's minimum mass and orbital period. This was the first technique to successfully detect exoplanets around Sun-like stars.
Radius
Unknown
Mass
381.39 M⊕
2.28E27 kg
Orbital Period
5,681.00 days
15.554 years
Eq. Temperature
Unknown
Orbital Semi-major Axis
6.1100 AU
Density
Unknown
381.39x Earth
15.55x Earth
Star Temperature
5,419 K
Star Radius
--
Star Mass
0.94 M☉
Planets in System
1
Stars in System
1
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
0.4200
Insolation Flux
Unknown
Earth flux = 1.0